Search results for " gamma-ray"

showing 10 items of 172 documents

Decoherence in a fermion environment: Non-Markovianity and Orthogonality Catastrophe

2013

We analyze the non-Markovian character of the dynamics of an open two-level atom interacting with a gas of ultra-cold fermions. In particular, we discuss the connection between the phenomena of orthogonality catastrophe and Fermi edge singularity occurring in such a kind of environment and the memory-keeping effects which are displayed in the time evolution of the open system.

Statistics and ProbabilityPhysicsCondensed Matter::Quantum GasesQuantum PhysicsQuantum decoherenceTime evolutionFOS: Physical sciencesStatistical and Nonlinear PhysicsFermionOpen system (systems theory)orthogonality catastrophe markovianitySettore FIS/03 - Fisica Della MateriaTheoretical physicsSingularityQuantum mechanicsQuantum Physics (quant-ph)Mathematical PhysicsFermi Gamma-ray Space Telescope
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Multiple band crossings and Fermi surface topology: Role of double nonsymmorphic symmetries in MnP-type crystal structures

2019

We use relativistic ab-initio methods combined with model Hamiltonian approaches to analyze the normal-phase electronic and structural properties of the recently discovered WP superconductor. Remarkably, the outcomes of such study can be employed to set fundamental connections among WP and the CrAs and MnP superconductors belonging to the same space group. One of the key features of the resulting electronic structure is represented by the occurrence of multiple band crossings along specific high symmetry lines of the Brilloiun zone. In particular, we demonstrate that the eight-fold band degeneracy obtained along the SR path at (kx,ky)=(Pi,Pi) is due to inversion-time reversal invariance and…

SuperconductivityMaterials scienceStrongly Correlated Electrons (cond-mat.str-el)Physics and Astronomy (miscellaneous)Condensed Matter - SuperconductivityDegenerate energy levelsFermi levelFOS: Physical sciencesFermi surface02 engineering and technologyElectronic structure021001 nanoscience & nanotechnologyTopology01 natural sciencesSuperconductivity (cond-mat.supr-con)Brillouin zoneCondensed Matter - Strongly Correlated Electronssymbols.namesake0103 physical sciencessymbolsGeneral Materials Science010306 general physics0210 nano-technologyHamiltonian (quantum mechanics)Fermi Gamma-ray Space TelescopePhysical Review Materials
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Enhanced CDW Transitions in Nb3X4(X = S, Se, Te): Intercalation and Surface Effects

2004

A x Nb 3 X 4 (A = In, Tl, ZnHg; X = S, Se, Te) compounds show CDW instabilities dependent on the type and concentration of intercalate. Tl or In intercalation flattens the Fermi surfaces and supports CDW formation. In the corresponding DOS spectrum the Fermi level is shifted towards coincidence with a small peak, derived mainly from the Nb dz 2 orbital. Localized modulated regions observed in STM images of Nb 3 X 4 at room temperature represent precursor effects to full CDW formation.

Surface (mathematics)Materials scienceCondensed matter physicsFermi levelIntercalation (chemistry)Fermi surfaceElectronic structureCondensed Matter PhysicsElectronic Optical and Magnetic Materialslaw.inventionsymbols.namesakeSmall peaklawsymbolsScanning tunneling microscopeFermi Gamma-ray Space TelescopeFerroelectrics
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Properties of Swift's intermediate bursts

2011

Based on their prompt, high-energy emission, gamma-ray bursts are usually classified into short-duration and long-duration classes. A third intermediate group has been identified on statistical grounds but its individual properties have not yet been studied in detail. Using the large sample of follow-up observations of GRBs produced during the Swift era we analyze the individual characteristics of this group. We find that intermediate bursts are significantly different from short GRBs but share many properties with long bursts, probably pointing to a common progenitor type. However, we find that intermediate bursts are significantly dimmer and have on average lower redshifts. Based on their…

