Search results for " gamma-ray"

showing 10 items of 172 documents

Fermion Condensation in Strongly Interacting Fermi Liquids

2017

This article discusses the construction of a theory which is capable to explain so-called non-Fermi liquid behavior of strongly correlated Fermi systems. We show that such explanation can be done within the framework of a so-called fermion condensation approach. In this approach, as a result of fermion condensation quantum phase transition, ordinary Landau quasiparticles do not decay, but reborn, gaining new properties, as Phoenix from the ashes. The physical reason for that is altering of Fermi surface topology. To be more specific, in contrast to standard Landau paradigm stating that the quasiparticle effective mass does not depend on external stimuli like magnetic field and/or temperatur…

PhysicsCondensed matter physicsHeavy fermionCondensationheavy-fermion compoundsFermionFermi liquid theoryquantum phase transitionfermion condensationNon-Fermi liquid behaviorFermi Gamma-ray Space Telescope
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ESTREMO/WFXRT: Extreme phySics in the TRansient and Evolving COsmos

2006

We present a mission designed to address two main themes of the ESA Cosmic Vision Programme: the Evolution of the Universe and its Violent phenomena. ESTREMO/WFXRT is based on innovative instrumental and observational approaches, out of the mainstream of observatories of progressively increasing area, i.e.: Observing with fast reaction transient sources, like GRB, at their brightest levels, thus allowing high resolution spectroscopy. Observing and surveying through a X-ray telescope with a wide field of view and with high sensitivity extended sources, like cluster and Warm Hot Intragalactic Medium (WHIM). ESTREMO/WFXRT will rely on two cosmological probes: GRB and large scale X-ray structur…

PhysicsCosmic VisionAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectDark matterAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyX-ray telescopeAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmologyUniverselaw.inventionTelescopeSettore FIS/05 - Astronomia e AstrofisicalawX-ray instruments Cosmology Gamma-Ray Bursts Clusters of galaxiesDark energyGamma-ray burstmedia_common
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Dark matter scattering on electrons: Accurate calculations of atomic excitations and implications for the DAMA signal

2016

We revisit the WIMP-type dark matter scattering on electrons that results in atomic ionization and can manifest itself in a variety of existing direct-detection experiments. Unlike the WIMP-nucleon scattering, where current experiments probe typical interaction strengths much smaller than the Fermi constant, the scattering on electrons requires a much stronger interaction to be detectable, which in turn requires new light force carriers. We account for such new forces explicitly, by introducing a mediator particle with scalar or vector couplings to dark matter and to electrons. We then perform state-of-the-art numerical calculations of atomic ionization relevant to the existing experiments.…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsScatteringPhysics beyond the Standard ModelDark matterScalar (mathematics)FOS: Physical sciencesElectron01 natural sciencesHigh Energy Physics - ExperimentPhysics - Atomic PhysicsComputational physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Ionization0103 physical sciencesAtomic physics010306 general physicsRelativistic quantum chemistryAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopePhysical Review D
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A measurement of the tau lifetime

1993

The tau lepton lifetime is measured using four different methods with the DELPHI detector. Three measurements using one prong decays are combined, accounting for correlations, resulting in tau(tau) = 298 +/- 7 (stat.) +/- 4 (syst.) fs while the decay length distribution of three prong decays gives tau(tau) = 298 +/- 13 (stat.) +/- 5 (syst.) fs. The combined result is tau(tau) = 298 +/- 7 fs. The ratio of the Fermi coupling constant from tau decay relative to that from muon decay is found to be 0.985 +/- 0.013, compatible with lepton universality.

PhysicsCoupling constantParticle physicsArgusNuclear and High Energy PhysicsMuonPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsElectron–positron annihilation01 natural sciences7. Clean energyNuclear physics0103 physical sciencesDecay lengthLEPTONS[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentFísica nuclearCombined result010306 general physicscomputerParticle Physics - ExperimentFermi Gamma-ray Space TelescopeLeptoncomputer.programming_language
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CONSTRUCTION OF METASTABLE STATES IN QUANTUM ELECTRODYNAMICS

2004

In this paper, we construct metastable states of atoms interacting with the quantized radiation field. These states emerge from the excited bound states of the non-interacting system. We prove that these states obey an exponential time-decay law. In detail, we show that their decay is given by an exponential function in time, predicted by Fermi's Golden Rule, plus a small remainder term. The latter is proportional to the (4+β)th power of the coupling constant and decays algebraically in time. As a result, though it is small, it dominates the decay for large times. A central point of the paper is that our remainder term is significantly smaller than the one previously obtained in [1] and as…

PhysicsCoupling constantStatistical and Nonlinear PhysicsExponential functionsymbols.namesakeQuantum mechanicsQuantum electrodynamicsMetastabilityExcited stateBound statesymbolsFermi's golden ruleRemainderMathematical PhysicsFermi Gamma-ray Space TelescopeReviews in Mathematical Physics
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The influence of Fermi motion on the comparison of the polarization transfer to a proton in elastic e→p and quasi-elastic e→A scattering

2019

Abstract A comparison between polarization-transfer to a bound proton in quasi-free kinematics by the A ( e → , e ′ p → ) knockout reaction and that in elastic scattering off a free proton can provide information on the characteristics of the bound proton. In the past the reported measurements have been compared to those of a free proton with zero initial momentum. We introduce, for the first time, expressions for the polarization-transfer components when the proton is initially in motion and compare them to the 2H data measured at the Mainz Microtron (MAMI). We show the ratios of the transverse ( P x ) and longitudinal ( P z ) components of the polarization transfer in H 2 ( e → , e ′ p → …

