0000000000919648

AUTHOR

S. Wagner

showing 49 related works from this author

Measurement of Compton scattering at MAMI for the extraction of the electric and magnetic polarizabilities of the proton

2021

A precise measurement of the differential cross-sections $d\sigma/d\Omega$ and the linearly polarized photon beam asymmetry $\Sigma_3$ for Compton scattering on the proton below pion threshold has been performed with a tagged photon beam and almost $4\pi$ detector at the Mainz Microtron. The incident photons were produced by the recently upgraded Glasgow-Mainz photon tagging facility and impinged on a cryogenic liquid hydrogen target, with the scattered photons detected in the Crystal Ball/TAPS set-up. Using the highest statistics Compton scattering data ever measured on the proton along with two effective field theories (both covariant baryon and heavy-baryon) and one fixed-$t$ dispersion …

Nuclear Theory (nucl-th)Nuclear TheoryFOS: Physical sciencesHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experiment
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A new measurement of the neutron detection efficiency for the NaI Crystal Ball detector

2015

We report on a measurement of the neutron detection efficiency in NaI crystals in the Crystal Ball detector obtained from a study of single π0 photoproduction on deuterium using the tagged photon beam at the Mainz Microtron. The results were obtained up to a neutron energy of 400 MeV . They are compared to previous measurements made more than 15 years ago at the pion beam at the BNL AGS.

PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsDetectorNuclear TheoryFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Neutron temperatureHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Pion beamDeuteriumNeutron detectionPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentPhoton beamNuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationMicrotronNuclear ExperimentMathematical PhysicsCrystal Ball
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Measurement of the decay η′→π0π0η at MAMI

2018

An experimental study of the eta' -> pi(0)pi(0)eta -> 6 gamma decay has been conducted with the best up-to-date statistical accuracy, by measuring. 0 mesons produced in the gamma p -> eta'p reaction with the A2 tagged-photon facility at the Mainz Microtron, MAMI. The results obtained for the standard parametrization of the eta' -> pi(0)pi(0)eta matrix element are consistent with the most recent results for eta' -> pi pi eta decays, but have smaller uncertainties. The available statistics and experimental resolution allowed, for the first time, an observation of a structure below the pi(+)pi(-) thorn p-mass threshold, the magnitude and sign of which, checked within the framewo…

PhysicsHigh Energy Physics::ExperimentNuclear Experimentmatrix-element ; mass ; microtron ; 3-Pi(0) ; cusps ; ratio
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Reversibilität von Veränderungen der links- und rechtsventrikulären Geometrie und Hämodynamik bei pulmonaler Hypertonie. Echokardiographische Charakt…

1997

Durch pulmonale Thrombendarteriektomie kann bei Patienten mit chronischer embolisch bedingter pulmonaler Hypertonie eine akute rechtsventrikulare Nachlastsenkung erzielt werden. Der Einflus auf die rechts- und linksventrikulare Geometrie und Hamodynamik wurde prospektiv mit Hilfe der transthorakalen Echokardiographie an einem Kollektiv von 14 Patienten (8 Frauen, 6 Manner; Alter 55 ± 20 Jahre) vor und nach 18 ± 12 Tagen postoperativ untersucht. Nach operativer Desobliteration der Pulmonalarterien fand sich eine Abnahme des invasiv bestimmten totalen pulmonalen Gefaswiderstands von 986 ± 318 auf 323 ± 280 dyn x s/cm5; p < 0,05. Der echokardiographisch erfaste systolische pulmonalarterielle D…

Gynecologymedicine.medical_specialtyVentricule gauchebusiness.industrymedicineVentriculo derechoCardiology and Cardiovascular Medicinemedicine.diseasebusinessPulmonary embolismZeitschrift f�r Kardiologie
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Search for Cosmic Neutrino Point Sources with Four Year Data of the ANTARES Telescope

2012

In this paper, a time-integrated search for point sources of cosmic neutrinos is presented using the data collected from 2007 to 2010 by the ANTARES neutrino telescope. No statistically significant signal has been found and upper limits on the neutrino flux have been obtained. Assuming an E ¿2 n; spectrum, these flux limits are at 1-10 ¿10¿8 GeV cm¿2 s¿1 for declinations ranging from ¿90° to 40°. Limits for specific models of RX J1713.7¿3946 and Vela X, which include information on the source morphology and spectrum, are also given.

cosmic neutrinosUNIVERSEFluxVela01 natural scienceslaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawSIGNALSABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]MAXIMUM-LIKELIHOOD010303 astronomy & astrophysicsATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer database[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ASTRONOMYneutrinosastroparticle physicsFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaREMNANT RX J1713.7-3946Particle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescope[SDU.STU]Sciences of the Universe [physics]/Earth SciencesFOS: Physical sciencesddc:500.2Telescopeneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesPoint (geometry)ALGORITHMNeutrinosDETECTORCosmic raysUNDERWATER CHERENKOV NEUTRINO TELESCOPES010308 nuclear & particles physicsAstronomy and AstrophysicsHIGH-ENERGY PHOTONSSpace and Planetary ScienceFISICA APLICADAAstroparticle physics
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First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

2011

Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 0.1deg. The neutrino flux sensitivity is 7.5 ¿ 10 -8(E ¿/ GeV) -2 GeV -1 s -1 cm -2 for the part of the sky that is always visible (¿ < -48deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.

FLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesAngular resolutionALGORITHMNeutrinosDETECTOR010303 astronomy & astrophysicsCosmic raysmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorneutrinosASTRONOMYAstronomy and Astrophysicsastroparticle physics13. Climate actionSpace and Planetary ScienceSkyFISICA APLICADAddc:520Física nuclearHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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Helicity-dependent cross sections for the photoproduction of π0 pairs from nucleons

2020

The double-polarization observable $E$ and helicity-dependent cross sections $\sigma_{1/2}$, $\sigma_{3/2}$ have been measured for the photoproduction of $\pi^0$ pairs off quasi-free protons and neutrons at the Mainz MAMI accelerator with the Crystal Ball/TAPS setup. A circularly polarized photon beam was produced by bremsstrahlung from longitudinally polarized electrons and impinged on a longitudinally polarized deuterated butanol target. The reaction products were detected with an almost $4\pi$ covering calorimeter. The results reveal for the first time the helicity- and isospin-dependent structure of the $\gamma N\rightarrow N\pi^0\pi^0$ reaction. They are compared to predictions from re…

PhysicsProtonPhysicsspin polarization ; neutron ; photodisintegration ; Crystal Ball at MAMINuclear TheoryBremsstrahlungGeneral Physics and AstronomyElectron7. Clean energy01 natural sciencesResonance (particle physics)HelicityNuclear physics0103 physical sciencesNeutron010306 general physicsNucleonNuclear ExperimentNuclear ExperimentCrystal Ball
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The positioning system of the ANTARES Neutrino Telescope

2012

The ANTARES neutrino telescope, located 40km off the coast of Toulon in the Mediterranean Sea at a mooring depth of about 2475m, consists of twelve detection lines equipped typically with 25 storeys. Every storey carries three optical modules that detect Cherenkov light induced by charged secondary particles (typically muons) coming from neutrino interactions. As these lines are flexible structures fixed to the sea bed and held taut by a buoy, sea currents cause the lines to move and the storeys to rotate. The knowledge of the position of the optical modules with a precision better than 10cm is essential for a good reconstruction of particle tracks. In this paper the ANTARES positioning sys…

Positioning systemDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Detector modelling and simulations II (electric fieldsDetector alignment and calibration methods (lasers sources particle-beams)01 natural sciencesTiming detectorshardwareDetector alignment and calibration methods010303 astronomy & astrophysicsInstrumentationDETECTOR ALIGMENTMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSOUND[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Orientation (computer vision)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsTriangulation (computer vision)particle-beams)GeodesyDETECTOR CONTROL SYSTEMDetector modelling and simulations II (electric fields charge transport multiplication and induction pulse formation electron emission etc)Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)sources[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pulse formationarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2DETECTOR MODELLING AND SIMULATIONSDetector modelling and simulations IIalgorithmsPhysics::Geophysics0103 physical sciences14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationetc)multiplication and inductionBuoyDetector control systems010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsMooringcharge transport[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Detector alignment and calibration methods (laserselectron emissionFISICA APLICADAdetector modelling and simulations ii (electric fields; antares neutrino telescope; multiplication and induction; charge transport; pulse formation; electron emission; etc); hardware; architecture; timing detectors; detector control systems (detector and experiment monitoring and slow-control systems; algorithms; databases); sources; detector alignment; calibration.; acoustic positioning; detector alignment and calibration methods (lasers; particle-beams)
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Insight into the narrow structure in η-photoproduction on the neutron from helicity\ud dependent cross sections

2016

The double polarization observable E and the helicity dependent cross sections σ1/2 and σ3/2 were measured for η photoproduction from quasifree protons and neutrons. The circularly polarized tagged photon beam of the A2 experiment at the Mainz MAMI accelerator was used in combination with a longitudinally polarized deuterated butanol target. The almost 4π detector setup of the Crystal Ball and TAPS is ideally suited to detect the recoil nucleons and the decay photons from η→2γ and η→3π0. The results show that the narrow structure previously observed in η photoproduction from the neutron is only apparent in σ1/2 and hence, most likely related to a spin-1/2 amplitude. Nucleon resonances that …

Nuclear TheoryNuclear Experiment
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Deuteron photodisintegration by polarized photons in the region of the $d^*(2380)$

2019

We report the first large-acceptance measurement of the beam–spin asymmetry for deuteron photodisintegration (γ→d→pn) in the photon energy range 420&lt;Eγ&lt;620MeV. The measurement provides important new constraints on the mechanisms of photodisintegration above the Δ resonance and on the photocoupling of the recently discovered d⁎(2380) hexaquark.

Nuclear and High Energy PhysicsPhotonmedia_common.quotation_subjectNuclear TheoryHexaquarkFOS: Physical sciencesPhoton energy01 natural sciencesAsymmetryResonance (particle physics)Nuclear physics0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear Experimentmedia_commonPhysicsRange (particle radiation)010308 nuclear & particles physicsPhysicslcsh:QC1-999DeuteriumPhotodisintegrationlcsh:Physicsproton polarization ; cross-section ; disintegration ; asymmetry ; energies
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SEARCHES FOR POINT-LIKE AND EXTENDED NEUTRINO SOURCES CLOSE TO THE GALACTIC CENTER USING THE ANTARES NEUTRINO TELESCOPE

2014

A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been found. The most signal-like accumulation of events is located at equatorial coordinates R.A. = -46º.8 and decl. = -64º.9 and corresponds to a 2.2 sigma background fluctuation. In addition, upper limits on the flux normalization of an E-2 muon neutrino energy spectrum have been set for 50 pre-selected astrophysical objects. Finally, motivated by an accumulation of seven events relatively close to the Galactic Center in the recently reported neutrino sample…

Normalization (statistics)AstrofísicaParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicslaw.inventionHigh Energy Physics - ExperimentTelescopeHigh Energy Physics - Experiment (hep-ex)neutrinolaw[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Point (geometry)Muon neutrinoNeutrinsNeutrinosInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonCOSMIC cancer databaseGalaxy: center[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicFísicaneutrinosAstronomy and Astrophysicscenter [Galaxy]Galaxy centerNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionSpace and Planetary Scienceastroparticle physicsFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentNeutrinoAstroparticle physicsMATEMATICA APLICADAAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsastroparticle physics; Galaxy: center; neutrinos
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Search for Production of Invisible Final States in Single-Photon Decays of Υ(1S)

