0000000000443443

AUTHOR

J. Ahrens

showing 144 related works from this author

Negative Ionen und ihre Bedeutung für die Restgasanalyse

1965

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Photoproduction of neutral pion pairs from the proton

2000

Double neutral pion photoproduction from the proton has been measured at MAMI for photon energies between threshold and 820 MeV. The reaction was identified by an invariant mass and missing mass analysis. From threshold up to 370 MeV the total cross-section does not exceed 30 nb. For higher energies it shows a smooth rise until it reaches a maximum of about 10 μb at Eγ = 740 MeV. Dalitz plots of m2(π0π0) versusm2(p,π0) for seven bins of incident photon energy have been analysed. For Eγ > 610 MeV, a strong contribution of a sequential decay is observed with the Δ(1232)-resonance as intermediate state. A comparison to model calculations shows that these sequential decays presumably originate …

PhysicsNuclear and High Energy PhysicsPhotonProton010308 nuclear & particles physicsNuclear TheoryHadronResonanceDalitz plotPhoton energy7. Clean energy01 natural sciencesNuclear physicsPion0103 physical sciencesInvariant massAtomic physicsNuclear Experiment010306 general physicsThe European Physical Journal A
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Compton scattering from the free and bound proton at backward angles above π-threshold

1999

Differential cross sections for Compton scattering from the free proton at Theta(gamma)(lab) = 130.7 degrees in the energy region from 200 MeV to 410 MeV and far quasi-free Compton scattering from the proton bound in the deuteron at Theta(gamma)(lab) = 148.8 degrees in the energy region from 200 MeV to 290 MeV have been measured. The free proton data are in agreement with dispersion-theory predictions based on standard parameters. The difference of the proton polarizabilities has been extracted from the quasi-free data. Our result, - = [9.1 +/- 1.7(stat + syst) +/- 1.2(mod)] x 10(-4) fm(3), is in reasonable agreement with the world average of the free proton data if the backward spin polari…

PhysicsNuclear and High Energy PhysicsBackscatterProton010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryCompton scattering01 natural sciencesNuclear physicsDeuteriumPolarizabilityDispersion relation0103 physical sciencesNeutronAtomic physicsNuclear Experiment010306 general physicsSpin-½
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Abstracts from the sixth meeting of the international association of pancreatology, November 2–4, 1994, Chicago, IL

1994

medicine.medical_specialtyEndocrinologyOncologybusiness.industryFamily medicineGastroenterologymedicinebusinessInternational journal of pancreatology
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Test of Low-Energy Theorems forH1(γ→,π0)H1in the Threshold Region

2001

The photon asymmetry in the reaction H-1(, pi (0))H-1 close to threshold has been measured for the first time with the photon spectrometer TAPS using linearly polarized photons from the tagged-photon facility at the Mainz Microtron MAMI. The total and differential cross sections were also measured simultaneously with the photon asymmetry. This allowed determination of the S-wave and all three P-wave amplitudes. The values obtained at threshold are E0+ = [-1.33 +/- 0.08(stat) +/- 0.03(syst)] x 10(-3)/m(pi+), P-1 = [9.47 +/- 0.08(stat) +/- 0.29(syst)] x 10(-3)q /m(pi+)(2) P-2 [-9.46 +/- 0.1(stat) +/- 0.29(syst)] x 10(-3)q/m(pi+)(2), and P-3 = [11.48 +/- 0.06(stat) +/- 0.35(syst)] x 10(-3)q/m(…

PhysicsPhotonLow energy010308 nuclear & particles physics0103 physical sciencesPiAnalytical chemistryGeneral Physics and Astronomy010306 general physics01 natural sciencesNuclear theoryMicrotronPhysical Review Letters
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Compton Scattering by the Proton

2001

Compton scattering by the proton has been measured over a wide range covering photon energies 250 MeV < E_\gamma < 800 MeV and photon scattering angles 30^0 < \theta^{lab}_\gamma < 150^0, using the tagged-photon facility at MAMI (Mainz) and the large-acceptance arrangement LARA. The data are in good agreement with the dispersion theory based on the SAID-SM99K parameterization of photo-meson amplitudes. From the subset of data between 280 and 360 MeV the resonance pion-photoproduction amplitudes were evaluated leading to the multipole E2/M1 ratio EMR(340 MeV) =(-1.6 \pm 0.4(stat+syst) \pm 0.2(model)%. From all data below 455 MeV the proton's backward spin polarizability was determined to be …

PhysicsNuclear and High Energy PhysicsPhotonProton010308 nuclear & particles physicsNuclear TheoryCompton scatteringFOS: Physical sciences7. Clean energy01 natural sciencesResonance (particle physics)Scattering amplitudeNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Polarizability0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)010306 general physicsMultipole expansionNuclear ExperimentNuclear ExperimentSpin-½
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Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector

2007

The IceCube neutrino detector is a cubic kilometer TeV to PeV neutrino detector under construction at the geographic South Pole. The dominant population of neutrinos detected in IceCube is due to meson decay in cosmic-ray air showers. These atmospheric neutrinos are relatively well understood and serve as a calibration and verification tool for the new detector. In 2006, the detector was approximately 10% completed, and we report on data acquired from the detector in this configuration. We observe an atmospheric neutrino signal consistent with expectations, demonstrating that the IceCube detector is capable of identifying neutrino events. In the first 137.4 days of live time, 234 neutrino c…

PhysicsNuclear and High Energy PhysicsParticle physicseducation.field_of_studyPhysics::Instrumentation and DetectorsPhysicsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaPopulationDetectorAstrophysics (astro-ph)High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesSolar neutrino problemAstrophysicsNeutrino detectorAstronomiaMeasurements of neutrino speedddc:530High Energy Physics::ExperimentNeutrino astronomyNeutrinoeducation
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Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector

2002

A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of the Earth has been performed with the AMANDA-B10 neutrino detector. The data sample collected in 130.1 days of live-time in 1997, ~10^9 events, has been analyzed for this search. No excess over the expected atmospheric neutrino background is oberved. An upper limit at 90% confidence level on the annihilation rate of neutralinos in the center of the Earth is obtained as a function of the neutralino mass in the range 100 GeV-5000 GeV, as well as the corresponding muon flux limit.

PhysicsNuclear and High Energy PhysicsParticle physicsAnnihilationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterDetectorAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryAstrophysicsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Neutrino detectorWIMPNeutralinoHigh Energy Physics::Experimentddc:530Neutrino oscillation
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Double pi(0) photoproduction off the proton at threshold

2003

The reaction $\gamma p \to \pi^0 \pi^0 p$ has been measured using the TAPS BaF$_2$ calorimeter at the tagged photon facility of the Mainz Microtron accelerator. Chiral perturbation theory (ChPT) predicts that close to threshold this channel is significantly enhanced compared to double pion final states with charged pions. In contrast to other reaction channels, the lower order tree terms are strongly suppressed in 2$\pi^0$ photoproduction. The consequence is the dominance of pion loops in the 2$\pi^0$ channel close to threshold - a result that opens new prospects for the test of ChPT and in particular its inherent loop terms. The present measurement is the first which is sensitive enough fo…

PhysicsTAPSNuclear and High Energy PhysicsParticle physicsChiral perturbation theoryMesonProtonNuclear TheoryHigh Energy Physics::LatticeNEUTRAL-PION-PHOTOPRODUCTIONHadronNuclear TheoryElementary particleCHIRAL PERTURBATION-THEORYNuclear physicsPionTAGGED PHOTON SPECTROMETERNucleonNuclear ExperimentMicrotronNuclear Experiment
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Determination of theE2/M1ratio in theγN→Δ(1232)transition from a simultaneous measurement ofp(γ→,p)π0andp(γ→,π+)n

2000

Tagged linearly polarized photons have been used at the Mainz Microtron (MAMI) for simultaneous measurements of the $p(\stackrel{\ensuremath{\rightarrow}}{\ensuremath{\gamma}},p){\ensuremath{\pi}}^{0}$ and $p(\stackrel{\ensuremath{\rightarrow}}{\ensuremath{\gamma}},{\ensuremath{\pi}}^{+})n$ reaction channels to study the $\ensuremath{\gamma}\stackrel{\ensuremath{\rightarrow}}{N}\ensuremath{\Delta}(1232)$ transition. The energy dependence of the magnetic dipole ${M}_{1+}^{3/2}$ and electric quadrupole ${E}_{1+}^{3/2}$ amplitudes have been extracted from these data in the photon energy range from $270$ to 420 MeV. The $E2/M1$ ratio for the $\ensuremath{\gamma}\stackrel{\ensuremath{\rightarrow…

PhysicsNuclear and High Energy PhysicsParticle physicsMeson productionHigh Energy Physics::PhenomenologyResonancePhoton energyAngular distributionQuadrupolePiAtomic physicsNuclear ExperimentNuclear theoryEnergy (signal processing)Physical Review C
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Calibration and survey of AMANDA with the SPASE detectors

2004

We report on the analysis of air showers observed in coincidence by the Antarctic Muon and Neutrino detector array (AMANDA-B10) and the South Pole Air Shower Experiment (SPASE-1 and SPASE-2). We discuss the use of coincident events for calibration and survey of the deep AMANDA detector as well as the response of AMANDA to muon bundles. This analysis uses data taken during 1997 when both SPASE-1 and SPASE-2 were in operation to provide a stereo view of AMANDA. © 2003 Elsevier B.V. All rights reserved.

Antarctic Muon And Neutrino Detector ArrayPhysicsNuclear and High Energy PhysicsMuonDetectorAstronomyCosmic rayParticle detectorAir showerNeutrino detectorCosmic rays; Neutrino telescopesCoincidentNeutrino telescopesCosmic raysInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Results from the AMANDA telescope

2003

We present results from the AMANDA high energy neutrino telescope located at the South Pole. They include measurements of the atmospheric neutrino flux, search for UHE point sources, and diffuse sources producing electromagnetic/hadronic showers at the detector or close to it.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFluxCosmic rayAstrophysicsParticle detectorlaw.inventionMassless particleTelescopeNeutrino detectorlawHigh Energy Physics::ExperimentNeutrinoLeptonNuclear Physics A
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Study of three-nucleon mechanisms in the photodisintegration of 3He

1997

Abstract The cross section of the 3He(γ,pp)n reaction has been measured for the first time over a wide photon energy and proton angular range (200 MeV ≤ Eγ ≤ 800 MeV; 20° ≤ ϑplab ≤ 160°) using the large acceptance detector DAPHNE at the tagged photon facility of the MAMI microtron in Mainz. The wide kinematical coverage of the measurement has allowed a detailed analysis of three-nucleon absorption mechanisms. A model developed by Laget explains the main characteristics of the data in the Δ resonance region.

Nuclear reactionPhysicsNuclear and High Energy PhysicsPhotonProtonNuclear TheoryPhotofissionPhoton energyNuclear physicsPhotodisintegrationPhysics::Accelerator PhysicsNuclear ExperimentNucleonMicrotronNuclear Physics A
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Search for extraterrestrial point sources of high energy neutrinos with AMANDA-II using data collected in 2000-2002

2005

The results of a search for point sources of high energy neutrinos in the northern hemisphere using data collected by AMANDA-II in the years 2000, 2001 and 2002 are presented. In particular, a comparison with the single-year result previously published shows that the sensitivity was improved by a factor of 2.2. The muon neutrino flux upper limits on selected candidate sources, corresponding to an E^{-2} neutrino energy spectrum, are included. Sky grids were used to search for possible excesses above the background of cosmic ray induced atmospheric neutrinos. This search reveals no statistically significant excess for the three years considered.

Astroparticle physicsPhysicsNuclear and High Energy PhysicsSolar neutrinomedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesFluxCosmic rayQuasarAstrophysicsAstrophysics530SkyMuon neutrinoddc:530Neutrinomedia_common
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A source of polarized electrons based on photoemission of GaAsP.

1990

Abstract The source described is based on photoemission of electrons from 100-GaAs0.62P0.38 activated to negative electron affinity. It is built to inject a beam of polarized electrons into the 350 MeV linear accelerator in Mainz. It is capable of delivering a mean current of 28 μA spin-polarized longitudinally to a degree of 0.44. The lifetime of the cathode under operational conditions is better than 200 h. The source was successfully run in a parity experiment, in which the analysing power of quasielastic scattering from beryllium for longitudinally polarized electrons was measured.

PhysicsNuclear and High Energy PhysicsQuasielastic scatteringMeV linear acceleratorInverse photoemission spectroscopychemistry.chemical_elementAngle-resolved photoemission spectroscopyParity (physics)ElectronCathodelaw.inventionchemistrylawBerylliumAtomic physicsInstrumentation
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Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector.

2006

On December 27th 2004, a giant gamma flare from the Soft Gamma-ray Repeater 1806-20 saturated many satellite gamma-ray detectors. This event was by more than two orders of magnitude the brightest cosmic transient ever observed. If the gamma emission extends up to TeV energies with a hard power law energy spectrum, photo-produced muons could be observed in surface and underground arrays. Moreover, high-energy neutrinos could have been produced during the SGR giant flare if there were substantial baryonic outflow from the magnetar. These high-energy neutrinos would have also produced muons in an underground array. AMANDA-II was used to search for downgoing muons indicative of high-energy gamm…

Astroparticle physicsPhysicsMuonSolar flarePhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Gamma rayGeneral Physics and AstronomyAstronomyFOS: Physical sciencesAstrophysicsAstrophysicsGalaxylaw.inventionPulsarlawAstronomiaHigh Energy Physics::ExperimentNeutrinoFlarePhysical review letters
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First year performance of the IceCube neutrino telescope

2006

The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005. One string of 60 sensors buried in the ice and a surface array of eight ice Cherenkov tanks took data until December 2005 when deployment of the next set of strings and tanks began. We have analyzed these data, demonstrating that the performance of the system meets or exceeds design requirements. Times are determined across the whole array to a relative precision of better than 3 ns, allowing reconstruction of muon tracks and light bursts in the ice, of air-showers in the surface array and of events seen in coincidence…

Astroparticle physicsPhysicsPhotomultiplierMuonPerformanceDetectorAstrophysics (astro-ph)AstronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsIceCube Neutrino ObservatoryAmandaIceCubeDetectionData acquisitionFirst yearAmanda; Detection; First year; IceCube; IceTop; Neutrino; Performance; South poleNeutrinoSouth poleAstronomiaIceTopNeutrinoCherenkov radiation
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Search for Neutrino-Induced Cascades with AMANDA

2004

We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high energy neutrinos in the data collected with the AMANDA II detector during the year 2000. The observed event rates are consistent with the expectations for atmospheric neutrinos and muons. We place upper limits on a diffuse flux of extraterrestrial electron, tau and muon neutrinos. A flux of neutrinos with a spectrum $\Phi \propto E^{-2}$ which consists of an equal mix of all flavors, is limited to $E^2 \Phi(E)=8.6 x 10^{-7} GeV/(cm^{2} s sr)$ at a 90% confidence level for a neutrino energy range 50 TeV to 5 PeV. We present bounds for specific extraterrestrial neutrino flux predictions. Several of t…

PhysicsAMANDAParticle physicsMuonPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHadronHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)FluxFOS: Physical sciencesAstronomy and AstrophysicsElectronAstrophysicsNeutrino astronomyAMANDA; Neutrino astronomy; Neutrino telescopesHigh Energy Physics::ExperimentNeutrino telescopesNeutrino astronomyNeutrinoEvent (particle physics)
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Double pion photoproduction off nuclei - Are there effects beyond final-state interaction?