SwiftPhysicsAstrophysics::High Energy Astrophysical PhenomenaGamma rayAstronomyAstrophysicsRedshiftLarge sampleIntermediate groupFIS/05 - ASTRONOMIA E ASTROFISICAredshift gamma-rays brightness spectral analysisgamma-ray sources (astronomical) brightness X-ray sources (astronomical)Spectral analysisGamma-ray burstcomputercomputer.programming_language
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EDGE: explorer of diffuse emission and gamma-ray burst explosions

2009

How structures on various scales formed and evolved from the early Universe up to present time is a fundamental question of astrophysical cosmology. EDGE will trace the cosmic history of the baryons from the early generations of massive star by Gamma-Ray Burst (GRB) explosions, through the period of cluster formation, down to very low redshifts, when between a third and one half of the baryons are expected to reside in cosmic filaments undergoing gravitational collapse by dark matter (Warm Hot Intragalactic Medium: WHIM). In addition EDGE, with its unprecedented observational capabilities, will provide key results on several other topics. The science is feasible with a medium class mission …

Vision[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Warm–hot intergalactic mediumAstrophysicsAstrophysics7. Clean energy01 natural sciencesCosmologySettore FIS/05 - Astronomia E AstrofisicaIntergalactic MediumWarm-Hot Intergalactic MediumX-rays Cosmology Clusters Gamma-ray bursts Warm-hot intergalactic medium Missions010303 astronomy & astrophysicsX-ray telescopesX-rays; Cosmology; Clusters; Gamma-ray bursts; Warm– hot intergalactic medium; MissionsPhysicsEquipment and servicesSatellite MissionSpectrometersAstrophysics (astro-ph)X-rays Cosmology Clusters Gamma-ray bursts Warm– hot intergalactic medium MissionsTemperatureAstrophysics::Instrumentation and Methods for AstrophysicsCosmologyGamma-ray burstsCosmic VisionSpectral resolutionGalaxy ClustersAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesWarm&ndashAstrophysics::Cosmology and Extragalactic AstrophysicsMissionshot intergalactic mediumAbsorptionNO010309 opticsX-rayClustersWarm–hot intergalactic mediumGalaxy groups and clusters0103 physical sciencesX-raysGalaxy groups and clustersImaging systems010306 general physicsGamma-ray burstWarm&ndashGalaxy clusterSpatial resolutionSensorsAstronomyX-rays clusters Gamma-Ray Bursts Warm-Hot Intergalactic Medium missionsAstronomy and AstrophysicsGalaxyRedshiftCluster13. Climate actionSpace and Planetary ScienceGamma-ray burstOptics for EUV, X-Ray, and Gamma-Ray Astronomy III. Edited by O'Dell, Stephen L.; Pareschi, Giovanni. Proceedings of the SPIE
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IBIS: The Imager on-board INTEGRAL

2003

The IBIS telescope is the high angular resolution gamma-ray imager on-board the INTEGRAL Observatory, successfully launched from Baikonur (Kazakhstan) the 17th of October 2002. This medium size ESA project, planned for a 2 year mission with possible extension to 5, is devoted to the observation of the gamma-ray sky in the energy range from 3 keV to 10 MeV (Winkler 2001). The IBIS imaging system is based on two independent solid state detector arrays optimised for low ( 15-1000 keV) and high ( 0.175-10.0 MeV) energies surrounded by an active VETO System. This high efficiency shield is essential to minimise the background induced by high energy particles in the highly excentric out of van All…

X-ray transientAstrophysics::High Energy Astrophysical PhenomenaINTEGRAL ; IBIS ; Gamma-ray imagingUNESCO::ASTRONOMÍA Y ASTROFÍSICAlaw.inventionTelescopesymbols.namesakeOpticslawObservatoryGamma-ray imagingAngular resolutionCoded aperturePhysicsIbisbiologyINTEGRALbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsbiology.organism_classification:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary ScienceVan Allen radiation beltsymbolsIBISUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniabusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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γ-RAY AND PARSEC-SCALE JET PROPERTIES OF A COMPLETE SAMPLE OF BLAZARS FROM THE MOJAVE PROGRAM