2010

We search for single-photon decays of the Upsilon(1S) resonance, Upsilon-&gt;gamma+invisible, where the invisible state is either a particle of definite mass, such as a light Higgs boson A0, or a pair of dark matter particles, chi chi-bar. Both A0 and chi are assumed to have zero spin. We tag Upsilon(1S) decays with a dipion transition Upsilon(2S)-&gt;pi+pi-Upsilon(1S) and look for events with a single energetic photon and significant missing energy. We find no evidence for such processes in the mass range m_A0&lt;=9.2 GeV and m_chi&lt;=4.5 GeV in the sample of 98e6 Upsilon(2S) decays collected with the BaBar detector and set stringent limits on new physics models that contain light dark ma…

Particle physicsPhotonAstrophysics::High Energy Astrophysical PhenomenaPhysics beyond the Standard ModelElectron–positron annihilationDark matterFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesResonance (particle physics)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PACS: 13.20.Gd 12.60.Jv 14.80.Da 95.35.+d0103 physical sciencessingle-photon decays of Upsilon(1S)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsLight dark matterPhysicsMissing energy010308 nuclear & particles physicsParticle physicsBABAR detectorHEPBaBarHiggs bosonHigh Energy Physics::ExperimentFísica de partículesExperimentsBaBar detector at SLAC
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Insight into the Narrow Structure in η Photoproduction on the Neutron from Helicity-Dependent Cross Sections

2016

The double polarization observable E and the helicity dependent cross sections σ1=2 and σ3=2 were measured for η photoproduction from quasifree protons and neutrons. The circularly polarized tagged photon beam of the A2 experiment at the Mainz MAMI accelerator was used in combination with a longitudinally polarized deuterated butanol target. The almost 4π detector setup of the Crystal Ball and TAPS is ideally suited to detect the recoil nucleons and the decay photons from η → 2γ and η → 3π0. The results show that the narrow structure previously observed in η photoproduction from the neutron is only apparent in σ1=2 and hence, most likely related to a spin-1=2 amplitude. Nucleon resonances t…

Nuclear TheoryNuclear Experimentη photoproduction ; neutron ; helicity-dependent cross sections
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Single π0 production off neutrons bound in deuteron with linearly polarized photons

2021

The quasifree γ→d→π0n(p) photon beam asymmetry, Σ, has been measured at photon energies, Eγ, from 390 to 610 MeV, corresponding to center of mass energy from 1.271 to 1.424 GeV, for the first time. The data were collected in the A2 hall of the MAMI electron beam facility with the Crystal Ball and TAPS calorimeters covering pion center-of-mass angles from 49∘ to 148∘. In this kinematic region, polarization observables are sensitive to contributions from the Δ(1232) and N(1440) resonances. The extracted values of Σ have been compared to predictions based on partial-wave analyses (PWAs) of the existing pion photoproduction database. Our comparison includes the SAID, MAID and Bonn–Gatchina anal…

deuteronpolarizationN(1440)partial waveNuclear Theoryphoton: energyDelta(1232)beam: asymmetryMainz Linackinematicsisospin: symmetrycalorimeterelectron: beampi0: photoproductionNuclear Experimentphoton: beamCrystal Ball
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Searches for clustering in the time integrated skymap of the ANTARES neutrino telescope

2014

Adrián-Martínez, S. et al.

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciences01 natural sciencesneutrino astronomy0103 physical sciencesNeutrinsNeutrinosCluster analysis010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AutocorrelationGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomyAstronomy and AstrophysicsGalaxyNeutrino astrophysicsneutrino astronomy; neutrino detectors[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Spatial clusteringNeutrinoMATEMATICA APLICADAAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsneutrino detectors
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ANTARES constrains a blazar origin of two IceCube PeV neutrino events

2015

Abstract Context. The source(s) of the neutrino excess reported by the IceCube Collaboration is unknown. The TANAMI Collaboration recently reported on the multiwavelength emission of six bright, variable blazars which are positionally coincident with two of the most energetic IceCube events. Objects like these are prime candidates to be the source of the highest-energy cosmic rays, and thus of associated neutrino emission. Aims. We present an analysis of neutrino emission from the six blazars using observations with the ANTARES neutrino telescope. Methods. The standard methods of the ANTARES candidate list search are applied to six years of data to search for an excess of muons and hence th…

Astrofísicaactive [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodFluxFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesSpectral line0103 physical sciencesNeutrinoGalaxies: active; Neutrinos; Quasars: generalNeutrinsNeutrinosBlazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonCosmologia010308 nuclear & particles physicsFísicaAstronomy and Astrophysicsgeneral [Quasars]Galaxies: activeAstronomy and AstrophysicNeutrino astrophysicsQuasars generalCosmologyneutrinos – galaxies: active – quasars: generalQuasars: generalSpace and Planetary ScienceGalaxies activeCol·lisions (Física nuclear)Galaxies: active; Neutrinos; Quasars: general; Astronomy and Astrophysics; Space and Planetary Science:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaMATEMATICA APLICADA[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astronomy & astrophysics
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Study of $\eta$ and $\eta'$ photoproduction at MAMI

2017

The reactions $\gamma p\to \eta p$ and $\gamma p\to \eta' p$ have been measured from their thresholds up to the center-of-mass energy $W=1.96$GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross sections were obtained with unprecedented accuracy, providing fine energy binning and full production-angle coverage. A strong cusp is observed in the total cross section and excitation functions for $\eta$ photoproduction at the energies in vicinity of the $\eta'$ threshold, $W=1896$MeV ($E_\gamma=1447$MeV). This behavior is explained in a revised $\eta$MAID isobar model by a significant branching of the $N(1895)1/2^-$ nucleon resonance to both, $\eta p$ and $\eta'…

