Search results for "Gamma ray spectra"

showing 3 items of 3 documents

Reliability of Monte Carlo event generators for gamma-ray dark matter searches

2013

We study the differences in the gamma-ray spectra simulated by four Monte Carlo event generator packages developed in particle physics. Two different versions of PYTHIA and two of HERWIG are analyzed, namely PYTHIA 6.418 and HERWIG 6.5.10 in Fortran and PYTHIA 8.165 and HERWIG 2.6.1 in C++. For all the studied channels, the intrinsic differences between them are shown to be significative and may play an important role in misunderstanding dark matter signals.

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FortranMonte Carlo methodDark matterFOS: Physical sciencesGamma ray spectra01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Reliability (semiconductor)0103 physical sciences010303 astronomy & astrophysicsEvent generatorcomputer.programming_languageHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGamma rayFísicaHigh Energy Physics - PhenomenologyMonte Carlo SimulationsAstrophysics - High Energy Astrophysical PhenomenacomputerEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics
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Linking gamma-ray spectra of supernova remnants to the cosmic ray injection properties in the aftermath of supernovae

2017

The acceleration times of the highest-energy particles which emit gamma-rays in young and middle-age SNRs are comparable with SNR age. If the number of particles starting acceleration was varying during early times after the supernova explosion then this variation should be reflected in the shape of the gamma-ray spectrum. We use the solution of the non-stationary equation for particle acceleration in order to analyze this effect. As a test case, we apply our method to describe gamma-rays from IC443. As a proxy of the IC443 parent supernova we consider SN1987A. First, we infer the time dependence of injection efficiency from evolution of the radio spectral index in SN1987A. Then, we use the…

Particle numberAstrophysics::High Energy Astrophysical PhenomenaSupernovae: generalFOS: Physical sciencesGamma ray spectraCosmic rayAstrophysics01 natural sciences0103 physical sciences010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy AstrophysicsGamma rays: ISMPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral index010308 nuclear & particles physicsGamma raySpectral densityAstronomy and AstrophysicsAstronomy and AstrophysicCosmic rayParticle accelerationSupernovaSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Spectroscopy of the neutron-deficient nuclide 171Pt

2003

A number of previously unobserved gamma-rays emitted from the neutron-deficient nuclide Pt-171 have been identified using the recoil decay tagging technique. The level scheme has been updated using ...

PhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryHadronGamma ray spectraNuclear physicsRecoilNuclear fusionNeutronNuclideAtomic physicsNuclear ExperimentSpectroscopyThe European Physical Journal A
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