2011

著者人数: 145名

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenagalaxies: activePopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio spectrumLuminosityRelativistic beamingquasars: generalgamma rays: galaxiesgalaxies0103 physical sciencesgalaxie [gamma rays]educationBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)radio continuum: galaxiesPhysicseducation.field_of_studygeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsQuasarBL Lacertae objects: generalgalaxies: jetsgalaxies [radio continuum]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; galaxies quasars: generaljet [galaxies]BL Lacertae objects: general; galaxies: active; galaxies: jets; gamma rays: galaxies; quasars: general; radio continuum: galaxiesSpace and Planetary Scienceactive [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopeThe Astrophysical Journal
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Observatory science with eXTP

2019

Disponible preprint en: arXiv:1812.04023v1 [astro-ph.HE] [v1] Mon, 10 Dec 2018 19:00:52 UTC (4,376 KB)

cataclysmic binariesAstronomyFIELD CAMERAS OBSERVATIONSspace research instruments nuclear astrophysics flare stars accretion and accretion disks mass loss and stellar winds cataclysmic binaries X-ray binaries supernova remnants active galactic nuclei X-ray bursts gamma-ray bursts gravitational wavesGeneral Physics and Astronomygamma-ray burstspace research instrument01 natural sciencesGamma ray burstsObservatoryAccretion and accretion disksAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsgravitational waveaccretion and accretion diskPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)supernova remnants[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]flare starsgamma-ray burstsAstrophysics::Instrumentation and Methods for Astrophysicsaccretion and accretion disks; active galactic nuclei; cataclysmic binaries; flare stars; gamma-ray bursts; gravitational waves; mass loss and stellar winds; nuclear astrophysics; space research instruments; supernova remnants; X-ray binaries; X-ray bursts; Physics and Astronomy (all)Space research instrumentsX ray burstSupernovaX-ray binariesgravitational wavesaccretion and accretion disksQUIETHigh massX-ray binarieMass loss and stellar windsNuclear astrophysicsGamma-ray burstsspace research instrumentsAstrophysics - High Energy Astrophysical PhenomenaPULSAR-WIND NEBULAEFAST RADIO-BURSTSAstrofísica nuclearActive galactic nucleusTIDAL DISRUPTIONSupernova remnantsAstrophysics::High Energy Astrophysical Phenomenanuclear astrophysicsPolarimetryFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsACCRETING NEUTRON-STARSaccretion and accretion disks; active galactic nuclei; cataclysmic binaries; flare stars; gamma-ray bursts; gravitational waves; mass loss and stellar winds; nuclear astrophysics; space research instruments; supernova remnants; X-ray binaries; X-ray burstsGravitational wavesPhysics and Astronomy (all)cataclysmic binarieSettore FIS/05 - Astronomia e AstrofisicaSUPERMASSIVE BLACK-HOLES0103 physical sciences010306 general physicsX-ray burstAstrophysics::Galaxy AstrophysicsCataclysmic binariesActive galactic nucleiflare starAstronomyWhite dwarfFlare starsStarssupernova remnantQB460-466 Astrophysics[SDU]Sciences of the Universe [physics]mass loss and stellar wind:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]active galactic nucleiX-RAYX-ray burstsSupernova remmantsmass loss and stellar windsX ray binaries[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]SEYFERT 1 GALAXYnuclear astrophysic
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Flat bands and strongly correlated Fermi systems

2019

Many strongly correlated Fermi systems including heavy-fermion (HF) metals and high-Tc superconductors belong to that class of quantum many-body systems for which Landau Fermiliquid (LFL) theory fails. Instead, these systems exhibit non-Fermi-liquid properties that arise from violation of time-reversal (T) and particle-hole (C) invariance. Measurements of tunneling conductance provide a powerful experimental tool for detecting violations of these basic symmetries inherent to LFLs, which guarantee that the measured differential conductivity dI/dV, where I is the current and V the bias voltage, is a symmetric function of V. Thus, it has been predicted that the conductivity becomes asymmetric …

flat bandsPhysicstunneling conductanceTunneling conductancestrongly correlated Fermi systemsCondensed matter physicsCondensed Matter PhysicsMathematical PhysicsAtomic and Molecular Physics and OpticsFermi Gamma-ray Space TelescopePhysica Scripta
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