Search results for "GAMMA-RAY"

showing 10 items of 374 documents

Strongly correlated one-dimensional Bose–Fermi quantum mixtures: symmetry and correlations

2017

We consider multi-component quantum mixtures (bosonic, fermionic, or mixed) with strongly repulsive contact interactions in a one-dimensional harmonic trap. In the limit of infinitely strong repulsion and zero temperature, using the class-sum method, we study the symmetries of the spatial wave function of the mixture. We find that the ground state of the system has the most symmetric spatial wave function allowed by the type of mixture. This provides an example of the generalized Lieb-Mattis theorem. Furthermore, we show that the symmetry properties of the mixture are embedded in the large-momentum tails of the momentum distribution, which we evaluate both at infinite repulsion by an exact …

PhysicsCondensed Matter::Quantum Gases[PHYS]Physics [physics][PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]FOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesSymmetry (physics)010305 fluids & plasmasQuantum Gases (cond-mat.quant-gas)Quantum mechanics0103 physical sciences[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]010306 general physicsCondensed Matter - Quantum GasesQuantumComputingMilieux_MISCELLANEOUSFermi Gamma-ray Space Telescope
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Experimental Manifestations of Fermion Condensation in 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 the Landau–Fermi liquid theory fails. Instead, these systems exhibit non-Fermi-liquid properties that arise from violation of time-reversal (T) and particle– hole (C) invariance. Here we consider two most recent experimental puzzles, which cannot be explained neither within the Landau–Fermi liquid picture nor can they be made intelligible by the approaches like the Hubbard model and/or the Kondo effect, which are commonly used to spell out the typical non-Fermi-liquid behavior. The first experimental puzzle is the asymmetric (with…

PhysicsCondensed matter physicsCondensationGeneral Physics and AstronomyFermionFermi Gamma-ray Space TelescopeActa Physica Polonica A
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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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GrailQuest and HERMES: hunting for gravitational wave electromagnetic counterparts and probing space-time quantum foam

2021

GrailQuest (Gamma-ray Astronomy International Laboratory for Quantum Exploration of Space-Time) is an ambitious astrophysical mission concept that uses a fleet of small satellites whose main objective is to search for a dispersion law for light propagation in vacuo. Within Quantum Gravity theories, different models for space-time quantization predict relative discrepancies of the speed of photons w.r.t. the speed of light that depend on the ratio of the photon energy to the Planck energy. This ratio is as small as 10-23 for photons in the γ- ray band (100 keV). Therefore, to detect this effect, light must propagate over enormous distances and the experiment must have extraordinary sensitivi…

PhysicsCubeSatsGamma-Ray BurstsPhotonGravitational Wave counterparts010308 nuclear & particles physicsGravitational waveSpace timeQuantum gravityAstronomyTriangulation (social science)01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaAll-sky monitorObservatoryX-rays0103 physical sciencesQuantum gravityNano-satellitesTemporal triangulationGamma-ray burstQuantum foam010303 astronomy & astrophysics
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Calibration and Simulation of the GRB trigger detector of the Ultra Fast Flash Observatory

2013

The UFFO (Ultra-Fast Flash Observatory) is a GRB detector on board the Lomonosov satellite, to be launched in 2013. The GRB trigger is provided by an X-ray detector, called UBAT (UFFO Burst Alarm & Trigger Telescope), which detects X-rays from the GRB and then triggers to determine the direction of the GRB and then alerts the Slewing Mirror Telescope (SMT) to turn in the direction of the GRB and record the optical photon fluxes. This report details the calibration of the two components: the MAPMTs and the YSO crystals and simulations of the UBAT. The results shows that this design can observe a GRB within a field of view of ±35° and can trigger in a time scale as short as 0.2 – 1.0 s af…

PhysicsDetectorGeneral EngineeringAstronomy and AstrophysicsField of viewAstrophysicslaw.inventionTelescopeFlash (photography)Space and Planetary SciencelawObservatoryCalibrationSatelliteGamma-ray burst
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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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