Search results for "Gamma-ray"

showing 10 items of 374 documents

Nonlocalities and Fermi motion corrections in K- atoms

2002

We evaluate the p-wave $K^-N$ amplitudes from the chiral Lagrangians and from there construct the p-wave part of the $K^-$ nucleus optical potential plus a small s-wave part induced from the elementary p-wave amplitude and the nuclear Fermi motion. Simultaneously, the momentum and energy dependence of the s-wave optical potential, previously developed, are taken into account and shown to generate a small p-wave correction to the optical potential. All the corrections considered are small compared to the leading s-wave potential, and lead to changes in the shifts and widths which are smaller than the experimental errors. A thorough study of the threshold region and low densities is conducted…

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsAmplitudeNuclear TheoryQuantum electrodynamicsFOS: Physical sciencesMotion (geometry)FísicaEnergy–momentum relationOptical potentialFermi Gamma-ray Space Telescope
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Photoproduction of the hypertriton

1997

In the framework of the impulse approximation we study the photoproduction of the hypertriton $^3_{\Lambda}$H by using realistic $^3$He wave functions obtained as solutions of Faddeev equations with the Reid soft-core potential for different $^3_{\Lambda}$H wave functions. We obtain relatively small cross sections of the order of 1 nb. We also find that the influence of Fermi motion is important, while the effect of different off-shell assumptions on the cross section is not too significant.

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsFaddeev equationsParticle physicsNuclear TheoryNuclear TheoryFOS: Physical sciencesImpulse (physics)Wave functionLambdaHypertritonFermi Gamma-ray Space TelescopeNuclear Physics A
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Shell-model calculation of isospin-symmetry breaking correction to superallowed Fermi beta-decay

2016

We investigate the radial-overlap part of the isospin-symmetry breaking correction to superallowed $0^+\to 0^+$-decay using the shell-model approach similar to that of Refs. [1, 2]. The 8 sd-shell emitters with masses between $A=22$ and $A=38$ have been re-examined. The Fermi matrix element is evaluated with realistic spherical single-particle wave functions, obtained from spherical Woods-Saxon (WS) or Hartree-Fock (HF) potentials, fine-tuned to reproduce the experimental data on charge radii and separation energies for nuclei of interest. The elaborated adjustment procedure removes any sensitivity of the correction to a specific parametrisation of the WS potential or to various versions of…

Nuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]SHELL modelNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences23.40.-sNuclear physicsNuclear Theory (nucl-th)21.60.Cs0103 physical sciences21.10.PcSensitivity (control systems)Symmetry breakingWave function010303 astronomy & astrophysics[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]Physicsta114010308 nuclear & particles physicsCharge (physics)Beta decay21.10.JxIsospinQuantum electrodynamics23.40.Bwbeta decayisospin-symmetry breakingFermi Gamma-ray Space Telescope
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Collectivity in ${}^{\mathrm{196,198}}$Pb isotopes probed in Coulomb-excitation experiments at REX-ISOLDE

2017

The neutron-deficient ${}^{\mathrm{196,198}}$Pb isotopes have been studied in Coulomb-excitation experiments employing the Miniball γ-ray spectrometer and radioactive ion beams from the REX-ISOLDE post-accelerator at CERN. The reduced transition probabilities of the first excited 2+ states in 196Pb and 198Pb nuclei have been measured for the first time. Values of $B(E2)={18.2}_{-4.1}^{+4.8}$ W.u. and $B(E2)={13.1}_{-3.5}^{+4.9}$ W.u., were obtained, respectively. The experiment sheds light on the development of collectivity when moving from the regime governed by the generalised seniority scheme to a region, where intruding structures, associated with different deformed shapes, start to com…

Nuclear and High Energy Physics3106Coulomb excitationREX-ISOLDESHELLHadronElementary particleCoulomb excitation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciences01 natural sciencesNuclear physicsSHAPE COEXISTENCE0103 physical sciencesSCATTERINGradioactive ion beamsACCELERATED RADIOACTIVE BEAMS010306 general physicsPhysicsPb isotopesNUCLEI010308 nuclear & particles physicsBaryongamma-ray spectroscopyEXCITED-STATESCoulomb-excitation experimentExcited stateAtomic physicsGround stateNucleongamma transitions and level energiesEnergy (signal processing)
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Search for dark matter from the Galactic halo with the IceCube neutrino telescope

2011

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihilation cross section of ⟨σAv⟩≃10-22 cm3 s-1 for weakly interacting massive particle masses above 1 TeV, assuming a monochromatic neutrino line spectrum.