High Energy Physics - PhenomenologyNuclear TheoryHigh Energy Physics::ExperimentNuclear ExperimentNuclear ExperimentHigh Energy Physics - Experiment
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SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS

2013

A multimessenger analysis optimized for a correlation of arrival directions of ultra-high energy cosmic rays (UHECRs) and neutrinos is presented and applied to 2190 neutrino candidate events detected in 2007-2008 by the ANTARES telescope and 69 UHECRs observed by the Pierre Auger Observatory between 2004 January 1 and 2009 December 31. No significant correlation is observed. Assuming an equal neutrino flux (E-2 energy spectrum) from all UHECR directions, a 90% CL upper limit on the neutrino flux of 5.0 x 10(-8) GeV cm(-2) s(-1) per source is derived.

AstrofísicaSELECTIONPOINT SOURCESTELESCOPE[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]Astrophysics::High Energy Astrophysical Phenomenaastroparticle physics – cosmic rays – neutrinos[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]FOS: Physical sciencesCosmic rayAstrophysicsPROPAGATIONACCELERATION7. Clean energy01 natural scienceslaw.inventionTelescopecosmic rayslaw0103 physical sciencesICECUBE DETECTORBURSTSNeutrinos010303 astronomy & astrophysicsCosmic raysPierre Auger ObservatoryAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NUCLEI010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrinosastroparticle physicAstronomy and AstrophysicsGALACTIC MAGNETIC-FIELDMassless particleENERGY COSMIC-RAYSSpace and Planetary Scienceastroparticle physicsFISICA APLICADAHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)Lepton
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First measurement of the polarization observable E and helicity-dependent cross sections in single π 0 photoproduction from quasi-free nucleons

2017

The double-polarization observable $E$ and the helicity-dependent cross sections $\sigma_{1/2}$ and $\sigma_{3/2}$ have been measured for the first time for single $\pi^{0}$ photoproduction from protons and neutrons bound in the deuteron at the electron accelerator facility MAMI in Mainz, Germany. The experiment used a circularly polarized photon beam and a longitudinally polarized deuterated butanol target. The reaction products, recoil nucleons and decay photons from the $\pi^0$ meson were detected with the Crystal Ball and TAPS electromagnetic calorimeters. Effects from nuclear Fermi motion were removed by a kinematic reconstruction of the $\pi^{0}N$ final state. A comparison to data mea…

Nuclear and High Energy PhysicsPhotonMesonProton3106Nuclear Theory01 natural sciences7. Clean energyNuclear physicsRecoil0103 physical sciencesNeutronddc:530010306 general physicsNuclear ExperimentNuclear ExperimentPhysics010308 nuclear & particles physicsPhysicslcsh:QC1-9993. Good healthNuclear cross sectionAtomic physicsNucleoni-circle-dot ; meson photoproduction ; eta-photoproduction ; baryon resonances ; deuteron ; neutrons ; protons ; asymmetry ; photon ; pairsCrystal Balllcsh:PhysicsPhysics Letters B
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Intraventrikuläre Obstruktionen bei der Dobutamin-Streßechokardiographie: Determinanten ihrer Entstehung und klinische Folgen (Dynamic intraventricul…

1997

Die Dobutamin-Stresechokardiographie (DSE) fuhrt zu einer starken Hyperkontraktilitat des Myokards bei Tachykardie und Vesodilatation. Diese Effekte konnen zu einer unphysiologischen Abnahme des endsystolischen Volumenindex (ESVI) mit Obstruktion des linksventrikularen Ausflustraktes (LVOT) fuhren. Bei 100 Patienten (Pat.), die sich einer DSE (5–40) μg/kg/min) unterzogen, wurde die kontinuierliche Dopplerregistrierung (DW-Doppler) vor Infusion und bei maximaler Herzfrequenz durchgefuhrt. Eine dynamische, spat-systolische, Flusakzeleration auf mehr als 2 Meter/Sekunde (m/s) unter maximaler Stimulation wurde als systolische Obstruktion des LVOT interpretiert. Manifestationsfaktoren systolisch…

medicine.medical_specialtyDobutamine stress echocardiographybusiness.industryVentricule gaucheInternal medicinemedicineCardiologyDobutamineCardiology and Cardiovascular MedicinebusinessSurgerymedicine.drugZeitschrift f�r Kardiologie
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Insight into the narrow structure in {\boldmath{$\eta$}}-photoproduction on the neutron from helicity dependent cross sections

2017

The double polarization observable $E$ and the helicity dependent cross sections $\sigma_{1/2}$ and $\sigma_{3/2}$ were measured for $\eta$ photoproduction from quasi-free protons and neutrons. The circularly polarized tagged photon beam of the A2 experiment at the Mainz MAMI accelerator was used in combination with a longitudinally polarized deuterated butanol target. The almost $4\pi$ detector setup of the Crystal Ball and TAPS is ideally suited to detect the recoil nucleons and the decay photons from $\eta\rightarrow 2\gamma$ and $\eta\rightarrow 3\pi^0$. The results show that the narrow structure previously observed in $\eta$ photoproduction from the neutron is only apparent in $\sigma_…

Nuclear ExperimentNuclear Experiment
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Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope

2012

The ANTARES telescope observes a full hemisphere of the sky all the time with a duty cycle close to 100%. This makes it well suited for an extensive observation of neutrinos produced in astrophysical transient sources. In the surrounding medium of blazars, i.e. active galactic nuclei with their jets pointing almost directly towards the observer, neutrinos may be produced together with gamma-rays by hadronic interactions, so a strong correlation between neutrinos and gamma-rays emissions is expected. The time variability information of the studied source can be obtained by the gamma-ray light curves measured by the LAT instrument on-board the Fermi satellite. If the expected neutrino flux ob…