2013

Photoproduction of $\pi^{0}\pi^{0}$ and $\pi^{0}\pi^{\pm}$ pairs from nuclei has been measured over a wide mass range ($^2$H, $^{7}$Li, $^{12}$C, $^{40}$Ca, and $^{\rm nat}$Pb) for photon energies from threshold to 600 MeV. The experiments were performed at the MAMI accelerator in Mainz, using the Glasgow photon tagging spectrometer and a 4$\pi$ electromagnetic calorimeter consisting of the Crystal Ball and TAPS detectors. A shift of the pion-pion invariant mass spectra for heavy nuclei to small invariant masses has been observed for $\pi^0$ pairs but also for the mixed-charge pairs. The precise results allow for the first time a model-independent analysis of the influence of pion final-sta…

PhysicsNuclear and High Energy PhysicsParticle physicsdouble pion photoproduction; crystal ball; sigma-in-medium modificationPhotonMeson010308 nuclear & particles physicsHadronNuclear TheoryCarbon-12FOS: Physical sciencesElementary particle01 natural sciences7. Clean energyNuclear physicsMassless particlePion0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentCrystal Ball
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C(,pn) photon asymmetry for Eγ=180–340 MeV

1999

The photon asymmetry (Σ) of the 12C(,pn) reaction has been measured using linearly polarised tagged photons at the Mainz microtron MAMI for Eγ=180–340 MeV. The data have been analysed in separate missing energy (Em) regions corresponding to the ejection of nucleons from (1p)2 and (1p)(1s) shells. The measured Σ values for both Em regions are smaller in magnitude than corresponding 2H data, but the (1p)2 results have a similar Eγ dependence. Calculations of direct two-nucleon emission overestimate the magnitude of Σ at all photon energies.

PhysicsNuclear and High Energy PhysicsMissing energyPhotonmedia_common.quotation_subjectNuclear TheoryAsymmetryNuclear physicsMagnitude (astronomy)Atomic physicsNuclear ExperimentNucleonMicrotronmedia_commonPhysics Letters B
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Flux limits on ultra high energy neutrinos with AMANDA-B10

2005

Abstract Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 10 16  eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E −2 , with an equal mix of all flavors, is limited to E 2 Φ (10 15  eV  E 18  eV) ⩽ 0.99 × 10 −6  GeV cm −2  s −1  sr −1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bound…

PhysicsParticle physicsAMANDAMuonPhysics::Instrumentation and DetectorsUHE neutrinosAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyFluxAstronomy and AstrophysicsSolar neutrino problemAMANDA; Neutrino astronomy; Neutrino telescopes; UHE neutrinosNeutrino detectorNeutrino astronomyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNeutrino telescopes
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Near threshold photoproduction of eta mesons off the proton.

1995

We have measured precise total and differential cross sections for the reaction $\ensuremath{\gamma}p\ensuremath{\rightarrow}p\ensuremath{\eta}$ from threshold to 790 MeV at the MAMI accelerator in Mainz with the neutral meson spectrometer TAPS. Resonance parameters of the ${S}_{11}$(1535) resonance and the electromagnetic coupling $\ensuremath{\gamma}p\ensuremath{\rightarrow}{S}_{11}$ have been extracted from the data. Contributions from the ${D}_{13}$(1520) resonance to $\ensuremath{\eta}$ photoproduction in the threshold region have been identified for the first time via interference terms in the angular distributions.

PhysicsNuclear physicsParticle physicsNear thresholdAngular distributionProtonMesonGeneral Physics and AstronomyResonanceElectromagnetic couplingNuclear ExperimentCoupling (probability)Physical review letters
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Coherent π0-photoproduction from atomic nuclei

2003

Differential and total cross sections for coherent pi0-photoproduction from 12C, 40Ca, 93Nb and Pb targets have been measured throughout the region of the Delta(1232)-resonance. The experiments were performed with the TAPS-detector at the Mainz accelerator MAMI. The characteristic proportionality of the cross section to the square of the atomic mass number and to the nuclear mass form factor is clearly demonstrated. The data allow for the first time detailed tests of model predictions for this reaction. The comparison of the data to model predictions shows that the Delta-nucleus interaction saturates: it is described for heavy nuclei with the same potential parameters as for 4He.

PhysicsMass numberNuclear physicsNuclear and High Energy PhysicsNuclear TheoryAtomic nucleusFOS: Physical sciencesNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentPhysics Letters B
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Quasifreeπ+production studied using theC12(γ, π+n)B11reaction in theΔ(1232)resonance region

1996

Results are presented from a coincidence study of the {sup 12}C({gamma},{pi}{sup +}{ital n}){sup 11}B quasifree pion production reaction made in the {Delta}-resonance region using tagged photons. Cross sections for reactions originating on 1{ital p}-shell protons are found to be significantly larger than predicted by calculations based on quasifree pion production. It is suggested that more sophisticated calculations, perhaps including medium effects, may be required to reproduce the data. {copyright} {ital 1996 The American Physical Society.}

PhysicsNuclear and High Energy PhysicsPhotonPionMeson productionPiProduction (computer science)Atomic physicsResonance (particle physics)Physical Review C
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Photon Asymmetry of Deuteron Photodisintegration Between 160 and 410 MeV

1999

The photon asymmetry Σ of the reaction has been measured across the photon energy range 160–410 MeV at the Mainz Microtron MAMI. Linearly polarized photons were obtained from coherent bremsstrahlung and their energies were determined with the Glasgow tagging spectrometer. The large acceptance detector DAPHNE enabled the outgoing protons to be measured over the complete azimuthal range and for polar angles from 35° to 155° in the c.m. system. The data are compared with existing results and recent theoretical calculations.

PhysicsRange (particle radiation)PhotonSpectrometermedia_common.quotation_subjectBremsstrahlungPhoton energyAsymmetryAtomic and Molecular Physics and OpticsNuclear physicsPhotodisintegrationPhysics::Accelerator PhysicsAtomic physicsNuclear ExperimentMicrotronmedia_commonFew-Body Systems
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New results on the Roper resonance and the P_{11} partial wave

2008

Properties of the Roper resonance, the first scalar excitation of the nucleon, are determined. Pole positions and residues of the $P_{11}$ partial wave are studied in a combined analysis of pion- and photo-induced reactions. We find the Roper pole at $\{(1371\pm7)-i(92\pm10)\}$ MeV and an elasticity of $0.61\pm 0.03$. The largest decay coupling is found for the $N\sigma$ ($\sigma=(\pi\pi)$-$S$-wave). The analysis is based on new data on $\gamma p\to p\pi^0\pi^0$ for photons in the energy range from the two-pion threshold to 820 MeV from TAPS at Mainz and from 0.4 to 1.3 GeV from Crystal Barrel at Bonn and includes further data from other experiments. The partial wave analysis excludes the p…

TAPSNuclear and High Energy PhysicsRoper resonancePhotonProtonPHOTON SPECTROMETERPartial wave analysisNuclear TheoryDalitz plotFOS: Physical sciencesPION-PHOTOPRODUCTIONPROTONTHRESHOLDNuclear physicsPionHigh Energy Physics - Phenomenology (hep-ph)Nuclear ExperimentPhysicsPI(0) PHOTOPRODUCTIONHigh Energy Physics - PhenomenologyRELATIVISTIC QUARK-MODELSTRANGE-BARYON SPECTRUMPOSITIVE-STRANGENESSFORCESNucleonExcitation
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Coherent photoproduction of η-mesons off 3He – search for η-mesic nuclei

2012

Coherent photoproduction of $\eta$-mesons off $^3$He, i.e. the reaction $\gamma ^3{He}\rightarrow \eta ^3{He}$, has been investigated in the near-threshold region. The experiment was performed at the Glasgow tagged photon facility of the Mainz MAMI accelerator with the combined Crystal Ball - TAPS detector. Angular distributions and the total cross section were measured using the $\eta\rightarrow \gamma\gamma$ and $\eta\rightarrow 3\pi^0\rightarrow 6\gamma$ decay channels. The observed extremely sharp rise of the cross section at threshold and the behavior of the angular distributions are evidence for a strong $\eta {^3{He}}$ final state interaction, pointing to the existence of a resonant …

PhysicsExcitation functionNuclear and High Energy PhysicsParticle physicsMesonHigh Energy Physics::PhenomenologyHadronGamma rayFOS: Physical sciencesBaryonNuclear physicsHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)total cross section ; photoproduction ; eta meson ; final-state interaction ; Crystal Ball ; MAMINucleonNuclear ExperimentNuclear ExperimentIsotopes of heliumCrystal Ball
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Total photofission cross section for 238U as a substitute for the photon absorption cross section in the energy range of the first baryon resonances

1992

Abstract The total photofission cross section σγ, F for 238U has been measured as a substitute for the total photon absorption cross section σtot in the energy range of the first baryon resonances (50⩽Eγ⩽800 MeV). The experiments were performed at the tagging facility of the new 855 MeV Mainz Microton MAMI B using monochromatic photons and a sophisticated 4π-arrangement of position sensitive fragment detectors. The measured cross section agrees in the Δ-resonance region with previous results and the so-called universal curve αtot/A. In the energy region of the D13-resonance near 710 MeV resonancelike structure could be observed as is seen for the free proton.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)PhotonProtonNuclear TheoryPhotofissionAbsorption cross sectionNuclear physicsBaryonCross section (physics)Monochromatic colorAtomic physicsNuclear ExperimentPhysics Letters B
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Photoproduction of $\eta$ $\pi$ pairs off nucleons and deuterons

2016

Quasi-free photoproduction of $\pi\eta$-pairs has been investigated from threshold up to incident photon energies of 1.4 GeV, respectively up to photon-nucleon invariant masses up to 1.9 GeV. Total cross sections, angular distributions, invariant-mass distributions of the $\pi\eta$ and meson-nucleon pairs, and beam-helicity asymmetries have been measured for the reactions $\gamma p\rightarrow p\pi^0\eta$, $\gamma n\rightarrow n\pi^0\eta$, $\gamma p\rightarrow n\pi^+\eta$, and $\gamma n\rightarrow p\pi^-\eta$ from nucleons bound inside the deuteron. For the $\gamma p$ initial state data for free protons have also been analyzed. Finally, the total cross sections for quasi-free production of $…

PhysicsNuclear and High Energy PhysicsPhotonProton010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciences01 natural sciences7. Clean energyNuclear physicsDeuteriumREACTION GAMMA-P ; TAGGED PHOTON SPECTROMETER ; I-CIRCLE-DOT ; MESON PHOTOPRODUCTION ; HIGH-STATISTICS ; PROTON ; THRESHOLD ; MAMI ; POLARIZATION ; PI(0)-PAIRS0103 physical sciencesPiNeutronHigh Energy Physics::Experimentddc:530Decay chainNuclear Experiment (nucl-ex)010306 general physicsNucleonNuclear ExperimentNuclear ExperimentCrystal Ball
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Photoproduction of π0-pairs off protons and off neutrons

2015

Total cross sections, angular distributions, and invariant-mass distributions have been measured for the photoproduction of π0π0 pairs off free protons and off nucleons bound in the deuteron. The experiments were performed at the MAMI accelerator facility in Mainz using the Glasgow photon tagging spectrometer and the Crystal Ball/TAPS detector. The accelerator delivered electron beams of 1508 and 1557MeV, which produced bremsstrahlung in thin radiator foils. The tagged photon beam covered energies up to 1400MeV. The data from the free proton target are in good agreement with previous measurements and were only used to test the analysis procedures. The results for differential cross sections…

Nuclear TheoryNuclear Experiment
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Photofission of235U and238U at intermediate energies: absolute cross sections and fragment mass distributions

1994

The total photofission cross section σγ,F for235U and238U has been measured in the energy range 50≤E γ≤800 MeV at the 855 MeV Mainz Microtron MAMI using energy and time tagged photons (Glasgow Tagger) and a 4π arrangement of position sensitive fragment detectors. Besides the absolute photofission cross section σγF , which almost completely exhausts the total photon absorption cross section for these nuclei, fragment mass distributions in this energy domain were determined via time of flight techniques (TOF). The results for the total photofission cross sections σγ,F normalized to the atomic numberA for both isotopes coincide, and agree in theΔ-resonance region, within the systematic errors,…

PhysicsNuclear and High Energy PhysicsProtonFissionNuclear TheoryAbsorption cross sectionPhotofissionResonance (particle physics)Nuclear physicsTime of flightPionMass spectrumAtomic physicsNuclear ExperimentZeitschrift f�r Physik A Hadrons and Nuclei
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Investigation of multiparticle final states in12C photoreactions

1998

The ${}^{12}\mathrm{C}(\ensuremath{\gamma},pn)$, ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp)$, ${}^{12}\mathrm{C}(\ensuremath{\gamma},ppp)$, ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp{\ensuremath{\pi}}^{\ifmmode\pm\else\textpm\fi{}})$, ${}^{12}\mathrm{C}(\ensuremath{\gamma},p{\ensuremath{\pi}}^{\ifmmode\pm\else\textpm\fi{}})$ reactions have been studied using tagged photons of energy ${E}_{\ensuremath{\gamma}}=250$--600 MeV. A model which includes all major absorption mechanisms and final state interactions gives results that agree well with the shapes of missing energy spectra, but for some channels the predicted cross sections are too large.