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesIceCubeGalactic halo0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsGamma-Ray EmissionHot dark matterAstronomyCosmic-Rays004Dark matter haloParticlesNeutrino detectorAnisotropyHigh Energy Physics::ExperimentHaloDwarf Spheroidal GalaxiesNeutrinoNeutrino astronomyinfo:eu-repo/classification/ddc/004
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Interaction position resolution simulations and in-beam measurements of the AGATA HPGe detectors

2011

WOS: 000290082600015

Nuclear and High Energy PhysicsFusion-evaporation ReactionsPhysics::Instrumentation and Detectorsg-ray trackingAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodEvaporationRay tracking[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesParticle detectorNuclear physicsAGATA Fusion-evaporation reactions HPGe detectors Monte Carlo Simulation Ray tracking; Computer simulation Evaporation Monte Carlo methods Phase transitions; DetectorsHPGe Detectors0103 physical sciencesNuclear Experiment010306 general physicsInstrumentationGamma-ray TrackingPhysics010308 nuclear & particles physics4. EducationResolution (electron density)DetectorMonte Carlo SimulationMonte Carlo methodsDetectorsComputer simulationSemiconductor detectorPhase transitionsMonte Carlo SimulationsMeasuring instrumentHigh Energy Physics::ExperimentAGATAAGATABeam (structure)
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Search for gamma ray bursts with the ARGO-YBJ detector in scaler mode

2009

We report on the search for Gamma Ray Bursts (GRBs) in the energy range 1-100 GeV in coincidence with the prompt emission detected by satellites using the Astrophysical Radiation with Ground-based Observatory at YangBaJing (ARGO-YBJ) air shower detector. Thanks to its mountain location (Yangbajing, Tibet, P.R. China, 4300 m a.s.l.), active surface (about 6700 m**2 of Resistive Plate Chambers), and large field of view (about 2 sr, limited only by the atmospheric absorption), the ARGO-YBJ air shower detector is particularly suitable for the detection of unpredictable and short duration events such as GRBs. The search is carried out using the "single particle technique", i.e. counting all the …

Nuclear and High Energy PhysicsGamma ray burstAstrophysics::High Energy Astrophysical PhenomenaAir shower arrayAstrophysicsArgo-YbjSettore FIS/05 - Astronomia e AstrofisicaObservatoryGamma Rays ObservationsInstrumentationZenithArgoPhysicsRange (particle radiation)Apparati di sciameDetectorSettore FIS/01 - Fisica SperimentaleGamma rayGamma ray bursts Air shower arraysMode (statistics)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsRedshiftAir showerSpace and Planetary ScienceGamma Ray Bursts Gamma Ray EmissionAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burst
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Ultrafast Dynamics of Magnetic Domain Structures Probed by Coherent Free-Electron Laser Light

2013

Synchrotron radiation news 26(6), 27 - 32 (2013). doi:10.1080/08940886.2013.850384

Nuclear and High Energy PhysicsMagnetic domainMagnetismAstrophysics::High Energy Astrophysical Phenomena02 engineering and technology53001 natural scienceslaw.inventionOpticslaw0103 physical sciencesddc:530010306 general physicsComputingMilieux_MISCELLANEOUSPhysicsMagnetic circular dichroismbusiness.industryScatteringFree-electron laser021001 nanoscience & nanotechnologyLaserAtomic and Molecular Physics and Optics[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Physics::Accelerator PhysicsAtomic physics0210 nano-technologybusinessUltrashort pulseFermi Gamma-ray Space TelescopeSynchrotron Radiation News
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Recent advances in the development of high-resolution 3D cadmium-zinc-telluride drift strip detectors.

2020

In the last two decades, great efforts have been made in the development of 3D cadmium–zinc–telluride (CZT) detectors operating at room temperature for gamma-ray spectroscopic imaging. This work presents the spectroscopic performance of new high-resolution CZT drift strip detectors, recently developed at IMEM-CNR of Parma (Italy) in collaboration with due2lab (Italy). The detectors (19.4 mm × 19.4 mm × 6 mm) are organized into collecting anode strips (pitch of 1.6 mm) and drift strips (pitch of 0.4 mm) which are negatively biased to optimize electron charge collection. The cathode is divided into strips orthogonal to the anode strips with a pitch of 2 mm. Dedicated pulse processing analysis…

Nuclear and High Energy PhysicsMaterials sciencePhysics::Instrumentation and Detectors030303 biophysics3D CdZnTe detectorsSTRIPS01 natural sciencesElectric chargelaw.invention03 medical and health scienceschemistry.chemical_compounddrift strip detectorslaw0103 physical sciencesInstrumentation0303 health sciencesRadiation010308 nuclear & particles physicsbusiness.industryDetectorElectrostatic inductionSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)CathodeCadmium zinc tellurideAnodeFull width at half maximumX-ray and gamma-ray detectorschemistryX-ray and gamma-ray detectors; 3D CdZnTe detectors; drift strip detectors; spectroscopic X-ray and gamma-ray imagingOptoelectronicsbusinessspectroscopic X-ray and gamma-ray imagingJournal of synchrotron radiation
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Shell evolution of $N=40$ isotones towards $^{60}$Ca: First spectroscopy of $^{62}$Ti

2020

7 pags., 4 figs., 1 tab.

Nuclear and High Energy PhysicsNuclear TheoryNuclear TheoryAb initioFOS: Physical sciencesShell evolution[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesShell evolution ; Radioactive beams ; Gamma-ray spectroscopyNuclear Theory (nucl-th)Gamma-ray spectroscopy; Radioactive beams; Shell evolution0103 physical sciencesddc:530Gamma-ray spectroscopyNuclear Experiment (nucl-ex)010306 general physicsSpectroscopyNuclear ExperimentNuclear ExperimentPhysics010308 nuclear & particles physicsIsland of inversionIsotonePhysicsStarke Wechselwirkung und exotische Kerne – Abteilung BlaumFísicalcsh:QC1-999Excited stateQuadrupoleAtomic physicsNucleonGround statelcsh:PhysicsRadioactive beams
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