ASTROPHYSICSAstrofísicaAstrophysicsNeutrino Astronomy01 natural sciences7. Clean energyLARGE-AREA TELESCOPElaw.inventionlawWATERInstrumentation010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Time-dependent searchCATALOGLIGHTNeutrino astronomyFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEINuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleus[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Point sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsfermi lat transient sources; neutrino astronomy; time-dependent search; antares; blazarsTelescopeMUONS0103 physical sciencesANTARES; Neutrino Astronomy; Fermi LAT transient sourcesBlazarANTARES010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsFermi LAT transient sourcesLight curveNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODEL13. Climate actionFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Neutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]BlazarsFermi Gamma-ray Space Telescope
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First results on dark matter annihilation in the Sun using the ANTARES neutrino telescope

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

PHOTINOAstrophysicsMASSIVE PARTICLES01 natural sciencesLIMITSDirect searchCANDIDATESPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilationdark matter detectors[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsAstrophysics::Instrumentation and Methods for AstrophysicsCAPTURELIGHTparticle physics - cosmology connectionWeakly interacting massive particlesneutrino experiments; particle physics - cosmology connection; dark matter detectors; supersymmetry and cosmologyFísica nuclearNeutrinosupersymmetry andAstrophysics - High Energy Astrophysical PhenomenaCosmology connectionsupersymmetry and cosmologyFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Supersymmetry and cosmologydark matter detectorAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeDark matterFOS: Physical sciencesddc:500.2neutrino experimentsSEARCH0103 physical sciencesDETECTORS010306 general physicsSelection (genetic algorithm)Dark matter detectors010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsNeutrino experimentsFISICA APLICADAParticle physics - cosmology connectionneutrino experimentHigh Energy Physics::ExperimentcosmologySYSTEM
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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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Dobutamine stress Doppler echocardiography: reproducibility and physiologic left ventricular filling patterns

1997

Qualitatively, dobutamine stress echocardiography has become an established procedure. Quantitative results are in great demand but this is still difficult due to limited endo- and epicardial border definition. Transmitral Doppler variables are strictly quantitative and less subjective. Furthermore, ischemic alterations precede systolic ones (ischemic cascade). There are preliminary reports of the utility of dobutamine stress Doppler echocardiography, but proof of reproducibility and left ventricular filling patterns are still lacking. Fourteen healthy volunteers (10 men, 4 women, median age 25.9 years, range 21-32 years) were investigated according to the usual dobutamine stress echocardio…

Malemedicine.medical_specialtyCardiotonic AgentsMyocardial IschemiaIschemiaHemodynamicsCoronary DiseaseDoppler echocardiographySensitivity and SpecificityVentricular Function Leftsymbols.namesakeReference ValuesDobutamineInternal medicinemedicineHumansObserver VariationReproducibilitymedicine.diagnostic_testVascular diseasebusiness.industryHemodynamicsReproducibility of ResultsIschemic cascademedicine.diseaseEchocardiography DopplerExercise TestsymbolsCardiologyFemaleDobutamineCardiology and Cardiovascular MedicinebusinessDoppler effectmedicine.drugInternational Journal of Cardiology
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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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Measurement of the beam-helicity asymmetry in photoproduction of π0η pairs on carbon, aluminum, and lead

2020

The beam-helicity asymmetry was measured, for the first time, in photoproduction of $\pi^{0}\eta$ pairs on carbon, aluminum, and lead, with the A2 experimental setup at MAMI. The results are compared to an earlier measurement on a free proton and to the corresponding theoretical calculations. The Mainz model is used to predict the beam-helicity asymmetry for the nuclear targets. The present results indicate that the photoproduction mechanism for $\pi^{0}\eta$ pairs on nuclei is similar to photoproduction on a free nucleon. This process is dominated by the $D_{33}$ partial wave with the $\eta\Delta(1232)$ intermediate state.

Nuclear and High Energy PhysicsProtonmedia_common.quotation_subjectNuclear Theorychemistry.chemical_element7. Clean energy01 natural sciencesAsymmetryNuclear physicsAluminium0103 physical sciencesIntermediate stateNuclear Experiment010306 general physicsNuclear ExperimentQCmedia_commonPhysics010308 nuclear & particles physicsHelicitylcsh:QC1-9993. Good healthchemistryHigh Energy Physics::ExperimentNucleonCarbonlcsh:PhysicsBeam (structure)Physics Letters B
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Normalwerte für die Dobutamin-Streßechokardiographie*

2008

UNLABELLED Dobutamine stress echocardiography having established itself as a sensitive method for diagnosing coronary heart disease, even in the absence of normative values, the physiological haemodynamics as well as the physiological values for global and regional left ventricular myocardial function were measured. TEST PERSONS AND METHODS 14 healthy subjects (ten men, four women; median age 25 [range 21-32] years) underwent dobutamine stress echocardiography according to an internationally practised dosage steps protocol (5-40 micrograms/kg/min with additional 0.5 mg atropine at 40 micrograms). RESULTS Maximal infusion rate achieved a serum dobutamine level of 1.67 micrograms/ml with mini…

medicine.medical_specialtyEjection fractionbusiness.industryDiastoleHemodynamicsGeneral MedicineContractilityAtropineBlood pressureInternal medicineHeart ratemedicineCardiologyDobutaminebusinessmedicine.drugDMW - Deutsche Medizinische Wochenschrift
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Study of eta and eta' Photoproduction at MAMI