PhysicsNuclear and High Energy PhysicsPionAstrophysics::High Energy Astrophysical PhenomenaAbsorption (logic)Atomic physicsSpectral lineEnergy (signal processing)Physical Review C
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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

2007

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the the…

Gamma rays: burstsNormalization (statistics)PhysicsRange (particle radiation)MuonAstrophysics::High Energy Astrophysical PhenomenaGamma rays: bursts; Neutrinos; TelescopesAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCoincidenceSpace and Planetary ScienceCascadeAstronomiaDiffuse fluxHigh Energy Physics::ExperimentNeutrinosNeutrinoGamma-ray burstTelescopesThe Astrophysical Journal
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The isospin structure of photoproduction of πη pairs from the nucleon in the threshold region

2015

Abstract Photoproduction of πη-pairs from nucleons has been investigated from threshold up to incident photon energies of ≈ 1.4 GeV. The quasi-free reactions γ p → p π 0 η , γ n → n π 0 η , γ p → n π + η , and γ n → p π − η were for the first time measured from nucleons bound in the deuteron. The corresponding reactions from a free-proton target were also studied to investigate final-state interaction effects (for neutral pions the free-proton results could be compared to previous measurements; the γ p → n π + η reaction was measured for the first time). For the π 0 η final state coherent production via the γ d → d π 0 η reaction was also investigated. The experiments were performed at the …

PhysicsNuclear and High Energy PhysicsPhotonPhysicsNuclear Theory7. Clean energylcsh:QC1-999photoproduction; final-state interaction; total cross section; Delta(1232) structure; deuteron; isospin; MAMIPionElectromagnetic calorimeterDeuteriumIsospinIsobarAtomic physicsNuclear ExperimentNucleonlcsh:PhysicsCrystal BallPhysics Letters B
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Quasi-free Compton Scattering and the Polarizabilities of the Neutron

2002

Differential cross sections for quasi-free Compton scattering from the proton and neutron bound in the deuteron have been measured using the Glasgow/Mainz tagging spectrometer at the Mainz MAMI accelerator together with the Mainz 48 cm $\oslash$ $\times$ 64 cm NaI(Tl) photon detector and the G\"ottingen SENECA recoil detector. The data cover photon energies ranging from 200 MeV to 400 MeV at $\theta^{LAB}_\gamma=136.2^\circ$. Liquid deuterium and hydrogen targets allowed direct comparison of free and quasi-free scattering from the proton. The neutron detection efficiency of the SENECA detector was measured via the reaction $p(\gamma,\pi^+ n)$. The "free" proton Compton scattering cross sect…

Nuclear and High Energy PhysicsProtonNuclear TheoryFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Polarizability0103 physical sciencesNeutron detectionNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysics010308 nuclear & particles physicsScatteringCompton scatteringHigh Energy Physics - PhenomenologyDeuteriumCover (topology)High Energy Physics::Experiment
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Compton scattering by the proton through θcms = 75° and 90° in the Δ-resonance region

1997

Abstract Differential cross sections for Compton scattering by the proton have been measured in the energy interval between 200 and 500 MeV at scattering angles of θcms = 75° and θcms = 90° using the CATS, the CATS/TRAJAN, and the COPP setups with the Glasgow Tagger at MAMI (Mainz). The data are compared with predictions from dispersion theory using photo-meson amplitudes from the recent VPI solution SM95. The experiment and the theoretical procedure are described in detail. It is found that the experiment and predictions are in agreement as far as the energy dependence of the differential cross sections in the Δ-range is concerned. However, there is evidence that a scaling down of the reso…

PhysicsNuclear and High Energy PhysicsProton010308 nuclear & particles physicsScatteringDispersion theoryCompton scattering01 natural sciencesResonance (particle physics)Nuclear physicsAmplitude0103 physical sciencesEnergy intervalAtomic physics010306 general physicsScalingNuclear Physics A
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Krusche et al. reply.

1995

PhysicsInformation retrievalText miningbusiness.industryGeneral Physics and AstronomybusinessPhysical review letters
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The IceCube data acquisition system: Signal capture, digitization, and timestamping

2008

IceCube is a km-scale neutrino observatory under construction at the South Pole with sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital Optical Modules (DOMs), detect, digitize and timestamp the signals from optical Cherenkov-radiation photons. The DOM Main Board (MB) data acquisition subsystem is connected to the central DAQ in the IceCube Laboratory (ICL) by a single twisted copper wire-pair and transmits packetized data on demand. Time calibration is maintained throughout the array by regular transmission to the DOMs of precisely timed analog signals, synchronized to a central GPS-disciplined clock. The design goals and consequent features, func…

AMANDANuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesAstrophysicsNeutrino telescopeSignalHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryNuclear physicsHigh Energy Physics - Experiment (hep-ex)IcecubeData acquisitionSignal digitizationddc:530Nuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationPhysicsbusiness.industryAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAMANDA; Icecube; Neutrino telescope; Signal digitizationTimestampingInstrumentation and Detectors (physics.ins-det)Analog signalTransmission (telecommunications)Systems designTimestampbusinessComputer hardware
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NEUTRINO ASTRONOMY AND COSMIC RAYS AT THE SOUTH POLE: LATEST RESULTS FROM AMANDA AND PERSPECTIVES FOR ICECUBE

2005

The AMANDA neutrino telescope has been in operation at the South Pole since 1996. The present final array configuration, operational since 2000, consists of 677 photomultiplier tubes arranged in 19 strings, buried at depths between 1500 and 2000 m in the ice. The most recent results on a multi-year search for point sources of neutrinos will be shown. The study of events triggered in coincidence with the surface array SPASE and AMANDA provided a result on cosmic ray composition. Expected improvements from IceCube/IceTop will also be discussed.

PhysicsNuclear and High Energy PhysicsPhotomultiplierAstronomyAstronomy and AstrophysicsCosmic rayAstrophysicsSolar neutrino problemAtomic and Molecular Physics and OpticsCoincidencelaw.inventionTelescopeNeutrino detectorlawNeutrino astronomyNeutrinoInternational Journal of Modern Physics A
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Polarizability of the neutron

1990

Abstract A first measurement of quasi-free Compton scattering by the neutron bound in the deuteron has yielded a value for the polarizability of the neutron of αn=(11.7 −11.7+4.3)×10 −4fm 3. This means that a finite value for the polarizability has been obtained, though the result is still consistent with zero. The π0 decay constant Fπ 0γγ and the pion nucleon coupling constant gNNπ have opposite signs.

Coupling constantPhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryCompton scatteringlcsh:QC1-999Nuclear physicsPionDeuteriumPolarizabilityNeutronAstrophysics::Earth and Planetary AstrophysicsExponential decayAtomic physicsNuclear ExperimentNucleonlcsh:PhysicsPhysics Letters B
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Neutron Skin ofPb208from Coherent Pion Photoproduction

2014

Information on the size and shape of the neutron skin on (208)Pb is extracted from coherent pion photoproduction cross sections measured using the Crystal Ball detector together with the Glasgow tagger at the MAMI electron beam facility. On exploitation of an interpolated fit of a theoretical model to the measured cross sections, the half-height radius and diffuseness of the neutron distribution are found to be c(n)=6.70±0.03(stat.)  fm and a(n)=0.55±0.01(stat.)(-0.03)(+0.02)(sys.)  fm, respectively, corresponding to a neutron skin thickness Δr(np)=0.15±0.03(stat.)(-0.03)(+0.01)(sys.)  fm. The results give the first successful extraction of a neutron skin thickness with an electromagnetic p…

PhysicsEquation of stateMeson010308 nuclear & particles physicsScatteringGeneral Physics and AstronomyRadius01 natural sciencesNuclear physicsPion0103 physical sciencesHigh Energy Physics::ExperimentNeutronNuclear Experiment010306 general physicsMicrotronCrystal BallPhysical Review Letters
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In-Medium Properties of theD13(1520) Nucleon Resonance

2001

The in-medium properties of the ${\mathrm{D}}_{13}(1520)$ nucleon resonance were studied via photoproduction of ${\ensuremath{\pi}}^{0}$ mesons from nuclei (C, Ca, Nb, Pb) with the TAPS detector at the Mainz Microton accelerator. The inclusive (single and multiple pion production) data disagree with model predictions which explain the disappearance of the second resonance bump in total photoabsorption via a medium modification of the ${\mathrm{D}}_{13}\ensuremath{\rightarrow}\mathrm{N}\ensuremath{\rho}$ decay. The exclusive single ${\ensuremath{\pi}}^{0}$ production data show no broadening of the resonance structure beyond Fermi smearing. Both results together cast doubt on attempts to expl…

PhysicsParticle physicsPionMesonNuclear TheoryGeneral Physics and AstronomyProduction (computer science)Nuclear ExperimentNucleonResonance (chemistry)Fermi Gamma-ray Space TelescopePhysical Review Letters
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Intense source of slow positrons from pulsed electron accelerators

1984

A pulsed LINAC is used for pair production in a tantalum target of 2.5 radiation lengths in an energy range from 80 to 260 MeV. Several well-annealed tungsten vanes are placed immediately behind the target and thermalize a small fraction of the fast positrons. The slow positrons are extracted from the target region and magnetically guided over a distance of 17 m to the detector at the end of an S-shaped solenoid. Two Nal detectors with well-known detection efficiency are used to register the 511 keV annihilationγ-rays. To reduce pile-up effects 50 mm of Pb were placed in front of the detectors. At an average electron current of 1 μA we could detect about 107 slow positrons per second. The p…

PhysicsRange (particle radiation)Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsGeneral EngineeringParticle acceleratorSolenoidGeneral ChemistryElectronRadiationLinear particle acceleratorlaw.inventionNuclear physicsPositronPair productionlawPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentGeneral Materials ScienceAtomic physicsApplied Physics A Solids and Surfaces
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Physics results from the Amanda neutrino detector

2001

In the winter season of 2000, the AMANDA (Antarctic Muon And Neutrino Detector Array) detector was completed to its final state. We report on major physics results obtained from the AMANDA-B10 detector, as well as initial results of the full AMANDA-II detector.

Astroparticle physicsPhysicsParticle physicsMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorSolar neutrino problemNuclear physicsNeutrino detectorHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNeutrino oscillationPhysics::Atmospheric and Oceanic PhysicsParticle Physics - Phenomenology
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Search for the charge-conjugation-forbidden decayω→ηπ0

2009

A new upper limit of 2.3x10{sup -4} on the branching ratio of the decay {omega}{yields}{eta}{pi}{sup 0} has been obtained using the Crystal Ball multiphoton spectrometer at the Mainz Microtron MAMI. This decay is forbidden by charge-conjugation invariance of the strong and electromagnetic interactions. We have also obtained the upper limit of 2.3x10{sup -4} for the forbidden decay {omega}{yields}3{pi}{sup 0} and the upper limit of 2.4x10{sup -4} for {omega}{yields}2{pi}{sup 0}.

PhysicsNuclear and High Energy PhysicsParticle physicsParticle decayPionMesonBranching fractionHadronAtomic physicsNuclear ExperimentOmega baryonOmegaCrystal BallPhysical Review C
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Total photoabsorption cross sections forH1,H2, andHe3from 200 to 800 MeV

1996

The total photoabsorption cross sections for $^{1}\mathrm{H}$, $^{2}\mathrm{H}$, and $^{3}\mathrm{He}$ have been measured for incident photon energies ranging from 200 to 800 MeV. The $^{3}\mathrm{He}$ data are the first for this nucleus. By using the large acceptance detector DAPHNE in conjunction with the tagged photon beam facility of the MAMI accelerator in Mainz, cross sections of high precision have been obtained. The results show clearly the changes in the nucleon resonances in going from $^{1}\mathrm{H}$ to $^{3}\mathrm{He}$. In particular, for the ${\mathit{D}}_{13}$ region the behavior for $^{3}\mathrm{He}$ is intermediate between that for $^{1}\mathrm{H}$, $^{2}\mathrm{H}$, and h…

Nuclear physicsPhysicsNuclear and High Energy PhysicsPhotonNuclear TheoryResonanceAbsorption (logic)Photon beamAtomic physicsNuclear ExperimentNucleonPhysical Review C
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The angular distribution of the 12C(γ,pn) reaction for Eγ=120−150 MeV

1998

The angular distribution of nucleons emitted in the 12C(γ,pn) reaction has been measured using tagged photons at the Mainz microtron MAMI. The variation of the reaction strength with the polar angles of the two emitted nucleons is reported for Eγ=120−150 MeV. The proton angular distribution peaks at more backward angles than the 2H(γ,p) differential cross section indicating a departure from the simple quasi-deuteron model of 2N photo-emission. The distribution shape is in reasonable agreement with microscopic theoretical models which include both π- and ρ-exchange.

PhysicsNuclear and High Energy PhysicsPhotonProtonNuclear TheoryShape of the distributionNuclear physicsAngular distributionNuclear fusionPolarAtomic physicsNuclear ExperimentNucleonMicrotronThe European Physical Journal A
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First Measurement of the Gerasimov-Drell-Hearn Sum Rule forH1from 0.7 to 1.8 GeV at ELSA

2003

To verify the fundamental Gerasimov-Drell-Hearn (GDH) sum rule for the first time experimentally, we measured the helicity dependent total photoabsorption cross section with circularly polarized real photons and longitudinally polarized nucleons in the photon energy range 0.68-1.82 GeV with the tagged photon facility at ELSA. The experiment was carried out with a 4pi detection system, a circularly polarized tagged photon beam, and a frozen spin polarized proton target. The contribution to the GDH sum rule in this photon energy range is [49.9+/-2.4(stat)+/-2.2(syst)] mub.