PhysicsElastic scatteringNuclear and High Energy Physics010308 nuclear & particles physicsScatteringInitial momentumNuclear TheoryKinematicsPolarization (waves)01 natural sciences7. Clean energyTransverse plane0103 physical sciencesPhysics::Accelerator PhysicsAtomic physicsNuclear Experiment010306 general physicsMicrotronFermi Gamma-ray Space TelescopePhysics Letters B
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The Corona of the Sun as a Star

2006

We study the physics of the solar corona as a whole, i.e. of the Sun as a Star, in order to understand its global features and to provide a template for stellar coronae. In this process we strive to understand the features of various structures which compose the solar corona. This process in not straightforward given the problems of observing the Sun as a whole: e.g., no recent X‐ray wide‐band, medium‐resolution, spectrum of the Sun is avaible, unlike stars and no X‐ray spectral monitoring of the Sun at various activity phases is available. The presentation will discuss our work in this field; we present the method we have devised, based on Yohkoh/SXT data, to derive the Differential Emissi…

PhysicsField (physics)Astrophysics::High Energy Astrophysical PhenomenaStellar atmosphereAstronomyA* search algorithmAstrophysicsCoronal radiative lossesCoronaCorona X-ray and gamma-ray emission X-raylaw.inventionStarsSettore FIS/05 - Astronomia E AstrofisicalawPhysics::Space PhysicsCoronal heatingAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsX ray spectra
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Thermal Transport and Wiedemann-Franz Law in the Disordered Fermi Liquid

2014

We study thermal transport in the disordered Fermi liquid at low temperatures. Gravitational potentials are used as sources for finding the heat density and its correlation function. For a comprehensive study, we extend the renormalization group (RG) analysis developed for electric transport by including the gravitational potentials into the RG scheme. Our analysis reveals that the Wiedemann-Franz law remains valid even in the presence of quantum corrections caused by the interplay of diffusion modes and the electron electron interaction. In the present scheme this fundamental relation is closely connected with a fixed point in the multi-parametric RG-flow of the gravitational potentials.

PhysicsField (physics)Condensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsStrongly Correlated Electrons (cond-mat.str-el)SigmaFOS: Physical sciencesCondensed Matter::Mesoscopic Systems and Quantum Hall EffectCondensed Matter Physics530Electronic Optical and Magnetic MaterialsGravitationNonlinear systemCondensed Matter - Strongly Correlated ElectronsThermal transportCondensed Matter::SuperconductivityQuantum mechanicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)Fermi liquid theoryWiedemann–Franz lawFermi Gamma-ray Space Telescope
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GrailQuest: hunting for atoms of space and time hidden in the wrinkle of Space-Time: A swarm of nano/micro/small-satellites to probe the ultimate str…

2021

AbstractGrailQuest(Gamma Ray Astronomy International Laboratory for QUantum Exploration of Space-Time) is a mission concept based on a constellation (hundreds/thousands) of nano/micro/small-satellites in low (or near) Earth orbits. Each satellite hosts a non-collimated array of scintillator crystals coupled with Silicon Drift Detectors with broad energy band coverage (keV-MeV range) and excellent temporal resolution (≤ 100 nanoseconds) each with effective area$\sim 100 \text {cm}^{2}$∼100cm2. This simple and robust design allows for mass-production of the satellites of the fleet. This revolutionary approach implies a huge reduction of costs, flexibility in the segmented launching strategy, …

PhysicsGamma-Ray Burstsγ-ray sourceAll-sky monitor; Constellation of satellites; Gamma-Ray Bursts; Quantum gravity; γ-ray sourcesPhotonbusiness.industryGravitational waveHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaConstellation of satellitesQuantum gravityAstronomy and AstrophysicsGamma-ray astronomyGamma-Ray Burstγ-ray sourcesOpticsConstellation of satelliteAll-sky monitorSpace and Planetary ScienceObservatoryTemporal resolutionSatellitebusinessGeocentric orbit
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Closure relations during the plateau emission of Swift GRBs and the fundamental plane

2021

The Neil Gehrels Swift observatory observe Gamma-Ray bursts (GRBs) plateaus in X-rays. We test the reliability of the closure relations through the fireball model when dealing with the GRB plateau emission. We analyze 455 X-ray lightcurves (LCs) collected by \emph{Swift} from 2005 (January) until 2019 (August) for which the redshift is both known and unknown using the phenomenological Willingale 2007 model. Using these fits, we analyze the emission mechanisms and astrophysical environments of these GRBs through the closure relations within the time interval of the plateau emission. Finally, we test the 3D fundamental plane relation (Dainotti relation) which connects the prompt peak luminosi…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaCosmic distance ladderFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics) gamma-ray burst: general [(stars]Astrophysics::Cosmology and Extragalactic AstrophysicsPlateau (mathematics)non-thermal [radiation mechanisms]01 natural sciencesRedshiftLuminositySpace and Planetary ScienceObservatory0103 physical sciencesISM [X-rays]Flatness (cosmology)Gamma-ray burstFundamental plane (elliptical galaxies)Astrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics
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