2017

The reactions γp→ηp and γp→η′p are measured from their thresholds up to the center-of-mass energy W=1.96 GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross sections are obtained with unprecedented statistical accuracy, providing fine energy binning and full production-angle coverage. A strong cusp is observed in the total cross section for η photoproduction at the energies in the vicinity of the η′ threshold, W=1896 MeV (Eγ=1447 MeV). Within the framework of a revised ηMAID isobar model, the cusp, in connection with a steep rise of the η′ total cross section from its threshold, can only be explained by a strong coupling of the poorly known N(1895)1/2− sta…

spectrometer ; photons ; proton ; taps
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Study of η and η' Photoproduction at MAMI

2017

The reactions γp → ηp and γp → η0\ud p are measured from their thresholds up to the center-of-mass\ud energy W ¼ 1.96 GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross\ud sections are obtained with unprecedented statistical accuracy, providing fine energy binning and full\ud production-angle coverage. A strong cusp is observed in the total cross section for η photoproduction at the\ud energies in the vicinity of the η0 threshold, W ¼ 1896 MeV (Eγ ¼ 1447 MeV). Within the framework of a\ud revised ηMAID isobar model, the cusp, in connection with a steep rise of the η0 total cross section from its\ud threshold, can only be explained by a strong coupling of …

ddc:550
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Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

2014

Adrián-Martínez, S. et al.

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsRayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesantaresAstrophysicsddc:500.2Neutrino fluxesGamma ray burstsPartícules (Física nuclear)law.inventionTelescopeneutrinoRaigs gammalaw14. Life underwaterNeutrinsNeutrinosEngineering (miscellaneous)Cherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayfermi bubbles; antares; neutrinoDetectorCharged particleNeutrino astrophysicsFermi bubbleneutrino telecope13. Climate actionFermi bubblesCol·lisions (Física nuclear):Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAntares neutrino telescopeFermi Gamma-ray Space Telescope
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A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

AstrofísicaEXPLOSIONSHigh energyPhotonPOINT SOURCESSUPERCONDUCTING COSMIC STRINGSGravitational waves / experimentsGravitational waves/experimentsAstrophysics01 natural scienceshigh energy neutrinosgravitational wavesgravitational waves / experiment010303 astronomy & astrophysicsQCmedia_commonLine (formation)QBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSdark matter detectorsGravitational waves / experiments; Neutrino astronomy; Astronomy and Astrophysicshigh energy neutrinos[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsgravitational waves; gravitational waves / experiments; neutrino astronomy; high energy neutrinos; high energy neutrinosgravitational wavesgravitational wavesparticle physics - cosmology connectionNeutrino astronomyCOSMIC STRINGSRELATIVISTIC JETSNeutrinoAstrophysics - High Energy Astrophysical Phenomenasupersymmetry and cosmology[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]gravitational waves / experiments; neutrino astronomyTELESCOPEmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaSCIENCE RUNFOS: Physical sciencesddc:500.2GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; SUPERCONDUCTING COSMIC STRINGS; MAGNETAR GIANT FLARES; SCIENCE RUN; RELATIVISTIC JETS; POINT SOURCES; BLACK-HOLES; LOCAL-RATE; TELESCOPEGravitational wavesGeneral Relativity and Quantum CosmologyCORE-COLLAPSE SUPERNOVAESettore FIS/05 - Astronomia e AstrofisicaCoincidentneutrino experiments0103 physical sciences010306 general physicsMAGNETAR GIANT FLARESBLACK-HOLESHigh Energy Astrophysical PhenomenaGravitational waveAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsDRIVENUniverseLIGOGIANT FLARESLOCAL-RATEFISICA APLICADALUMINOSITYRADIATIONHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Helicity-dependent cross sections and double-polarization observable E in eta photoproduction from quasi-free protons and neutrons

2017

Precise helicity-dependent cross sections and the double-polarization observable $E$ were measured for $\eta$ photoproduction from quasi-free protons and neutrons bound in the deuteron. The $\eta\rightarrow 2\gamma$ and $\eta\rightarrow 3\pi^0\rightarrow 6\gamma$ decay modes were used to optimize the statistical quality of the data and to estimate systematic uncertainties. The measurement used the A2 detector setup at the tagged photon beam of the electron accelerator MAMI in Mainz. A longitudinally polarized deuterated butanol target was used in combination with a circularly polarized photon beam from bremsstrahlung of a longitudinally polarized electron beam. The reaction products were de…

FOS: Physical sciencesNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experiment
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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Study of η and η′ Photoproduction at MAMI

2017

The reactions γp→ηp and γp→η′p are measured from their thresholds up to the center-of-mass energy W=1.96  GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross sections are obtained with unprecedented statistical accuracy, providing fine energy binning and full production-angle coverage. A strong cusp is observed in the total cross section for η photoproduction at the energies in the vicinity of the η′ threshold, W=1896  MeV (Eγ=1447  MeV). Within the framework of a revised ηMAID isobar model, the cusp, in connection with a steep rise of the η′ total cross section from its threshold, can only be explained by a strong coupling of the poorly known N(1895)1/2− …

Cusp (singularity)PhysicsParticle physicsPhotonProton010308 nuclear & particles physicsGeneral Physics and Astronomy01 natural sciencesNuclear physicsCross section (physics)Excited state0103 physical sciencesIsobar010306 general physicsMicrotronCrystal BallPhysical Review Letters
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Measurement of the π0→e+e−γ Dalitz decay at the Mainz Microtron

2017

The Dalitz decay π0→e+e−γ has been measured in the γp→π0p reaction with the A2 tagged-photon facility at the Mainz Microtron, MAMI. The value obtained for the slope parameter of the π0 electromagnetic transition form factor, aπ=0.030±0.010tot, is in agreement with existing measurements of this decay and with recent theoretical calculations. The uncertainty obtained in the value of aπ is lower than in previous results based on the π0→e+e−γ decay.

