Search results for "Gamma-Ray"

showing 10 items of 374 documents

Gamma ray sources observation with the ARGO-YBJ detector

2011

In this paper we report on the observations of TeV gamma ray sources performed by the air shower de- tector ARGO-YBJ. The objects studied in this work are the blazar Markarian 421 and the extended galactic source MGROJ1908+06, monitored during 2 years of operation. Mrk421 has been detected by ARGO-YBJ with a statisti- cal significance of 11 standard deviations. The observed TeV emission was highly variable, showing large enhance- ments of the flux during active periods. The study of the spectral behaviour during flares revealed a positive correla- tion of the hardness with the flux, as already reported in the past by the Whipple telescope, suggesting that this is a long term property of the…

PhysicsNuclear and High Energy PhysicsGamma AstronomyPhysics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaDetectorGamma rayFluxAstronomyExtensive Air ShowerAstronomy and AstrophysicsAstrophysicsGamma-ray astronomyArray DetectorGamma-RayArgo-YbjGamma Astronomy Array DetectorCrab NebulaAir showerPulsarMilagroBlazarInstrumentationArgoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Microscopic quasiparticle-phonon description of odd-mass127−133Xeisotopes and their β decay

1998

Quasiparticle-phonon equations of motion are solved starting from a microscopic realistic many-body Hamiltonian. In this microscopic quasiparticle-phonon model (MQPM) the relevant part of the three-quasiparticle Hilbert space may possibly be taken into account even in calculations using large single-particle bases. As an example, the MQPM is applied to the calculation of energy levels and Fermi and Gamow-Teller beta-decay transition amplitudes for transitions between odd-mass ${}^{127\ensuremath{-}133}\mathrm{Xe}$, ${}^{127\ensuremath{-}133}\mathrm{I}$, and ${}^{127\ensuremath{-}133}\mathrm{Cs}$ isotopes. Considering the fully microscopic nature of the MQPM, comparison of its results and da…

PhysicsNuclear and High Energy PhysicsIsotopePhononHilbert spaceEquations of motionsymbols.namesakeAmplitudeQuantum mechanicsQuasiparticlesymbolsCondensed Matter::Strongly Correlated ElectronsAtomic physicsHamiltonian (quantum mechanics)Fermi Gamma-ray Space TelescopePhysical Review C
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Theoretical study of incoherent phi photoproduction on a deuteron target

2012

We study the photoproduction of phi mesons in deuteron, paying attention to the modification of the cross section from bound protons to the free ones with the aim of comparing with recent results at LEPS. For this purpose we take into account Fermi motion in single scattering and rescattering of the phi to account for phi absorption on a second nucleon as well as the rescattering of the proton. We find that the contribution of the double scattering is much smaller than the typical cross section of gamma p to phi p in free space, which implies a very small screening of the phi production in deuteron. The contribution from the proton rescattering, on the other hand, is found to be not negligi…

PhysicsNuclear and High Energy PhysicsMesonProtonNuclear Theory010308 nuclear & particles physicsScatteringNuclear TheoryFísicaFOS: Physical sciences01 natural sciences7. Clean energyNuclear physicsMomentumNuclear Theory (nucl-th)Cross section (physics)Phase space0103 physical sciences010306 general physicsNucleonNuclear ExperimentFermi Gamma-ray Space Telescope
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Conservative upper limits on WIMP annihilation cross section from Fermi-LAT γ rays

2012

The spectrum of an isotropic extragalactic {\gamma}-ray background (EGB) has been measured by the Fermi-LAT telescope at high latitudes. Two new models for the EGB are derived from the subraction of unresolved point sources and extragalactic diffuse processes, which could explain from 30% to 70% of the Fermi-LAT EGB. Within the hypothesis that the two residual EGBs are entirely due to the annihilation of dark matter (DM) particles in the Galactic halo, we obtain stringent upper limits on their annihilation cross section. Severe bounds on a possible Sommerfeld enhancement of the annihilation cross section are set as well. Finally, we consider models for DM annihilation depending on the inver…

PhysicsNuclear and High Energy PhysicsParticle physicsAnnihilationdark matter theoryAstrophysics::High Energy Astrophysical PhenomenaDark matterGamma raysGamma rayAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalactic haloGamma rays; dark matter theoryPulsarWIMPHaloAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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Scalar isoscalar pion pairs in nuclei and theA(π,ππ)Xreaction

1999

The reaction A(pi,pi pi)X has been studied at low energies, paying particular attention to the interaction of the two final pions in the scalar isoscalar (I=J=0) channel. We have developed a microscopic model for the pion production, and then implemented the two pion final state interaction by using the results of a non-perturbative unitary coupled-channels method based in the standard chiral Lagrangians. The resulting model, describes well the reaction on the nucleon for all different isospin channels. Finally, we have considered the reaction in nuclei. Our calculation takes into account Fermi motion, Pauli blocking, pion absorption, and also the strong modification of the pi-pi interactio…