PhysicsParticle physicsRange (particle radiation)PhotonProton010308 nuclear & particles physicsNuclear TheoryGeneral Physics and AstronomyPhoton energy01 natural sciencesHelicityNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentSum rule in quantum mechanicsNuclear Experiment010306 general physicsNucleonSpin-½Physical Review Letters
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Beam-Helicity Asymmetries in Double-Pion Photoproduction off the Proton

2009

Beam-helicity asymmetries have been measured at the MAMI accelerator in Mainz in the three isospin channels $\vec{\gamma}p\to \pi^{+}\pi^0n$, $\vec{\gamma}p\to \pi^{0}\pi^0p$ and $\vec{\gamma}p\to \pi^{+}\pi^{-}p$ . The circularly polarized photons, produced from bremsstrahlung of longitudinally polarized electrons, were tagged with the Glasgow magnetic spectrometer. Charged pions and the decay photons of $\pi^0$ mesons were detected in a $~4\pi$ electromagnetic calorimeter which combined the Crystal Ball detector with the TAPS detector. The precisely measured asymmetries are very sensitive to details of the production processes and are thus key observables in the modeling of the reaction d…

PhysicsParticle physicsProtonMeson010308 nuclear & particles physicsNuclear TheoryHadronFOS: Physical sciencesGeneral Physics and Astronomy7. Clean energy01 natural sciencesHelicity3. Good healthNuclear physicsPair productionPion0103 physical sciencesHigh Energy Physics::ExperimentInvariant massNuclear Experiment (nucl-ex)Nuclear Experiment010306 general physicsNuclear Experimentbeam-helicity asymmetries ; charged pions and the decay photonLeptonPhysical Review Letters
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A polarized 3He target for the photon beam at MAMI

2011

Abstract A polarized 3 He target has been installed for the first time inside the 4 π Crystal Ball detector at the tagged photon beam of the MAinz MIcrotron (MAMI). It has been demonstrated that the system works reliably and that the polarization losses during handling of the polarized gas are under control. Initial polarization values up to 70% and total relaxation times up to 20 h could be obtained during a first test beam time devoted to the measurement of the double polarized photoabsorption cross-section in the Δ ( 1232 ) baryon resonance region.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsDetectorPolarization (waves)01 natural sciencesParticle detectorDelta baryonNuclear physicsBaryonHelium-30103 physical sciencesPhysics::Accelerator Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Atomic physics010306 general physicsNuclear ExperimentInstrumentationMicrotronCrystal Ball
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Recent results from AMANDA II

2003

Abstract We present new data taken with the AMANDA-II neutrino telescope array. The AMANDA-II upgrade was completed at the beginning of 2000. It significantly extends the sensitivity of the 10-string AMANDA-B10 detector to high- and ultrahigh-energy neutrino fluxes into regions of interest for probing current astrophysical models which remain unexplored by other experiments.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeDetectorAstronomyCosmic rayAstrophysicsComputer Science::Computational GeometryAtomic and Molecular Physics and OpticsParticle detectorUpgradeNeutrino detectorHigh Energy Physics::ExperimentNeutrinoNuclear Physics B - Proceedings Supplements
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Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

2003

We present the results of a Monte-Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from sources such as active galaxies and gamma-ray bursts. We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino emissions, including an assessment of the sensitivity to neutrinos detected in coincidence with gamma-ray burst observatio…

PhysicsActive galactic nucleusMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorAstrophysics (astro-ph)Gamma rayFOS: Physical sciencesIceCube; Neutrino astronomy; Neutrino telescopeAstronomy and AstrophysicsCosmic rayAstrophysicsAstrophysicsNeutrino telescopeIceCubeNeutrino astronomyHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyGamma-ray burst
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IceCube contributions to the XIV International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2006)

2008

IceCube contributions to the XIV International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2006) Weihai, China - August 15-22

PhysicsNuclear and High Energy PhysicsHigh energyCosmic rayAstrophysicsChinaAtomic and Molecular Physics and OpticsNuclear Physics B - Proceedings Supplements
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Enhancement of the linear polarization of coherent bremsstrahlung by collimation of the photon beam

1998

A method is described to precisely predict the relative intensities and degrees of linear polarization of coherent bremsstrahlung from diamond crystals, taking into account the collimation of the photon beam and the lateral distribution and angular divergence of the electron beam in addition to the properties of the crystal. It is confirmed that the increase of the degree of linear polarization through collimation of the photon beam is a sizable effect. Compared to previous approaches considerable progress has been made in reproducing the experimentally observed relative intensities of collimated coherent bremsstrahlung, by taking into account the angular distribution of coherent bremsstrah…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsLinear polarizationAstrophysics::High Energy Astrophysical PhenomenaBremsstrahlung01 natural sciencesCollimated lightCrystalDistribution (mathematics)0103 physical sciencesCathode rayPhysics::Accelerator PhysicsRadial polarizationAtomic physics010306 general physicsDivergence (statistics)Physical Review C
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Photoproduction of π 0 mesons off protons and neutrons in the second and third nucleon resonance regions

2018

Photoproduction of mesons off quasi-free nucleons bound in the deuteron allows to study the electromagnetic excitation spectrum of the neutron and the isospin structure of the excitation of nucleon resonances. The database for such reactions is much more sparse than for free proton targets. Single $\pi^0$ photoproduction off quasi-free nucleons from the deuteron was experimentally studied. Nuclear effects were investigated by a comparison of the results for free protons and quasi-free protons and used as a correction for the quasi-free neutron data. The experiment was performed at the tagged photon beam of the Mainz MAMI accelerator for photon energies between 0.45~GeV and 1.4~GeV, using an…

PhysicsNuclear reactionProtonMeson010308 nuclear & particles physicsHadronNuclear Theory7. Clean energy01 natural sciences3. Good healthNuclear physicsPionIsospin0103 physical sciencestagged photon spectrometer ; polarization observable E ; cross-sections ; pion-photoproduction ; baryon resonances ; deuteron ; MAMI ; asymmetry ; microtron ; thresholdNeutronddc:530010306 general physicsNucleonNuclear ExperimentNuclear Experiment
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First measurement of helicity-dependent cross sections in Photoproduction From Quasi-free Nucleons

2018

The helicity-dependent cross sections for the photoproduction of π0η pairs have been measured for the first time. The experiment was performed at the tagged photon facility of the Mainz MAMI accelerator with the combined Crystal Ball – TAPS calorimeter. The experiment used a polarized deuterated butanol target and a circularly polarized photon beam. This arrangement allowed the σ1/2 (photon and target spin antiparallel) and σ3/2 (parallel spins) components to be measured for quasi-free production of π0η pairs off protons and neutrons. The main finding is that the two helicity components contribute identically, within uncertainties, for both participant protons and neutrons. The absolute cou…

Physics Letters
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Optical properties of deep glacial ice at the South Pole

2006

We have remotely mapped optical scattering and absorption in glacial ice at the South Pole for wavelengths between 313 and 560 nm and depths between 1100 and 2350 m. We used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice. At depths greater than 1300 m, both the scattering coefficient and absorptivity follow vertical variations in concentration of dust impurities, which are seen in ice cores from other Antarctic sites and which track climatological changes. The scattering coefficient varies by a factor of seven, and absorptivity (for wavelengths less than ∼450 nm) varies by a fact…

Atmospheric ScienceSoil ScienceMineralogyAquatic ScienceOceanographyLight scatteringPhysics::GeophysicsIce coreGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Absorption (electromagnetic radiation)Physics::Atmospheric and Oceanic PhysicsEarth-Surface ProcessesWater Science and Technologygeographygeography.geographical_feature_categoryEcologyScatteringPaleontologyForestryGlacierMolar absorptivityWavelengthGeophysicsSpace and Planetary ScienceAttenuation coefficientAstrophysics::Earth and Planetary AstrophysicsGeologyJournal of Geophysical Research
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Photoproduction of $ \pi^{0}$ -pairs off protons and off neutrons

2015

Total cross sections, angular distributions, and invariant-mass distributions have been measured for the photoproduction of $\pi^0\pi^0$ pairs off free protons and off nucleons bound in the deuteron. The experiments were performed at the MAMI accelerator facility in Mainz using the Glasgow photon tagging spectrometer and the Crystal Ball/TAPS detector. The accelerator delivered electron beams of 1508 and 1557~MeV, which produced bremsstrahlung in thin radiator foils. The tagged photon beam covered energies up to 1400~MeV. The data from the free proton target are in good agreement with previous measurements and were only used to test the analysis procedures. The results for differential cros…

Nuclear reactionPhysicsNuclear and High Energy PhysicsProtonMesonNuclear TheoryBremsstrahlung7. Clean energyDelta baryonNuclear physicsPhysics::Accelerator PhysicsNeutronAtomic physicsNuclear ExperimentNucleonNuclear ExperimentCrystal BallThe European Physical Journal A
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Total cross section measurement for the three double pion photoproduction channels on the proton

1995

Abstract The total cross sections for the three γp → Nππ reactions have been measured for photon energies from 400 to 800 MeV. The γ p → p π 0 π 0 and γ p → n π + π 0 cross sections have never been measured before while the γ p → p π + π − results are much improved compared to earlier data. These measurements were performed with the large acceptance hadronic detector DAPHNE, at the tagged photon beam facility of the MAMI microtron in Mainz.

PhysicsNuclear physicsNuclear and High Energy PhysicsCross section (physics)Particle physicsPhotonPionProtonHadronDetectorPhoton beamMicrotronPhysics Letters B
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Measurement of the cosmic ray composition at the knee with the SPASE-2/AMANDA-B10 detectors

2004

The mass composition of high-energy cosmic rays at energies above 1015 eV can provide crucial information for the understanding of their origin. Air showers were measured simultaneously with the SPASE-2 air shower array and the AMANDA-B10 Cherenkov telescope at the South Pole. This combination has the advantage to sample almost all high-energy shower muons and is thus a new approach to the determination of the cosmic ray composition. The change in the cosmic ray mass composition was measured versus existing data from direct measurements at low energies. Our data show an increase of the mean log atomic mass 〈lnA〉 by about 0.8 between 500 TeV and 5 PeV. This trend of an increasing mass throug…

Astroparticle physicsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsCosmic rayAstrophysicsCosmic Rays; Mass composition; Neutrino astronomyMass compositionCosmic RaysAtomic massAir showerNeutrino astronomyUltra-high-energy cosmic rayNeutrinoNeutrino astronomyCherenkov radiationAstroparticle Physics
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Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector

2003

Data from the AMANDA-B10 detector taken during the austral winter of 1997 have been searched for a diffuse flux of high energy extraterrestrial muon-neutrinos, as predicted from, e.g., the sum of all active galaxies in the universe. This search yielded no excess events above those expected from the background atmospheric neutrinos, leading to upper limits on the extraterrestrial neutrino flux. For an assumed E^-2 spectrum, a 90% classical confidence level upper limit has been placed at a level E^2 Phi(E) = 8.4 x 10^-7 GeV cm^-2 s^-1 sr^-1 (for a predominant neutrino energy range 6-1000 TeV) which is the most restrictive bound placed by any neutrino detector. When specific predicted spectral…

PhysicsPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Physics and AstronomyQuasarCosmic rayAstrophysicsAstrophysicsUniverseMassless particlePhysics::Popular PhysicsExtraterrestrial lifeHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLeptonmedia_common
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Mechanisms in theC12(γ,pn)and(γ,pp)Reactions

1998

${}^{12}\mathrm{C}(\ensuremath{\gamma},pn)$ and $(\ensuremath{\gamma},pp)$ cross sections have been measured in kinematics which emphasize direct $2N$ knockout for ${E}_{\ensuremath{\gamma}}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}120--400\mathrm{MeV}$ and ${\ensuremath{\theta}}_{p}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}23\ifmmode^\circ\else\textdegree\fi{}--152\ifmmode^\circ\else\textdegree\fi{}$. The cross sections for both reactions peak strongly in the $\ensuremath{\Delta}$-resonance region. Theoretical calculations that account for the medium dependence of the $\ensuremath{\Delta}$ propagator predict a similar photon energy dependence to the data and describe the …

PhysicsGeneral Physics and AstronomyPropagatorAngular dependenceAtomic physicsPhoton energyPhysical Review Letters
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A high angular-resolution and time-of-flight detector system for recoil protons from the reactions p(γ, γ)p and p(γ, π0)p

1996

Using the Mainz NaI(Tl)BaF2 photon spectrometer CATS (Compton And Two photon Spectrometer) together with the prototype of a universal spectrometer for recoil protons TRAJAN (TRAjectory ANalyser) we have studied different methods to disentangle Compton scattering by the proton from the large π0 background through the energy range of the Δ resonance. CATS is a modular 48 cm ⊘ × 64 cm NaI(Tl) detector with an energy resolution of 1.5% combined with a 2π array of 61 BaF2 detectors. TRAJAN consists of a hodoscope with two planes, a wire chamber with horizontal and vertical wires and a grid of horizontal and vertical plastic scintillator strips, followed by a wall of nine NaI(Tl) detectors. By t…

PhysicsElastic scatteringNuclear and High Energy PhysicsSpectrometerPhysics::Instrumentation and Detectors010308 nuclear & particles physicsScatteringCompton scatteringScintillator01 natural sciencesNuclear physicsRecoilHodoscope0103 physical sciencesScintillation counterNuclear Experiment010306 general physicsInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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First results from MAMI

1993

Abstract The 100% duty factor electron accelerator MAMI (Mainzer Mikrotron) has gone into operation. First experiments with quasi-monochromatic real photons have been performed. First results, mostly preliminary, are presented.

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsPhotonDuty cyclelawParticle acceleratorlaw.inventionNuclear Physics A
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Measurement of Helicity-Dependent Photoabsorption Cross Sections on the Neutron from 815 to 1825 MeV

2005

Helicity-dependent total photoabsorption cross sections on the deuteron have been measured for the first time at ELSA (Bonn) in the photon energy range from 815 to 1825 MeV. Circularly polarized tagged photons impinging on a longitudinally polarized LiD target have been used together with a highly efficient 4pi detector system. The data around 1 GeV are not compatible with predictions from existing multipole analyses. From the measured energy range an experimental contribution to the GDH integral on the neutron of [33.9 +/- 5.5(stat) +/- 4.5(syst)] microb is extracted.

PhysicsRange (particle radiation)Photon010308 nuclear & particles physicsNuclear TheoryGeneral Physics and AstronomyPhoton energy7. Clean energy01 natural sciencesHelicityNuclear physicsDeuterium0103 physical sciencesNeutronAtomic physicsNuclear Experiment010306 general physicsMultipole expansionCircular polarizationPhysical Review Letters
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Quasifree photoproduction of eta mesons off protons and neutrons

2014

Differential and total cross sections for the quasifree reactions $\ensuremath{\gamma}p\ensuremath{\rightarrow}\ensuremath{\eta}p$ and $\ensuremath{\gamma}n\ensuremath{\rightarrow}\ensuremath{\eta}n$ have been determined at the MAMI-C electron accelerator by using a liquid deuterium target. Photons were produced via bremsstrahlung from the 1.5 GeV incident electron beam and energy tagged with the Glasgow photon tagger. Decay photons of the neutral decay modes $\ensuremath{\eta}\ensuremath{\rightarrow}2\ensuremath{\gamma}$ and $\ensuremath{\eta}\ensuremath{\rightarrow}3{\ensuremath{\pi}}^{0}\ensuremath{\rightarrow}6\ensuremath{\gamma}$ and coincident recoil nucleons were detected in a combin…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryProtonMesonNuclear TheoryBremsstrahlung7. Clean energyHigh Energy Physics - ExperimentNuclear physicsRecoilNeutronNuclear ExperimentNucleonNuclear ExperimentEnergy (signal processing)Crystal BallPHYSICAL REVIEW C
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Search for narrow dibaryon resonances in neutral pion photoproduction from the deuteron

2000

The reaction γd↦π0 X has been measured with TAPS at MAMI in the energy range E γ = 140-300 MeV. Using the Glasgow tagging spectrometer a photon energy resolution of 0.8 MeV was achieved. The energy excitation functions of integral and differential total cross-sections show no structures of statistical significance > 2σ. Upper limits for the production of narrow isoscalar or isovector dibaryons with masses m? 2100 MeV/c2 were deduced. They are in the range 2-5 μb averaged over the 0.8 MeV energy resolution.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Particle physicsIsovectorSpectrometer010308 nuclear & particles physicsIsoscalarNuclear TheoryHadronPhoton energy7. Clean energy01 natural sciencesNuclear physicsPion0103 physical sciencesNuclear fusionNuclear Experiment010306 general physicsThe European Physical Journal A
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Proton photoproduction from 12C

1995

Abstract The 12 C(γ,p) differential cross-section in the Δ-resonance region has been measured using tagged photons. Data are presented for 20 MeV wide photon energy bins at 200, 300, 400 and 500 MeV and for proton angles from 52° to 128°. The present 12 C(γ,p) measurements are compared with previous experiments carried out at Frascati, Tokyo and Bonn. Comparisons are also made with theoretical calculations developed at Gent and Valencia which provide an interpretation of the photon reaction mechanism in terms of the major contributing processes. Coincidence data with correlated neutrons, protons and pions are also presented.