Nuclear physicsPhysicsParticle physicsMeson010308 nuclear & particles physics0103 physical sciencesForm factor (quantum field theory)010306 general physics01 natural sciencesMicrotronDark photonPhysical Review C
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First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope

2013

A search for neutrino-induced muons in correlation with a selection of 40 gamma-ray bursts that occurred in 2007 has been performed with the ANTARES neutrino telescope. During that period, the detector consisted of 5 detection lines. The ANTARES neutrino telescope is sensitive to TeV-PeV neutrinos that are predicted from gamma-ray bursts. No events were found in correlation with the prompt photon emission of the gamma-ray bursts and upper limits have been placed on the flux and fluence of neutrinos for different models.

AstrofísicaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]neutrino experiments; neutrino astronomy; gamma ray bursts theoryPOINT SOURCESPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaREDSHIFTFluxFOS: Physical sciencesAstrophysics01 natural sciencesICECUBEneutrino astronomyneutrino experiments0103 physical sciencesgamma ray bursts theory010303 astronomy & astrophysicsNeutrino experimentsATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonGamma ray bursts theory010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomygamma ray bursts theory; neutrino astronomy; neutrino experimentsAstronomy and Astrophysicsgamma ray burstsCATALOGRedshiftNeutrino detectorNeutrino astronomyFISICA APLICADAneutrino experimentHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstSYSTEM
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Insight into the Narrow Structure in eta Photoproduction on the Neutron from Helicity-Dependent Cross Sections

2016

The double polarization observable E and the helicity dependent cross sections σ1/2 and σ3/2 were measured for η photoproduction from quasifree protons and neutrons. The circularly polarized tagged photon beam of the A2 experiment at the Mainz MAMI accelerator was used in combination with a longitudinally polarized deuterated butanol target. The almost 4π detector setup of the Crystal Ball and TAPS is ideally suited to detect the recoil nucleons and the decay photons from η→2γ and η→3π0. The results show that the narrow structure previously observed in η photoproduction from the neutron is only apparent in σ1/2 and hence, most likely related to a spin-1/2 amplitude. Nucleon resonances that …

Nuclear TheoryNuclear Experiment
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Measurement of the group velocity of light in sea water at the ANTARES site

2012

The group velocity of light has been measured at eight different wavelengths between 385 nm and 532 nm in the Mediterranean Sea at a depth of about 2.2 km with the ANTARES optical beacon systems. A parametrisation of the dependence of the refractive index on wavelength based on the salinity, pressure and temperature of the sea water at the ANTARES site is in good agreement with these measurements.

Light velocityRefractive indexAtmospheric sciencesNeutrino telescope01 natural scienceslaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Mediterranean sealawOptical beacon systemPhysicsOptical beaconPressure and temperature[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Wavelengthoptical beacon system; neutrino telescope; antares; refractive index; velocity of lightVelocity of lightGroup velocityFísica nuclear[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]ParametrisationFOS: Physical sciencesddc:500.2010309 opticsOpticsLight--Speed--Measurement0103 physical sciencesOptical systemsSeawater14. Life underwater:Física::Acústica [Àrees temàtiques de la UPC]ANTARES010308 nuclear & particles physicsbusiness.industryAstronomy and AstrophysicsLaser[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]SalinityLlum -- VelocitatFISICA APLICADAVelocity of lightMediterranean seaSeawaterNeutrino telescopesbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Refractive indexSYSTEM
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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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Measurement of θ13 in Double Chooz using neutron captures on hydrogen with novel background rejection techniques

2016

The Double Chooz collaboration presents a measurement of the neutrino mixing angle θ[subscript 13] using reactor [bar over ν[subscript e]] observed via the inverse beta decay reaction in which the neutron is captured on hydrogen. This measurement is based on 462.72 live days data, approximately twice as much data as in the previous such analysis, collected with a detector positioned at an average distance of 1050 m from two reactor cores. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties. Accidental coincidences, the dominant background in this analysis, are suppressed by more than an order of magnitude with respec…

data analysis methodNuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsNeutrino Detectors and TelescopeGadoliniumnuclear reactor [antineutrino/e]energy spectrumchemistry.chemical_elementFluxmixing angle: measured [neutrino]CHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - Experimentflux [antineutrino]Flavor physicscapture [n]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interactionddc:530Neutron010306 general physicsPhysicsNeutrino Detectors and Telescopesbackground010308 nuclear & particles physicsoscillation [neutrino]suppressionDouble ChoozNeutron captureOscillationchemistryhydrogenInverse beta decayFlavor physicspectralHigh Energy Physics::ExperimentgadoliniumNeutrinoOrder of magnitudeexperimental results
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Pertussis vaccines--1993.

1993

AdolescentWhooping CoughJapanmedicinemedia_common.cataloged_instanceHumansEuropean UnionEuropean unionChildWhooping coughDiphtheria-Tetanus-Pertussis Vaccinemedia_commonPertussis Vaccinebusiness.industryInfant NewbornInfantDiphtheria-Tetanus-Pertussis Vaccinemedicine.diseaseInfant newbornVaccinationEuropeChild PreschoolPediatrics Perinatology and Child HealthImmunologyPertussis vaccinebusinessTos ferinamedicine.drugForecastingEuropean journal of pediatrics
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Quantitative assessment of aortic stenosis by three-dimensional echocardiography

1997

The purpose of this study was to assess the feasibility of three-dimensional echocardiography in aortic stenosis. Planimetric determination of valve area and dynamic volume-rendered display were performed. Three-dimensional echocardiography permits display of any desired plane of the cardiac structure. Thus in the case of aortic stenosis, the plane used for planimetric evaluation can be positioned exactly through the valve orifice. Dynamic volume-rendered display may provide a spatial demonstration of the stenotic valve. In 48 patients aortic valve area was measured by planimetry. The three-dimensional data set was acquired by a workstation in the course of a multiplane transesophageal exam…