PhysicsNuclear and High Energy PhysicsParticle physicsIsoscalarNuclear TheoryScalar (mathematics)Nuclear physicssymbols.namesakePauli exclusion principlePionDeuteriumIsospinsymbolsNuclear ExperimentNucleonFermi Gamma-ray Space TelescopePhysical Review C
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Quasielastic neutrino (antineutrino) reactions in nuclei and the axial-vector form factor of the nucleon

1992

Abstract Quasielastic neutrino and antineutrino reactions in nuclei are studied to investigate the effect of the nuclear medium on the determination of axial dipole mass M A in nuclei. The calculations are done in the local density approximation and various nuclear effects like Pauli blocking, Fermi motion of nucleons and strong renormalization effects in the spin-isospin channel are taken into account. The nuclear effects are found to be quite large at low q 2 , but the data in this region are too meagre to influence the determination of M A . The experimental data on differential and total cross sections are found to be consistent with M A as determined from deuterium experiments and no c…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryForm factor (quantum field theory)Nuclear physicsDipolesymbols.namesakePauli exclusion principleDeuteriumsymbolsNeutrinoNuclear ExperimentNucleonPseudovectorFermi Gamma-ray Space TelescopeNuclear Physics A
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Mesonic and binding contributions to the EMC effect in a relativistic many-body approach

1996

We revise the conventional nuclear effects of Fermi motion, binding and pionic effects in deep inelastic lepton scattering using a relativistic formalism for an interacting Fermi sea and the local density approximation to translate results from nuclear matter to finite nuclei. In addition we also consider effects from rho-meson renormalization in the nucleus. The use of nucleon Green's functions in terms of their spectral functions offers a precise way to account for Fermi motion and binding. On the other hand the use of many body Feynman diagrams in a relativistic framework allows one to avoid using prescriptions given in the past to introduce relativistic corrections in a non relativistic…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryMesonHigh Energy Physics::PhenomenologyEMC effectNuclear TheoryFOS: Physical sciencesFísicaNuclear matterNuclear Theory (nucl-th)RenormalizationHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)symbolsFeynman diagramNucleonNuclear ExperimentFermi Gamma-ray Space TelescopeLepton
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Antihyperon potentials in nuclei via exclusive antiproton–nucleus reactions

2015

Abstract The exclusive production of hyperon–antihyperon pairs close to their production threshold in p ‾ -nucleus collisions offers a unique and hitherto unexplored opportunity to elucidate the behavior of antihyperons in nuclei. For the first time we analyze these reactions in a microscopic transport model using the Giesen Boltzmann–Uehling–Uhlenbeck transport model. The calculation takes the delicate interplay between the strong absorption of antihyperons, their rescattering and mean field deflection as well as the Fermi motion of the struck nucleon into account. We find a substantial sensitivity of transverse momentum correlations of coincident Λ ‾ Λ -pairs to the assumed depth of the Λ…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear Theorylcsh:QC1-999IonNuclear physicsmedicine.anatomical_structureDeflection (physics)Mean field theoryAntiprotonmedicineFacility for Antiproton and Ion ResearchNuclear ExperimentNucleonNucleuslcsh:PhysicsFermi Gamma-ray Space TelescopePhysics Letters B
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Relativistic direct Urca processes in cooling neutron stars

2001

We derive a relativistic expression for neutrino energy losses caused by the direct Urca processes in degenerate baryon matter of neutron stars. We use two different ways to calculate the emissivity caused by the reactions to our interest. First we perform a standard calculation by Fermi's ''golden'' rule. The second calculation, resulting in the same expression, is performed with the aid of polarization functions of the medium. Our result for neutrino energy losses strongly differs from previous non-relativistic results. We also discuss nonconservation of the baryon vector current in reactions through weak charged currents in the medium, when the asymmetry between protons and neutrons is c…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear Theorymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Degenerate energy levelsNuclear TheoryFOS: Physical sciencesFísicaAstrophysicsPolarization (waves)AsymmetryNuclear Theory (nucl-th)BaryonHigh Energy Physics - PhenomenologyNeutron starHigh Energy Physics - Phenomenology (hep-ph)NeutronNeutrinoNuclear Experimentmedia_commonFermi Gamma-ray Space Telescope
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Nuclear medium effects inν(ν¯)-nucleus deep inelastic scattering

2011

We study nuclear medium effects in the weak structure functions ${F}_{2}(x,{Q}^{2})$ and ${F}_{3}(x,{Q}^{2})$ in the deep inelastic neutrino and antineutrino induced reactions in nuclei. We use a theoretical model for the nuclear spectral functions which incorporates the conventional nuclear effects, such as Fermi motion, binding, and nucleon correlations. We also consider the pion and rho meson cloud contributions calculated from a microscopic model for meson-nucleus self-energies. The calculations have been performed using relativistic nuclear spectral functions. Our results are compared with the experimental data of the NuTeV and the CERN Dortmund Heidelberg Saclay Warsaw (CDHSW) collabo…

PhysicsNuclear and High Energy PhysicsParticle physicsRho mesonLarge Hadron Collider010308 nuclear & particles physicsNuclear TheoryDeep inelastic scattering01 natural sciences7. Clean energyNuclear physicsPionDeuterium0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoNuclear Experiment010306 general physicsNucleonFermi Gamma-ray Space TelescopePhysical Review C
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