PhysicsNuclear and High Energy PhysicsPhotonProtonbiologyNuclear TheoryPhoton energybiology.organism_classificationCoincidenceNuclear physicsPionNeutronNuclear ExperimentValenciaNuclear Physics A
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Coherent and incoherent π0 photoproduction from the deuteron

2001

Differential cross-sections for the reactions d(gamma,pi (o))d and d(gamma,pi (o))pn have been measured at MAMI with the TAPS detector setup in the energy range 140 MeV > E- > 306 MeV. By use of the Glasgow tagging spectrometer an 0.8 MeV energy resolution for photons incident on the target was achieved. The (o) missing energy resolution was sufficient for a reliable separation of coherent and incoherent channels. The data for the break-up channel exhibit very strong final state interaction effects, whereas the observed angular dependence of the inclusive process d(gamma, pi (o))X is in quantitative agreement with predictions for a quasi-free process. The observed absolute d(gamma, pi (o))X…

PhysicsNuclear and High Energy PhysicsRange (particle radiation)PhotonMissing energySpectrometer010308 nuclear & particles physicsHadron01 natural sciences7. Clean energyNuclear physicsDeuterium0103 physical sciencesNuclear fusionNeutronAtomic physicsNuclear Experiment010306 general physicsThe European Physical Journal A
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The12C(γ,NN)reaction studied over a wide kinematic range

2000

The ${}^{12}\mathrm{C}(\ensuremath{\gamma},np)$ and ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp)$ reactions have been studied using the Glasgow photon tagging spectrometer at the Mainz MAMI electron microtron for ${E}_{\ensuremath{\gamma}}=150--700$ MeV over a kinematic range which extends well beyond the approximately back-to-back detector arrangements of previous work. For ${}^{12}\mathrm{C}(\ensuremath{\gamma},np)$ the general trends of the missing energy distributions are reproduced over a wide range of kinematics and photon energies by the theory developed by the Valencia group. The corresponding ${}^{12}\mathrm{C}(\ensuremath{\gamma},pp)$ channel is overestimated by a factor of \ensurem…

PhysicsNuclear physicsNuclear and High Energy PhysicsRange (particle radiation)RecoilMissing energyPhotonYield (chemistry)Monte Carlo methodResonanceElectronAtomic physicsNuclear ExperimentPhysical Review C
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In-medium modifications of the pi pi interaction in photon-induced reactions

2002

Differential cross sections of the reactions $(\gamma,\pi^\circ\pi^\circ)$ and $(\gamma,\pi^\circ\pi^++\pi^\circ\pi^-)$ have been measured for several nuclei ($^1$H,$^{12}$C, and $^{\rm nat}$Pb) at an incident-photon energy of $E_{\gamma}$=400-460 MeV at the tagged-photon facility at MAMI-B using the TAPS spectrometer. A significant nuclear-mass dependence of the $\pi\pi$ invariant-mass distribution is found in the $\pi^\circ\pi^\circ$ channel. This dependence is not observed in the $\pi^\circ\pi^{+/-}$ channel and is consistent with an in-medium modification of the $\pi\pi$ interaction in the $I$=$J$=0 channel. The data are compared to $\pi$-induced measurements and to calculations within …

PhysicsPhotonMesonPAIRSHadronCarbon-12General Physics and AstronomyElementary particleNONPERTURBATIVE APPROACHCHIRAL-SYMMETRY RESTORATIONPionNUCLEAR MEDIUMPiSPECTROMETERMESONAtomic physicsNuclear ExperimentNuclear ExperimentMATTERBoson
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Measurement of the beam-helicity asymmetry I⊙ in the photoproduction of π0-pairs off the proton and off the neutron

2013

Abstract Beam-helicity asymmetries have been measured at the MAMI accelerator in Mainz for the photoproduction of neutral pion pairs in the reactions γ → p → p π 0 π 0 and γ → d → ( n ) p π 0 π 0 , γ → d → ( p ) n π 0 π 0 off free protons and off quasi-free nucleons bound in the deuteron for incident photon energies up to 1.4 GeV. Circularly polarized photons were produced from bremsstrahlung of longitudinally polarized electrons and tagged with the Glasgow magnetic spectrometer. Decay photons from the π 0 mesons, recoil protons, and recoil neutrons were detected in the 4π covering electromagnetic calorimeter composed of the Crystal Ball and TAPS detectors. After kinematic reconstruction of…

PhysicsNuclear and High Energy PhysicsProtonMeson010308 nuclear & particles physicsNuclear TheoryHadron01 natural sciences7. Clean energyHelicityCharged particleNuclear physicsPion0103 physical sciencesHigh Energy Physics::ExperimentNeutronAtomic physicsNuclear Experiment010306 general physicsCrystal BallPhysics Letters B
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Neutron polarizabilities investigated by quasi-free Compton scattering from the deuteron

2002

Measuring Compton scattered photons and recoil neutrons in coincidence, quasifree Compton scattering by the neutron has been investigated at MAMI (Mainz) at ${\ensuremath{\theta}}_{\ensuremath{\gamma}}^{\mathrm{lab}}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}136\ifmmode^\circ\else\textdegree\fi{}$ in an energy range from 200 to 400 MeV. From the data a polarizability difference of ${\ensuremath{\alpha}}_{n}\ensuremath{-}{\ensuremath{\beta}}_{n}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}9.8\ifmmode\pm\else\textpm\fi{}3.6(\mathrm{stat}{)}_{\ensuremath{-}1.1}^{+2.1}(\mathrm{syst})\ifmmode\pm\else\textpm\fi{}2.2(\mathrm{model})$ in units of ${10}^{\ensuremath{-}4}{\mathrm{fm}}^{…

Physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaCompton scatteringGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Deuterium0103 physical sciencesNeutronHigh Energy Physics::ExperimentAtomic physicsNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentEnergy (signal processing)Astrophysics::Galaxy Astrophysics
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Two-body photodisintegration of the deuteron from 100 to 800 MeV

1996

Abstract The total and the differential cross sections for the D(γ,p)n reaction have been measured over the photon energy range 100-800 MeV at the 855 MeV MAMI Microtron in Mainz. Using the large acceptance detector DAPHNE in conjunction with the Glasgow tagging spectrometer, high precision results with small systematic errors were obtained. The data are presented in the form of thirty-five angular distributions at c.m. proton angles between 30°–160° in 10° intervals and at photon energies in steps of 20 MeV. Previous experimental work is reassessed in the light of the present results and comparison with some recent theoretical calculations.

Nuclear physicsNuclear reactionPhysicsNuclear and High Energy PhysicsPhotonProtonDeuteriumSpectrometerPhotodisintegrationPhysics::Accelerator PhysicsPhoton energyNuclear ExperimentMicrotronNuclear Physics A
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Total photoabsorption cross section for4He from 200 to 800 MeV

1997

The total photoabsorption cross section for ${}^{4}$He has been measured for the first time over a wide photon energy range (200 MeV$l~{E}_{\ensuremath{\gamma}}l~$800 MeV). By using the large acceptance detector DAPHNE at the tagged photon facility of the MAMI microtron in Mainz high precision results with small systematic errors were obtained. This measurement shows that ${}^{4}$He has a behavior similar to heavy nuclei and, in particular, a reduction of the cross section with respect to the lighter nuclei is found for ${E}_{\ensuremath{\gamma}}g$600 MeV.

PhysicsSystematic errorMass numberNuclear and High Energy PhysicsRange (particle radiation)Light nucleusPhoton010308 nuclear & particles physicsNuclear TheoryPhoton energy01 natural sciencesNuclear physicsCross section (physics)0103 physical sciencesPhysics::Accelerator PhysicsAtomic physicsNuclear Experiment010306 general physicsMicrotronPhysical Review C
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Mass and Γ3π0/Γγγ decay branching ratio of theη-meson from the p(γ, η)p reaction

1995

Near threshold photoproduction ofη-mesons from the proton has been measured at the MAMI accelerator with the TAPS spectrometer. The mass of theη-meson was deduced from the threshold energy forη-photoproduction. The result of m η =(547.12 ± 0.06 ± 0.25) MeV supports the low value of theη-mass reported from a dp →3Heη measurement at SATURNE in 1992. Theη-decay branching ratio Γ3π0/Γγγ was measured to be (0.832±0.005±0.012).

Nuclear physicsPhysicsNuclear and High Energy PhysicsNear thresholdMesonSpectrometerProtonBranching fractionNuclear fusionThreshold energyZeitschrift für Physik A Hadrons and Nuclei
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First measurement of the helicity dependence of 3He photoreactions in the Δ(1232) resonance region

2013

The first measurement of the helicity dependence of the total inclusive 3He photo-absorption cross section and of the partial cross sections for several reaction channels was carried out at MAMI (Mainz) in the photon energy range between 150 and 500 MeV. The experiment used the large acceptance Crystal Ball spectrometer, complemented by charged particle and vertex detectors, a circularly polarised tagged photon beam and a longitudinally polarised high-pressure 3He gas target. The results obtained give information on the GDH integral on 3He and on the neutron and allow an investigation of the modifications of nucleon properties inside 3He.

PhysicsNuclear reactionNuclear and High Energy PhysicsPhoton010308 nuclear & particles physicsNuclear TheoryNucleon spin structurePhoton energy01 natural sciencesResonance (particle physics)HelicityNuclear physics0103 physical sciencesNeutronNuclear Experiment010306 general physicsCrystal BallPhysics Letters B
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POLARIZED 3HE TARGETS FOR REAL AND VIRTUAL PHOTONS

2011

PhysicsOpticsbusiness.industryVirtual particlebusinessPolarized targetPolarized Sources, Targets and Polarimetry
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The IceCube prototype string in Amanda

2006

The Antarctic Muon And Neutrino Detector Array (Amanda) is a high-energy neutrino telescope. It is a lattice of optical modules (OM) installed in the clear ice below the South Pole Station. Each OM contains a photomultiplier tube (PMT) that detects photons of Cherenkov light generated in the ice by muons and electrons. IceCube is a cubic-kilometer-sized expansion of Amanda currently being built at the South Pole. In IceCube the PMT signals are digitized already in the optical modules and transmitted to the surface. A prototype string of 41 OMs equipped with this new all-digital technology was deployed in the Amanda array in the year 2000. In this paper we describe the technology and demonst…

Antarctic Muon And Neutrino Detector ArrayAstroparticle physicsPhysicsNuclear and High Energy PhysicsPhotomultiplierPhotonMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Neutrino telescopeAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyAstrophysicsNeutrino telescopeAmandaIceCubeData acquisitionSignal digitizationAmanda; IceCube; Neutrino telescope; Signal digitizationInstrumentationCherenkov radiation
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Negative ions and their importance for the analysis of residual gas

1963

Abstract In the case of heavy molecules, mass spectre obtained with the help of positive ions generally lead to the recording of fragments only, and thus do not indicate the true original mass. In order to overcome this drawback, an attempt was made to attach slow electrons to heavy molecules, since less dissociation products are expected with spectre produced by negative ions. As a preliminary experiment, a simple and cheap form of ion source was constructed which produces mainly atomic negative ions.

ChemistryMoleculeElectronAtomic physicsCondensed Matter PhysicsResidualInstrumentationIon sourceDissociation (chemistry)Surfaces Coatings and FilmsIonVacuum
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Limits on the muon flux from neutralino annihilations at the center of the Earth with AMANDA

2006

A search has been performed for nearly vertically upgoing neutrino-induced muons with the Antarctic Muon And Neutrino Detector Array (AMANDA), using data taken over the three year period 1997–99. No excess above the expected atmospheric neutrino background has been found. Upper limits at 90% confidence level have been set on the annihilation rate of neutralinos at the center of the Earth, as well as on the muon flux at AMANDA induced by neutrinos created by the annihilation products.

Astroparticle physicsPhysicsAntarctic Muon And Neutrino Detector ArrayParticle physicsAMANDAAnnihilationMuonAMANDA; Dark matter; IceCube; Neutralino; Neutrino telescopesPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDark matterNeutralinoAstronomy and AstrophysicsIceCubeNuclear physicsWIMPNeutralinoDark matterHigh Energy Physics::ExperimentNeutrinoNeutrino telescopes
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Multiyear search for a diffuse flux of muon neutrinos with AMANDA-II

2007

A search for TeV - PeV muon neutrinos from unresolved sources was performed on AMANDA-II data collected between 2000 and 2003 with an equivalent livetime of 807 days. This diffuse analysis sought to find an extraterrestrial neutrino flux from sources with non-thermal components. The signal is expected to have a harder spectrum than the atmospheric muon and neutrino backgrounds. Since no excess of events was seen in the data over the expected background, an upper limit of E^{2}\Phi_{90% C.L.} < 7.4 x 10^{-8} GeV cm^{-2} s^{-1} sr^{-1} is placed on the diffuse flux of muon neutrinos with a \Phi \propto E^{-2} spectrum in the energy range 16 TeV to 2.5 PeV. This is currently the most sensitive…

Astroparticle physicsPhysicsNuclear and High Energy PhysicsRange (particle radiation)MuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFluxCosmic rayAstrophysicsAstrophysicsSpectral lineAstronomiaNeutron detectionddc:530High Energy Physics::ExperimentNeutrino
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Incoherent neutral pion photoproduction on 12C.