AdultMaleCardiac Catheterizationmedicine.medical_specialtymedicine.medical_treatmentEchocardiography Three-DimensionalQuantitative assessmentHumansMedicineRadiology Nuclear Medicine and imagingCardiac structureAgedCardiac catheterizationAged 80 and overObserver Variationbusiness.industryThree dimensional echocardiographyAortic Valve StenosisMiddle Agedmedicine.diseaseData setStenosisAortic valve areaAortic valve stenosisFemaleRadiologyCardiology and Cardiovascular MedicinebusinessEchocardiography TransesophagealJournal of the American Society of Echocardiography
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Constraining the neutrino emission of gravitationally lensed Flat-Spectrum Radio Quasars with ANTARES data

2014

This paper proposes to exploit gravitational lensing effects to improve the sensitivity of neutrino telescopes to the intrinsic neutrino emission of distant blazar populations. This strategy is illustrated with a search for cosmic neutrinos in the direction of four distant and gravitationally lensed Flat-Spectrum Radio Quasars. The magnification factor is estimated for each system assuming a singular isothermal profile for the lens. Based on data collected from 2007 to 2012 by the ANTARES neutrino telescope, the strongest constraint is obtained from the lensed quasar B0218+357, providing a limit on the total neutrino luminosity of this source of 1.08×10^46 erg s-1. This limit is about one o…

Point sourceAstronomyAstrophysics::High Energy Astrophysical Phenomenagravitational lensingFOS: Physical sciencesgravitational lensing; neutrino astronomyAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLuminosityneutrino astronomyNeutrino0103 physical sciencesSensitivity (control systems)Blazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)gravitational lensing; neutrino astronomy; Astronomy and AstrophysicsCOSMIC cancer database010308 nuclear & particles physicshigh energy astrophysical neutrinosAstrophysics::Instrumentation and Methods for AstrophysicsFísicaQuasarAstronomy and AstrophysicsGravitational lensFISICA APLICADANeutrinoMATEMATICA APLICADAAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Regional climate model simulations for Europe at 6 k and 0.2 k yr BP: sensitivity to changes in anthropogenic deforestation

2013

Abstract. This study aims to evaluate the direct effects of anthropogenic deforestation on simulated climate at two contrasting periods in the Holocene, ~6 k BP and ~0.2 k BP in Europe. We apply RCA3, a regional climate model with 50 km spatial resolution, for both time periods, considering three alternative descriptions of the past vegetation: (i) potential natural vegetation (V) simulated by the dynamic vegetation model LPJ-GUESS, (ii) potential vegetation with anthropogenic land cover (deforestation) as simulated by the HYDE model (V + H), and (iii) potential vegetation with anthropogenic land cover as simulated by the KK model (V + K). The KK model estimates are closer to a set of polle…

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Measurement of the atmospheric ?µ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

2013

Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric energy spectrum in the energy range 0.1-200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is similar to 25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index gamma (meas)=3.58 +/- 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

Astrofísica:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]Physics and Astronomy (miscellaneous)Raigs còsmicsFluxOceanografia7. Clean energy01 natural scienceslaw.inventionlawUnderwater acousticsEnergy range 0.1 to 200 TeVNeutrino TelescopePhysicsRange (particle radiation)Spectral index[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]atmospheric neutrinoNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsLorentz Invariance ViolationFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]OscillationsSoroll -- Aspectes ambientalsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayddc:500.2MACRONuclear physicsTelescopeMUONSSEARCH0103 physical sciencesNeutrinsNeutrinos010306 general physicsEngineering (miscellaneous)Cosmic raysDETECTOR:Física::Acústica [Àrees temàtiques de la UPC]ANTARESAtmospheric neutrino antineutrino010308 nuclear & particles physicsAntares telescopeHigh Energy Physics::Phenomenology[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionFISICA APLICADAlorentz invariance violation; neutrino oscillation; muonsHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)European Physical Journal C
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Signatures of the d*(2380) Hexaquark in d(γ,pn→)

2020

We report a measurement of the spin polarization of the recoiling neutron in deuterium photodisintegration, utilizing a new large acceptance polarimeter within the Crystal Ball at MAMI. The measured photon energy range of 300-700 MeV provides the first measurement of recoil neutron polarization at photon energies where the quark substructure of the deuteron plays a role, thereby providing important new constraints on photodisintegration mechanisms. A very high neutron polarization in a narrow structure centered around E_{γ}∼570 MeV is observed, which is inconsistent with current theoretical predictions employing nucleon resonance degrees of freedom. A Legendre polynomial decomposition sugge…

PhysicsPhotonSpin polarizationNuclear TheoryGeneral Physics and AstronomyPhoton energy01 natural sciencesNuclear physicsRecoilPhotodisintegration0103 physical sciencesNeutronNuclear Experiment010306 general physicsNucleonCrystal BallPhysical Review Letters
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Measurement of the decay η′→π0π0η at MAMI

2018

An experimental study of the η′→π0π0η→6γ decay has been conducted with the best up-to-date statistical accuracy, by measuring η′ mesons produced in the γp→η′p reaction with the A2 tagged-photon facility at the Mainz Microtron, MAMI. The results obtained for the standard parametrization of the η′→π0π0η matrix element are consistent with the most recent results for η′→ππη decays, but have smaller uncertainties. The available statistics and experimental resolution allowed, for the first time, an observation of a structure below the π+π− mass threshold, the magnitude and sign of which, checked within the framework of the nonrelativistic effective-field theory, demonstrated good agreement with t…

Physical Review
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