2007

We present the first detailed measurement of incoherent photoproduction of neutral pions to a discrete state of a residual nucleus. The C-12(gamma,pi(0))C-12(4.4 MeV)* reaction has been studied with the Glasgow photon tagger at MAMI employing a new technique which uses the large solid angle Crystal Ball detector both as a pi(0) spectrometer and to detect decay photons from the excited residual nucleus. The technique has potential applications to a broad range of future nuclear measurements with the Crystal Ball and similar detector systems elsewhere. Such data are sensitive to the propagation of the Delta in the nuclear medium and will give the first information on matter transition form fa…

PhysicsNuclear reactionPhotonMesonmeasurement of incoherent photoproduction010308 nuclear & particles physicsHadronNuclear TheoryGeneral Physics and AstronomyElementary particle01 natural sciences7. Clean energyNuclear physicsPionExcited state0103 physical sciencesAtomic physics010306 general physicsNuclear ExperimentCrystal BallPhysical review letters
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Measurement of coherent and incoherent π0 photoproduction off the deuteron with tagged photons up to the Δ region

2000

Coherent and incoherent pi(0) photoproduction off the deuteron has been measured for incident quasi-monoenergetic photons in the energy range from pi(0) threshold up to 300 MeV using the TAPS setup together with the Glasgow tagger at MAMI. Integral and differential cross sections over the full angular range have been obtained. Coherent and incoherent production are found to exhibit very different angle and energy dependences. The sum of both processes, the total pi(0) production off the deuteron is quantitatively extremely well described by a pure quasifree model, whereas the data for coherent and incoherent channels necessitate strong FSI effects for their description. Finally upper limits…

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Angular rangePhoton010308 nuclear & particles physicsNuclear Theory01 natural sciences7. Clean energyNuclear physicsDeuterium0103 physical sciencesAtomic physicsNuclear Experiment010306 general physicsNuclear Physics A
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Beam Asymmetry of Coherentπ° Photoproduction on4Hein theΔ(1232) Range Measured using Coherent Bremsstrahlung

1997

Using coherent bremsstrahlung at MAMI (Mainz), the beam asymmetry of the differential cross sections for coherent $\ensuremath{\pi}\ifmmode^\circ\else\textdegree\fi{}$ photoproduction on ${}^{4}\mathrm{He}$ has been measured in the energy interval from 200 to 500 MeV at an angle of ${\ensuremath{\theta}}_{\mathrm{lab}}\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}37\ifmmode^\circ\else\textdegree\fi{}$. The coherent ( $\ensuremath{\gamma},\ensuremath{\pi}\ifmmode^\circ\else\textdegree\fi{}$) reaction is used as a precise linear polarimeter for the first time. Agreement with predictions has been obtained on a $\ensuremath{\gtrsim}3%$ level of precision.

PhysicsParticle physicsRange (particle radiation)010308 nuclear & particles physicsmedia_common.quotation_subjectBremsstrahlungGeneral Physics and Astronomy01 natural sciencesAsymmetry0103 physical sciencesEnergy intervalAtomic physicsNuclear Experiment010306 general physicsBeam (structure)media_commonPhysical Review Letters
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Low-energy Compton scattering and the polarizabilities of the proton

2001

Differential cross-sections for Compton scattering from the proton have been measured at the MAMI tagged photon facility using the TAPS setup. The data cover an angular range of θlab γ = 59°-155° and photon energies ranging from 55 MeV to 165 MeV. Our results are in good agreement with those from previous experiments, but yield higher precision. Using dispersion relations the proton polarizabilities have been determined to be = [11.9±0.5stat.±1.3syst.±0.3mod.] . 10-4 fm 3 and = [1.2±0.7stat.±0.3syst.±0.4mod.)] . 10-4 fm 3. These results confirm the Baldin sum rule which was re-evaluated to be + = [13.8±0.4] . 10-4 fm 3. We can also conclude that there is no significant additional asymptotic…

PhysicsNuclear and High Energy PhysicsPhotonProton010308 nuclear & particles physicsHadronCompton scattering01 natural sciencesNuclear physicsPolarizabilityDispersion relation0103 physical sciencesSum rule in quantum mechanicsAtomic physics010306 general physicsSpin-½The European Physical Journal A
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Five years of searches for point sources of astrophysical neutrinos with the AMANDA-II neutrino telescope

2007

We report the results of a five-year survey of the northern sky to search for point sources of high energy neutrinos. The search was performed on the data collected with the AMANDA-II neutrino telescope in the years 2000 to 2004, with a live-time of 1001 days. The sample of selected events consists of 4282 upward going muon tracks with high reconstruction quality and an energy larger than about 100 GeV. We found no indication of point sources of neutrinos and set 90% confidence level flux upper limits for an all-sky search and also for a catalog of 32 selected sources. For the all-sky search, our average (over declination and right ascension) experimentally observed upper limit \Phi^{0}=(E/…

Astroparticle physicsPhysicsNuclear and High Energy PhysicsMuonAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectSolar neutrinoAstrophysics (astro-ph)High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSolar neutrino problemAstrophysicsSkyAstronomiaMeasurements of neutrino speedHigh Energy Physics::Experimentddc:530NeutrinoNeutrino astronomymedia_common
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Results from the AMANDA neutrino telescope

2004

The Amanda neutrino telescope at the South Pole has been taking data since 1996. Stepwise upgraded, it reached its final stage in January 2000. We present results from the search for extraterrestrial neutrinos, neutrinos from dark matter annihilation and magnetic monopoles.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyDark matterAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSolar neutrino problemAtomic and Molecular Physics and Opticslaw.inventionTelescopeNeutrino detectorlawMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNuclear Physics B - Proceedings Supplements
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Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

2002

The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 10^6 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05*10^9 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulat…

PhysicsAntarctic Muon And Neutrino Detector ArrayNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysicsSolar neutrino problemAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Neutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentddc:530Astrophysics::Earth and Planetary AstrophysicsNeutrinoNeutrino astronomyNeutrino oscillation
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12C(γ,π+n) and 12C(γ,π+p) reactions across the Δ resonance region

1997

Abstract Differential cross-sections from (γ,π+n) and (γ,π+p) experiments on 12C are presented together with a microscopic model calculation. The comparison of experimental data with theory confirms that quasifree pion production is the dominant process for the (γ,π+n) reaction. The comparison of (γ,π+p) with (γ,π+n) data shows the importance of final state interactions. first time to experimentally study the strength and the possible mechanisms involved in the final state interaction.

PhysicsNuclear and High Energy PhysicsCrystallographyPionAtomic physicsResonance (chemistry)Physics Letters B
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Three-nucleon mechanisms in photoreactions

2002

The $^{12}$C$(\gamma,ppn)$ reaction has been measured for E$_{\gamma}$=150-800 MeV in the first study of this reaction in a target heavier than $^3$He. The experimental data are compared to a microscopic many body calculation. The model, which predicts that the largest contribution to the reaction arises from final state interactions following an initial pion production process, overestimates the measured cross sections and there are strong indications that the overestimate arises in this two-step process. The selection of suitable kinematic conditions strongly suppresses this two-step contribution leaving cross sections in which up to half the yield is predicted to arise from the absorptio…

Nuclear physicsPhysicsNuclear and High Energy PhysicsPhotonPionYield (chemistry)FOS: Physical sciencesAbsorption (logic)Nuclear Experiment (nucl-ex)NucleonNuclear ExperimentNuclear ExperimentMany body
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Photoemission of protons from4He in theΔ-resonance region

1996

High resolution proton energy spectra from the4He(γ,p) reaction have been measured with tagged photons in the range Eγ = 130−525 MeV using the large Mainz NaI(T1) spectrometer atΘplab=37.1°. Three separate reaction channels were identified, viz.4He(γ,p)t two-body breakup,4He photodisintegration via two-nucleon photon absorption processes and the quasifree pion production channel. Differential cross sections are presented for each of these channels as a function of photon energy. The sum of the two-nucleon photon absorption and the quasifree pion production differential cross sections, in the CM system, resembles that of the corresponding free-nucleon differential cross section when Fermi mo…

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Photon010308 nuclear & particles physicsNuclear TheoryPhoton energy01 natural sciences7. Clean energyResonance (particle physics)Spectral lineNuclear physicsPionPhotodisintegration0103 physical sciencesAtomic physicsNuclear Experiment010306 general physicsAbsorption (electromagnetic radiation)Zeitschrift für Physik A: Hadrons and Nuclei
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Measurement of the Gerasimov-Drell-Hearn Integrand forH2from 200 to 800 MeV

2006

A measurement of the helicity dependence of the total inclusive photoabsorption cross section on the deuteron was carried out at MAMI (Mainz) in the energy range $200l{E}_{\ensuremath{\gamma}}l800\text{ }\text{ }\mathrm{MeV}$. The experiment used a $4\ensuremath{\pi}$ detection system, a circularly polarized tagged photon beam and a frozen-spin target which provided longitudinally polarized deuterons. The contribution to the Gerasimov-Drell-Hearn sum rule for the deuteron determined from the data is $407\ifmmode\pm\else\textpm\fi{}20(\mathrm{stat})\ifmmode\pm\else\textpm\fi{}24(\mathrm{syst})\text{ }\text{ }\ensuremath{\mu}\mathrm{b}$ for $200l{E}_{\ensuremath{\gamma}}l800\text{ }\text{ }\m…

PhysicsParticle physicsMeson production010308 nuclear & particles physicsNuclear TheoryGeneral Physics and AstronomyComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)01 natural sciencesHelicityNuclear physics0103 physical sciencesSum rule in quantum mechanicsPhoton beamNuclear Experiment010306 general physicsEnergy (signal processing)Physical Review Letters
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Nuclear pion photoproduction in theΔresonance region

1999

A measurement of the /sup 12/C( gamma , pi /sup +/n)/sup 11/B reaction in quasifree pi -production kinematic regimes has been performed using tagged photons in conjunction with large solid angle pi and n detectors. The aim of the experiment was to investigate predicted modifications to the Delta excitation of nucleons and their subsequent propagation and decay, brought about by the nuclear medium. Differential cross sections are presented for photon energies spanning the Delta (1232) excitation region. The measurements are consistent with distorted wave impulse approximation calculations in which the amplitude for proton Delta excitation, followed by Delta propagation and decay to pi /sup +…

Nuclear physicsPhysicsDeltaNuclear and High Energy PhysicsPionAmplitudePhotonSolid angleImpulse (physics)Atomic physicsNucleonExcitationPhysical Review C
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Helicity dependence of the total inclusive cross section on the deuteron

2009

Abstract A measurement of the helicity dependence of the total inclusive photoabsorption cross section on the deuteron was carried out at MAMI (Mainz) in the energy range 200 E γ 800 MeV . The experiment used a 4 π detection system, a circularly polarized tagged photon beam and a frozen spin target which provided longitudinally polarized deuterons. These new results are a significant improvement on the existing data and allow a detailed comparison with state-of-the-art calculations.

PhysicsAngular momentumRange (particle radiation)Nuclear and High Energy PhysicsNuclear TheoryPolarization (waves)HelicityDeuteron photoabsorptionCharged particleNuclear physicsCross section (physics)DeuteriumPhysics and AstronomyDouble polarization experimentSpin (physics)Nuclear ExperimentPhysics Letters B
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IceCube: A multipurpose neutrino telescope

2008

IceCube is a new high-energy neutrino telescope which will be coming online in the near future. IceCube will be capable of measuring fluxes of all three flavors of neutrino, and its peak neutrino energy sensitivity will be in the TeV–PeV range. Here, after a brief description of the detector, we describe its anticipated performance with a selection of physics topics: supernovae, extraterrestrial diffuse and point sources of neutrinos, gamma-ray bursts, neutrinos from WIMP annihilation, and cosmic ray composition.

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoGeneral Physics and AstronomyAstrophysics7. Clean energy01 natural sciencesWIMP0103 physical sciencesNeutrinos010306 general physicsCosmic rays; Neutrinos; WIMPsCosmic raysPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomySolar neutrino problemWIMPsCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

2006

The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN mode…

AMANDAActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsIceCubeLuminosityAGNNeutrinosBlazarAstrophysics::Galaxy AstrophysicsAGN; AMANDA; IceCube; Neutrinos; Point sources; Source stackingAstroparticle physicsPhysicsAstrophysics (astro-ph)Point sourcesAstronomyAstronomy and AstrophysicsQuasarSource stackingNeutrino detectorAstronomiaHigh Energy Physics::ExperimentNeutrino
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Backward spin polarizabilityγπof the proton

2002

Using the Mainz $48\mathrm{cm}\ensuremath{\emptyset}\ifmmode\times\else\texttimes\fi{}64\mathrm{cm}$ NaI(Tl) detector and the segmented G\"ottingen recoil detector SENECA in coincidence, Compton scattering by the proton at ${\ensuremath{\theta}}_{\ensuremath{\gamma}}^{\mathrm{lab}}=136\ifmmode^\circ\else\textdegree\fi{}$ has been measured at MAMI (Mainz) in the energy range from 200 to 470 MeV. The new data confirm the previous observation that there is a systematic discrepancy between MAMI and LEGS (Brookhaven) data leading to different spin polarizabilities ${\ensuremath{\gamma}}_{\ensuremath{\pi}}=\ensuremath{-}38.7\ifmmode\pm\else\textpm\fi{}1.8$ and $\ensuremath{-}27.2\ifmmode\pm\else\…

Elastic scatteringPhysicsNuclear and High Energy PhysicsParticle physicsProton010308 nuclear & particles physicsHadronElementary particle01 natural sciencesOrientation (vector space)Nuclear physicsBaryon0103 physical sciences010306 general physicsNucleonEnergy (signal processing)Physical Review C
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Two neutral pion photoproduction off the proton between threshold and 800 MeV

1997

Abstract The photoproduction of two neutral pions off the proton has been studied for incident photon energies between E γ = 309 MeV (threshold) and 792 MeV with the TAPS photon spectrometer at the Mainz Microtron MAMI. Both 3γ- and 4γ-events have been analysed in order to deduce the total p ( γ , 2 π 0 ) p cross section. The total cross section is less than 300 nb between threshold and ⋍ 460 MeV, beyond which it starts to rise to a maximum value of about 11 μb at around 750 MeV. For the highest energies it starts to decrease again. The 4γ-sample has been used to reconstruct 2 neutral pions from the above reaction channel by an invariant mass and a missing mass analysis. After reconstructio…

PhysicsNuclear physicsNuclear and High Energy PhysicsPionPhotonProtonIntermediate stateDalitz plotInvariant massDecay chainAtomic physicsMicrotronPhysics Letters B
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Measurement of the Parity Violation in Quasi-Elastic Electroweak Electron-Scattering from 9Be

1986

In the energy range of about 300 MeV, available at the Mainz- Linac, quasi-elastic scattering dominates the total cross section at backward scattering angles. This process can therefore be detected efficiently by a gas Cerenkov-counter with large solid angle. This is a prerequisit for experiments on parity violation due to the very small asymmetry effect being of the order of 1|10-5 at these energies [1]. The counting system built, consists of 12 elliptical mirrors, imaging the Cerenkov photons seen in target direction onto photomultipliers. The mirrors cover the full azimuth for polar angles 115°≦ϑ≦145°, thus covering 20% of 4π (Fig. 1). The detector has been proved to yield a statistical …

PhysicsAzimuthParticle physicsPhotonScatteringmedia_common.quotation_subjectElectroweak interactionSolid angleElectronAsymmetryElectron scatteringComputational physicsmedia_common
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Photoproduction ofπ0Mesons off Neutrons in the Nucleon Resonance Region

2014

Precise angular distributions have been measured for the first time for the photoproduction of π0 mesons off neutrons bound in the deuteron. The effects from nuclear Fermi motion have been eliminated by a complete kinematic reconstruction of the final state. The influence of final-state-interaction effects has been estimated by a comparison of the reaction cross section for quasifree protons bound in the deuteron to the results for free protons and then applied as a correction to the quasifree neutron data. The experiment was performed at the tagged photon facility of the Mainz Microtron MAMI with the Crystal Ball and TAPS detector setup for incident photon energies between 0.45 and 1.4 GeV…

PhysicsParticle physicsMesonProtonNuclear TheoryGeneral Physics and AstronomyPhoton energy7. Clean energyNuclear physicsIsospinNeutronNuclear ExperimentNucleonMicrotronCrystal BallPhysical Review Letters
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First measurement of helicity-dependent cross sections in π0η photoproduction from quasi-free nucleons

2018

The helicity-dependent cross sections for the photoproduction of $\pi^0\eta$ pairs have been measured for the first time. The experiment was performed at the tagged photon facility of the Mainz MAMI accelerator with the combined Crystal Ball - TAPS calorimeter. The experiment used a polarized deuterated butanol target and a circularly polarized photon beam. This arrangement allowed the $\sigma_{1/2}$ (photon and target spin antiparallel) and $\sigma_{3/2}$ (parallel spins) components to be measured for quasi-free production of $\pi^0\eta$ pairs off protons and neutrons. The main finding is that the two helicity components contribute identically, within uncertainties, for both participant pr…

Nuclear and High Energy PhysicsPhotonNuclear TheoryFOS: Physical sciences7. Clean energy01 natural sciencesNuclear physicsPion0103 physical sciencesNeutronddc:530Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentSpin-½Physics010308 nuclear & particles physicsPhysicsHelicitylcsh:QC1-9993. Good healthDeuteriumNucleonlcsh:PhysicsCrystal Ballreaction gamma-p ; polarization ; eta ; mesons ; mami ; Pi(0)-pairs ; photon ; proton ; pairs
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Results from the Real Photon Programme at MAMI

1995

The accelerator MAMI (Mainzer Mikrotron) with its excellent beam properties and its duty factor of 100% allows to apply coincidence techniques in intermediate energy nuclear physics, which has led to a variety of results with high precision. The real photon collaboration (A2) uses energy tagged bremsstrahlung photons with energies up to 800 MeV. We have results on total photon absorption (proton, deuteron, 3He and U), on Compton scattering (proton, 4He and 12C) and on meson production, especially on π°- and η-photoproduction. Double pion production on the proton and the deuteron was measured. The two and three body breakup of 3He was investigated as well as the reactions (γ,NN) and (γ, π ± …

PhysicsNuclear physicsPhotonPionProtonDeuteriumNuclear TheoryCompton scatteringBremsstrahlungPhysics::Accelerator PhysicsNuclear ExperimentAbsorption (electromagnetic radiation)Coincidence
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Limits to the muon flux from neutralino annihilations in the Sun with the AMANDA detector

2005

A search for an excess of muon-neutrinos from neutralino annihilations in the Sun has been performed with the AMANDA-II neutrino detector using data collected in 143.7 days of live-time in 2001. No excess over the expected atmospheric neutrino background has been observed. An upper limit at 90% confidence level has been obtained on the annihilation rate of captured neutralinos in the Sun, as well as the corresponding muon flux limit at the Earth, both as functions of the neutralino mass in the range 100 GeV-5000 GeV.

Astroparticle physicsPhysicsParticle physicsRange (particle radiation)AMANDAMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorDark matterHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)NeutralinoFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAMANDA; Dark matter; Neutralino; Neutrino telescopesNuclear physicsNeutrino detectorNeutralinoMuon fluxDark matterHigh Energy Physics::ExperimentNeutrino telescopes
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Single and double πo-photoproduction from the deuteron

1999

Photoproduction of neutral pions from the deuteron has been studied for incident photon energies from 200 MeV to 792 MeV with the TAPS detector at the Mainz MAMI accelerator. Total and differential cross sections covering the full angular range have been obtained for coherent and incoherent single πo-photoproduction. Good agreement between model predictions and the data was found for the coherent process. The incoherent cross section in the energy region of the Δ(1232)-resonance is overestimated by existing models. A comparison to model predictions indicates that final state interaction effects are much more important than for the coherent reaction. However, the angular dependence of the da…

PhysicsNuclear and High Energy PhysicsPhotonProtonNuclear TheoryHadronResonance (particle physics)Nuclear physicsPionDeuteriumNeutronAtomic physicsNuclear ExperimentNucleonThe European Physical Journal A
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Angular and polarization dependence of Compton scattering from in the Δ-resonance region

1998

Abstract Using linearly polarized tagged photons from coherent bremsstrahlung, differential cross sections and beam asymmetries for Compton scattering by 4 He have been measured at MAMI in the energy interval between 150 MeV and 500 MeV for scattering angles of θ γ lab =37°, 93° and 137°, thus largely increasing the available data base. Improved calculations in terms of the Δ -hole model completely fail to describe the data at large scattering angles. The same proved to be true for a schematic model, even after taking into account properties of nuclear photo-absorption in very detail.

PhysicsNuclear and High Energy PhysicsPhoton010308 nuclear & particles physicsScatteringCompton scatteringScattering lengthInelastic scatteringMott scattering01 natural sciencesSmall-angle neutron scatteringNuclear physicsX-ray Raman scattering0103 physical sciencesNuclear Experiment010306 general physicsPhysics Letters B
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Helicity Dependence ofγp→Nπbelow 450 MeV and Contribution to the Gerasimov-Drell-Hearn Sum Rule

2000

The helicity dependence of the single pion photoproduction on the proton has been measured in the energy range from 200 to 450 MeV for the first time. The experiment, performed at the Mainz microtron MAMI, used a 4pi-detector system, a circularly polarized, tagged photon beam, and a frozen-spin target. The data obtained provide new information for multipole analyses of pion photoproduction and determine the main contributions to the Gerasimov-Drell-Hearn sum rule and the forward spin polarizability gamma(0).

PhysicsParticle physicsProtonNuclear TheoryGeneral Physics and AstronomyHelicityNuclear physicsPionPolarizabilityPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentSum rule in quantum mechanicsNuclear ExperimentMultipole expansionMicrotronSpin-½Physical Review Letters
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Measurement of theE2/M1Ratio in theN→ΔTransition Using the Reactionp(γ→,p)π0[Phys. Rev. Lett. 78, 606 (1997)]

1997

The small electric quadrupole $E2$ amplitude of the predominantly magnetic dipole $M1$ $p\ensuremath{\rightarrow}\ensuremath{\Delta}(1232)$ transition has been measured using 270 to 420 MeV tagged linearly polarized photons in the $p(\stackrel{\ensuremath{\rightarrow}}{\ensuremath{\gamma}},p){\ensuremath{\pi}}^{o}$ reaction at the Mainz Microtron MAMI. Differential cross sections and photon asymmetries were determined by measuring the recoil proton in the cylindrically symmetric $4\ensuremath{\pi}$ detector DAPHNE. From the proton angular distributions the ratio $E2/M1\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}\ensuremath{-}(2.5\ifmmode\pm\else\textpm\fi{}0.2\ifmmode\pm\else\textpm\…

Recoil protonPhysicsAngular distributionAmplitudePhotonProtonQuantum mechanicsQuadrupoleResonanceGeneral Physics and AstronomyAtomic physicsNuclear ExperimentMagnetic dipolePhysical Review Letters
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Radiative Pion Photoproduction from the Proton and π + Meson Polarizabilities

1995

We study the possibility of investigating radiative pion photoproduction from the proton at the microtron MAMI-B with the aim to obtain an experimental information about the π + meson polarizabilities. It is shown that an exposition time of about 30 days will allow to determine the π + meson polarizability with quite high accuracy.

PhysicsTriple coincidenceParticle physicsMesonProtonHigh Energy Physics::LatticeNuclear TheoryPionPolarizabilityRadiative transferNeutron detectionHigh Energy Physics::ExperimentNuclear ExperimentMicrotron
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Double- π0 photoproduction from the deuteron

2000

The photoproduction of two neutral pions from the deuteron has been studied for incident photon energies from 200 MeV to 820 MeV with the TAPS spectrometer at MAMI (Mainz Microtron). The total cross-section was determined and used to deduce the cross-section from the neutron. Due to the good statistical quality of the data Dalitz plots for the three particles in the exit channel (pi (0)pi N-0) could be constructed. The invariant mass distributions derived from them are presented in this paper. They indicate that the important reaction mechanism in the second resonance region is a sequential decay pattern involving the population of the Delta (1232)-resonance as an intermediate state.

PhysicsNuclear and High Energy Physicseducation.field_of_study010308 nuclear & particles physicsNuclear TheoryHadronPopulation01 natural sciencesResonance (particle physics)Nuclear physicsPionDeuterium0103 physical sciencesNeutronInvariant massAtomic physicsNuclear Experiment010306 general physicseducationMicrotronThe European Physical Journal A
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Elastic and inelastic photon scattering from 12C

1994

Abstract The elastic and inelastic photon scattering from 12 C was investigated in the energy range of the Δ-resonance ( E γ = 200–500 MeV) at a scattering angle of 40°. The experiment was performed with the tagged photon facility at the cw electron accelerator MAMI ( E e − = 855 MeV). By using a large NaI(Tl) detector having an energy resolution of 1.5%, the elastic scattering could be separated from the inelastic process to the first excited state ( E x = 4.44 MeV of 12 C. The differential cross section for the coherent scattering is compared with a simple static ansatz, that uses the known charge form factor, and with a recent Δ-hole calculation.

PhysicsElastic scatteringNuclear and High Energy PhysicsQuasielastic scattering010308 nuclear & particles physicsScatteringScattering lengthMott scatteringInelastic scatteringDeep inelastic scattering7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesScattering theoryAtomic physics010306 general physicsPhysics Letters B
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Compton scattering from the free and bound proton above π-threshold

2000

The differential cross sections for Compton scattering from the proton have been measured at MAMI with three different detector setups. There is a good agreement among all the results. The theoretical calculation based on dispersion relations shows that there is no drastic change necessary in the parameters of this approach.

PhysicsNuclear and High Energy PhysicsProton010308 nuclear & particles physicsDetectorCompton scatteringCompton wavelengthInelastic scattering01 natural sciencesNuclear physicsDispersion relation0103 physical sciencesNuclear Experiment010306 general physics
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Narrow Structure in the Excitation Function of eta Photoproduction off the Neutron

2013

The photoproduction of $\eta$-mesons off nucleons bound in $^2$H and $^3$He has been measured in coincidence with recoil protons and recoil neutrons for incident photon energies from threshold up to 1.4 GeV. The experiments were performed at the Mainz MAMI accelerator, using the Glasgow tagged photon facility. Decay photons from the $\eta\rightarrow 2\gamma$ and $\eta\rightarrow 3\pi^0$ decays and the recoil nucleons were detected with an almost $4\pi$ electromagnetic calorimeter combining the Crystal Ball and TAPS detectors. The data from both targets are of excellent statistical quality and show a narrow structure in the excitation function of $\gamma n\rightarrow n\eta$. The results from…

ProtonMesonNuclear TheoryFOS: Physical sciencesGeneral Physics and AstronomyPhysics::OpticsPhoton energyη; meson; photoproduction off the neutron; MAMI01 natural sciences7. Clean energyNuclear physicsRecoil0103 physical sciencesNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsExcitation function010308 nuclear & particles physicsPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentAtomic physicsNucleonCrystal BallPHYSICAL REVIEW LETTERS
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Polarized photon measurements of the12C(γ→,pp)and12C(γ→,pn)reactions forEγ=160−350MeV

2001

The ${}^{12}\mathrm{C}(\stackrel{\ensuremath{\rightarrow}}{\ensuremath{\gamma}},pp)$ and ${}^{12}\mathrm{C}(\stackrel{\ensuremath{\rightarrow}}{\ensuremath{\gamma}},pn)$ reactions have been studied for ${E}_{\ensuremath{\gamma}}=160\ensuremath{-}350$ MeV using linearly polarized photons from the Glasgow tagged photon spectrometer at the Mainz microtron MAMI. Both reaction channels show a negative photon asymmetry $\ensuremath{\Sigma}$ for missing energies ${E}_{m}$ below 70 MeV, where direct emission nucleon pairs is expected. A strong peak at low ${E}_{m}$ is observed in ${\ensuremath{\Sigma}}_{(\ensuremath{\gamma},pp)},$ but not in ${\ensuremath{\Sigma}}_{(\ensuremath{\gamma},pn)}.$ Furth…

PhysicsNuclear and High Energy PhysicsPhotonPionmedia_common.quotation_subjectNuclear TheoryProduction (computer science)Angular dependenceAtomic physicsNuclear ExperimentNucleonAsymmetrymedia_commonPhysical Review C
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Compton Scattering by the Proton using a Large-Acceptance Arrangement

2001

Compton scattering by the proton has been measured over a wide range covering photon energies 250 MeV lt or approximately=E/sub gamma / lt or approximately=800 MeV and photon scattering angles 30 degrees lt or approximately= theta /sub gamma //sup lab/ lt or approximately=150 degrees , using the tagged-photon facility at MAMI (Mainz) and the large-acceptance arrangement LARA. The previously existing data base on proton Compton scattering is greatly enlarged by more than 700 new data points. The new data are interpreted in terms of dispersion theory based on the SAID-SM99K parametrization of photo-meson amplitudes. It is found that two-pion exchange in the t-channel is needed for a descripti…

Nuclear and High Energy PhysicsProtonNuclear TheoryFOS: Physical sciencesValue (computer science)01 natural sciencesResonance (particle physics)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Dispersion relation0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentQCSpin-½Physics010308 nuclear & particles physicsCompton scatteringHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics::ExperimentMultipole expansion
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Muon track reconstruction and data selection techniques in AMANDA

2004

The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500m and 2000m. The primary goal of this detector is to discover astrophysical sources of high energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of r…

Antarctic Muon And Neutrino Detector ArrayPhysicsAMANDANuclear and High Energy PhysicsParticle physicsAMANDA; Neutrino astrophysics; Neutrino telescope; Track reconstructionMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)DetectorFOS: Physical sciencesAstrophysicsNeutrino telescopeTrack reconstructionNeutrino astrophysicsIceCube Neutrino ObservatoryNeutrino detectorHigh Energy Physics::ExperimentMuon neutrinoNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationLeptonNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Angular distribution of scattered electrons associated with collimated bremsstrahlung and the tagging technique

2009

Abstract We investigate the angular correlation between a bremsstrahlung photon and its corresponding post-bremsstrahlung electron within the context of a magnetic tagging spectrometer with the aim of improving the instrument's efficiency. Our results are given in terms of angular distributions of the post-bremsstrahlung electron associated with photons that pass through a circular collimator centered in the forward direction. We start from the fully differential Bethe–Heitler (first Born approximation) cross-section, including the Moliere screening correction, which is then integrated over the photon azimuthal angle and over the photon polar angle defined by the collimator. These integrati…

PhysicsNuclear and High Energy PhysicsPhotonbusiness.industryBremsstrahlungCollimatorElectronSmall-angle approximationCollimated lightlaw.inventionAzimuthOpticslawBorn approximationbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Status of the IceCube Neutrino Observatory

2004

Abstract The IceCube neutrino telescope, to be constructed near the Antarctic South Pole, represents the next generation of neutrino telescope. Its large 1 km3 size will make it uniquely sensitive to the detection of neutrinos from astrophysical sources. The current design of the detector is presented. The basic performance of the detector and its ability to search for neutrinos from various astrophysical sources has been studied using detailed simulations and is discussed.

PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrophysicsSolar neutrino problemIceCube Neutrino Observatorylaw.inventionTelescopeNeutrino detectorSpace and Planetary SciencelawMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNew Astronomy Reviews
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Search for Supernova Neutrino-Bursts with the AMANDA Detector

2001

The core collapse of a massive star in the Milky Way will produce a neutrino burst, intense enough to be detected by existing underground detectors. The AMANDA neutrino telescope located deep in the South Pole ice can detect MeV neutrinos by a collective rate increase in all photo-multipliers on top of dark noise. The main source of light comes from positrons produced in the CC-reaction of anti-electron neutrinos on free protons $\antinue + p \to e^+ + n$. This paper describes the first supernova search performed on the full sets of data taken during 1997 and 1998 (215 days of live time) with 302 of the detector's optical modules. No candidate events resulted from this search. The performan…

PhysicsPhysics::Instrumentation and DetectorsMilky WayAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)DetectorFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxySupernovaPositronHigh Energy Physics::ExperimentNeutrinoCharged currentAstrophysics::Galaxy AstrophysicsDark current
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The Reactionγp→π0γ′pand the Magnetic Dipole Moment of theΔ+(1232)Resonance

2002

The reaction $\ensuremath{\gamma}p\ensuremath{\rightarrow}{\ensuremath{\pi}}^{0}{\ensuremath{\gamma}}^{\ensuremath{'}}p$ has been measured with the TAPS calorimeter at the Mainz Microtron accelerator facility MAMI for energies between $\sqrt{s}=1221--1331\text{ }\text{ }\mathrm{M}\mathrm{e}\mathrm{V}$. The cross section's differential in angle and energy have been determined for the photon ${\ensuremath{\gamma}}^{\ensuremath{'}}$ in three bins of the excitation energy. This reaction channel provides access to the magnetic dipole moment of the ${\ensuremath{\Delta}}^{+}(1232)$ resonance and, for the first time, a value of ${\ensuremath{\mu}}_{{\ensuremath{\Delta}}^{+}}=\mathbf{[}{2.7}_{\ensu…

BaryonPhysicsCrystallographyParticle physicsAngular distributionMagnetic momentPiGeneral Physics and AstronomyResonanceNuclear ExperimentEnergy (signal processing)Physical Review Letters
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Direct Observation of aρDecay of theD13(1520)Baryon Resonance

2001

The reaction {gamma}p{yields}{pi}{sup +}{pi}{sup 0}n has been measured at MAMI for photon energies up to 820MeV. Invariant mass spectra of the particles in the final state ({pi}{sup +}n) , ({pi}{sup 0}n) , ({pi}{sup +}{pi}{sup 0}) have been determined for several bins of incident photon energy. Differences in {pi}{sup +}{pi}{sup 0} and simultaneously measured {pi}{sup 0}{pi}{sup 0} invariant mass distributions are assigned to a {rho} branch of the D{sub 13}(1520) nucleon resonance.

PhysicsProton010308 nuclear & particles physicsGeneral Physics and AstronomyResonancePhoton energy01 natural sciencesSpectral lineBaryon0103 physical sciencesMass spectrumInvariant massAtomic physics010306 general physicsNucleonPhysical Review Letters
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Measurements of Double-Polarized Compton Scattering Asymmetries and Extraction of the Proton Spin Polarizabilities

2015

The spin polarizabilities of the nucleon describe how the spin of the nucleon responds to an incident polarized photon. The most model-independent way to measure the nucleon spin polarizabilities is through polarized Compton scattering. Double-polarized Compton scattering asymmetries on the proton were measured in the $\Delta(1232)$ region using circularly polarized incident photons and a transversely polarized proton target at the Mainz Microtron. Fits to asymmetry data were performed using a dispersion model calculation and a baryon chiral perturbation theory calculation, and a separation of all four proton spin polarizabilities in the multipole basis was achieved. The analysis based on a…

PhysicsPhotonProtonNuclear TheoryCompton scatteringGeneral Physics and AstronomyFOS: Physical sciences7. Clean energy3. Good healthBaryonNuclear physicsProton spin crisisspin polarizabilities; nucleon; photon; ∆(1232) region; MAMINuclear Experiment (nucl-ex)NucleonNuclear ExperimentMicrotronNuclear ExperimentSpin-½
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Experimental Check of the Gerasimov-Drell-Hearn Sum Rule for H1

2004

For the first time we checked the fundamental Gerasimov-Drell-Hearn (GDH) sum rule for the proton experimentally in the photon energy range from 0.2-2.9 GeV with the tagged photon facilities at MAMI (Mainz) and ELSA (Bonn). New data of the doubly polarized total cross section difference are presented in the energy range from 1.6 to 2.9 GeV. The contribution to the GDH integral from 0.2-2.9 GeV yields [254+/-5(stat)+/-12(syst)] microb with negative contributions in the Regge regime at photon energies above 2.1 GeV. This trend supports the validity of the GDH sum rule.

PhysicsRange (particle radiation)PhotonProton010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and AstronomyPhoton energy01 natural sciencesNuclear physicsRegge theory0103 physical sciencesHigh Energy Physics::ExperimentSum rule in quantum mechanicsNuclear Experiment010306 general physicsAstrophysics::Galaxy AstrophysicsPhysical Review Letters
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Near threshold photoproduction of η mesons from 4 He

1999

Photoproduction of η mesons from 4He has been measured for the first time. The experiment was performed at the Mainz Microtron (MAMI) using the TAPS photon spectrometer and the Glasgow/Mainz tagged photon facility. η mesons were identified in coincidence with recoil nucleons. Total and differential cross sections are presented in the photon energy range between threshold and 818 MeV. The exclusive data are used to determine the ratio of the elementary production cross sections on bound neutrons and protons, σn/σp= 0.68 ± 0.02 ± 0.09. In addition, upper limits for the total coherent cross section have been derived.

PhysicsNuclear and High Energy PhysicsParticle physicsPhotonMeson010308 nuclear & particles physicsNuclear TheoryHadronPhoton energy01 natural sciences7. Clean energyNuclear physicsRecoil0103 physical sciencesHigh Energy Physics::ExperimentNeutronNuclear Experiment010306 general physicsNucleonMicrotronThe European Physical Journal A
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New experimental method for investigation of the nucleon polarizabilities

2010

Abstract At the continuous wave (cw) Superconducting Darmstadt Electron Linear Accelerator S-DALINAC, a new method has been developed for the determination of the electric ( α ¯ ) and magnetic ( β ¯ ) polarizabilities of the proton and the deuteron. For that purpose the energy and angular dependence of the differential cross-section for elastic γ p and γ d scattering of bremsstrahlung photons in the energy range between 20 and 100 MeV is measured by detecting the recoiling proton (deuteron) in coincidence with the scattered bremsstrahlung photon. α ¯ and β ¯ are then found by means of a best fit to a theoretical description of the scattering cross-section with these quantities as open param…

PhysicsNuclear and High Energy PhysicsPhotonProtonScatteringBremsstrahlungCompton scatteringNuclear physicsDeuteriumIonizationPhysics::Accelerator PhysicsAtomic physicsNuclear ExperimentNucleonInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Double Pion Photoproduction on the Proton up to 800 MeV

1995

The total cross sections for the three γp → N ππ reactions have been measured for photon energies from 450 to 800 MeV. The γp → pπ0π0 and γp → nπ+π0 rcross sections have never been measured before while the γp → pπ+π− results are much improved compared to earlier data. These measurements were performed with the large acceptance hadronic detector DAPHNE, at the tagged photon beam facility of MAMI microtron in Mainz.

PhysicsNuclear physicsPhotonPionProtonHadronDetectorPhoton beamMicrotron
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Threshold enhancement in η photoproduction from 2H and 4He

2002

The photoproduction of η-mesons from 2H and 4He has been studied for energies close to the production thresholds. The experiments were carried out with the tagged photon beam of the Mainz MAMI accelerator. The η-mesons were detected via their two photon decays with the electromagnetic calorimeter TAPS. Total cross-sections, angular and momentum distributions of the η-mesons have been determined for both reactions. The total cross-sections in the threshold region show a large enhancement over the predictions of a participant-spectator model, indicating significant final-state interaction effects. The results are compared to recent model calculations taking into account nucleon-nucleon and nu…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsNuclear TheoryHadron01 natural sciences7. Clean energyNuclear physicsMomentumElectromagnetic calorimeter0103 physical sciencesNuclear fusionHigh Energy Physics::ExperimentAtomic physicsPhoton beamNuclear Experiment010306 general physicsThe European Physical Journal A
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"Table 6" of "In-medium modifications of the pi pi interaction in photon-induced reactions."

2005

Differential cross section for PI0PI+/- production with a Lead target. Errors are statistical only.

Single Differential Cross SectionPhotoproductionDSIG/DMGAMMA PB --&gt; PI0 PI+GAMMA PB --&gt; PI0 PI-ExclusiveGAMMA NUCLEUS --&gt; PI- PI0GAMMA NUCLEUS --&gt; PI+ PI0
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"Table 2" of "In-medium modifications of the pi pi interaction in photon-induced reactions."

2005

Differential cross section for PI0PI0 production with a Carbon target. Errors are statistical only.

GAMMA NUCLEUS --&gt; PI0 PI0Single Differential Cross SectionPhotoproductionDSIG/DMGAMMA C --&gt; PI0 PI0Exclusive
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"Table 1" of "In-medium modifications of the pi pi interaction in photon-induced reactions."

2005

Differential cross section for PI0PI0 production with a proton target. Errors are statistical only. Note that the data given in this table are sightly different (newer) than the data points presented in the paper.

Single Differential Cross SectionGAMMA P --&gt; PI0 PI0PhotoproductionDSIG/DMExclusive1.277-1.32
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"Table 4" of "In-medium modifications of the pi pi interaction in photon-induced reactions."

2005

Differential cross section for PI0PI+ production with a proton target. Errors are statistical only. Note that the data given in this table are sightly different (newer) than the data points presented in the paper.

Single Differential Cross SectionPhotoproductionDSIG/DMExclusiveGAMMA P --&gt; PI0 PI+1.277-1.32
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"Table 3" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the triple differential cross section w.r.t. the scattered proton.

PhotoproductionTriple Differential Cross SectionExclusiveGAMMA DEUT --&gt; GAMMA P NNuclear ExperimentD3SIG/DE/DOMEGA/DOMEGA
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"Table 3" of "In-medium modifications of the pi pi interaction in photon-induced reactions."

2005

Differential cross section for PI0PI0 production with a Lead target. Errors are statistical only.

GAMMA NUCLEUS --&gt; PI0 PI0Single Differential Cross SectionPhotoproductionDSIG/DMExclusiveGAMMA PB --&gt; PI0 PI0
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"Table 1" of "Compton scattering from the free and bound proton at backward angles above pi threshold."

2000

No description provided.

Single Differential Cross SectionPhotoproduction1.12-1.284GAMMA P --&gt; P GAMMAExclusiveDSIG/DOMEGA
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"Table 1" of "Double pi0 photoproduction off the proton at threshold."

2004

Total cross section measurement. Statistical errors only.

PhotoproductionIntegrated Cross SectionGAMMA P --&gt; PI0 PI0 PExclusiveCross SectionSIG1.211-1.289
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"Table 2" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the quasi-free proton differential cross section.

Single Differential Cross SectionPhotoproduction1.146-1.266ElasticNuclear TheoryPhysics::Accelerator PhysicsGAMMA P --&gt; GAMMA PNuclear ExperimentDSIG/DOMEGA
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"Table 5" of "In-medium modifications of the pi pi interaction in photon-induced reactions."

2005

Differential cross section for PI0PI+/- production with a Carbon target. Errors are statistical only.

GAMMA C --&gt; PI0 PI-Single Differential Cross SectionGAMMA C --&gt; PI0 PI+PhotoproductionDSIG/DMExclusiveGAMMA NUCLEUS --&gt; PI- PI0GAMMA NUCLEUS --&gt; PI+ PI0
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"Table 1" of "Total photoabsorption cross-section for He-4 from 200-MeV to 800-MeV"

1998

No description provided.

PhotoproductionGAMMA HE --&gt; INELASTICIntegrated Cross SectionExclusiveCross SectionSIG
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"Table 5" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the free neutron differential cross section.

Single Differential Cross SectionPhotoproductionElasticAstrophysics::High Energy Astrophysical PhenomenaGAMMA N --&gt; GAMMA NNuclear Theory1.125-1.255Nuclear ExperimentDSIG/DOMEGA
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"Table 4" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the triple differential cross section w.r.t. the scattered neutron.

PhotoproductionAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryTriple Differential Cross SectionExclusiveGAMMA DEUT --&gt; GAMMA P NNuclear ExperimentD3SIG/DE/DOMEGA/DOMEGA
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"Table 1" of "Test of low-energy theorems for p(gamma(pol.),pi0)p in the threshold region."

1995

Polarized photon beam.

Inclusive1.073-1.091PhotoproductionPhysics::OpticsPhysics::Accelerator PhysicsPBAR P --&gt; JET XJet ProductionAMP
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"Table 1" of "Angular and polarization dependence of Compton scattering from He-4 in the Delta resonance region"

1999

Axis error includes +- 0.0/0.0 contribution.

PhotoproductionAsymmetry MeasurementExclusiveGAMMA HE --&gt; HE GAMMAASYM
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"Table 1" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the free-proton differential cross section.

Single Differential Cross SectionPhotoproductionElasticNuclear TheoryPhysics::Accelerator PhysicsGAMMA P --&gt; GAMMA P1.13-1.327Nuclear ExperimentDSIG/DOMEGA
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