Search results for " gamma-ray"

showing 10 items of 172 documents

NH3 dynamics in Zn(NH3)4I2 and Zn(NH3)4Br2 investigated by incoherent quasielastic neutron scattering

1997

We report on studies of NH3 dynamics in Zn(NH3)4I2 and Zn(NH3)4Br2 by means of incoherent quasielastic neutron scattering in the temperature range from 150 to 300 K. Quasielastic experiments were carried out on the Fermi chopper time-of-flight spectrometer at NIST. The Lorentzian full-widths at half-maximum, ƒw, of the quasielastic line follow an Arrhenius law and increase from 0.39 [0.25] meV at 150 K to 1.33 [0.80] meV at 300 K. We find an activation energy Ea for the NH3 reorientations of 32(1) and 30(3) meV for Zn(NH3)4I2 and Zn(NH3)4Br2, respectively.

PhysicsArrhenius equationQuasielastic scatteringSpectrometerAnalytical chemistryActivation energyAtmospheric temperature rangeCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsNuclear physicssymbols.namesakeQuasielastic neutron scatteringsymbolsElectrical and Electronic EngineeringFermi Gamma-ray Space TelescopeLine (formation)Physica B: Condensed Matter
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High energy neutrinos from novae in symbiotic binaries: The case of V407 Cygni

2010

Detection of high-energy (>= 100 MeV) gamma rays by the Fermi Large Area Telescope from a nova in the symbiotic binary system V407 Cygni has opened the possibility of high-energy neutrino detection from this type of source. A thermonuclear explosion on the white dwarf surface sets off a nova shell in motion that expands and slows down in a dense surrounding medium provided by the red giant companion. Particles are accelerated in the shocks of the shell and interact with the surrounding medium to produce observed gamma rays. We show that proton-proton interaction, which is most likely responsible for producing gamma rays via neutral pion decay, produces >= 0:1 GeV neutrinos that can be detec…

PhysicsAstrofísicaHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsRed giantAstrophysics::High Energy Astrophysical PhenomenaWhite dwarfFOS: Physical sciencesCosmic rayAstrophysicsType (model theory)High Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)PionHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorAstrophysics::Solar and Stellar AstrophysicsNeutrinoAstrophysics - High Energy Astrophysical PhenomenaNuclear ExperimentAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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Constraining spectral models of a terrestrial gamma‐ray flash from a terrestrial electron beam observation by the Atmosphere‐Space Interactions Monit…

2021

Terrestrial Gamma ray Flashes (TGFs) are short flashes of high energy photons, produced by thunderstorms. When interacting with the atmosphere, they produce relativistic electrons and positrons, and a part gets bounded to geomagnetic field lines and travels large distances in space. This phenomenon is called a Terrestrial Electron Beam (TEB). The Atmosphere-Space Interactions Monitor (ASIM) mounted on-board the International Space Station detected a new TEB event on March 24, 2019, originating from the tropical cyclone Johanina. Using ASIM's low energy detector, the TEB energy spectrum is resolved down to 50 keV. We provide a method to constrain the TGF source spectrum based on the detected…

PhysicsAtmosphereGeophysicsCathode rayGeneral Earth and Planetary SciencesSpace (mathematics)Computational physicsTerrestrial gamma-ray flash
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Production altitude and time delays of the terrestrial gamma flashes: Revisiting the Burst and Transient Source Experiment spectra

2008

[1] On the basis of the RHESSI results it has been suggested that terrestrial gamma flashes (TGFs) are produced at very low altitudes. On the other hand some of the Burst and Transient Source Experiment (BATSE) spectra show unabsorbed fluxes of X rays in the 25–50 keV energy range, indicating a higher production altitude. To investigate this, we have developed a Monte Carlo code for X-ray propagation through the atmosphere. The most important features seen in the modeled spectra are (1) a low-energy cutoff which moves to lower energies as TGFs are produced at higher altitudes, (2) a high-energy cutoff which moves to lower energies as TGFs are observed at larger zenith angles, and (3) time d…

PhysicsAtmospheric ScienceEcologyAstrophysics::High Energy Astrophysical PhenomenaCompton scatteringPaleontologySoil ScienceForestryAstrophysicsAquatic ScienceOceanographySpectral lineAtmosphereGeophysicsAltitudeRelativistic runaway electron avalancheSpace and Planetary ScienceGeochemistry and PetrologyPhysics::Space PhysicsEarth and Planetary Sciences (miscellaneous)Atmospheric electricityZenithEarth-Surface ProcessesWater Science and TechnologyTerrestrial gamma-ray flashJournal of Geophysical Research: Space Physics
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Universality of Many-Body States in Rotating Bose and Fermi Systems

2008

We propose a universal transformation from a many-boson state to a corresponding many-fermion state in the lowest Landau level approximation of rotating many-body systems, inspired by the Laughlin wave function and by the Jain composite-fermion construction. We employ the exact-diagonalization technique for finding the many-body states. The overlap between the transformed boson ground state and the true fermion ground state is calculated in order to measure the quality of the transformation. For very small and high angular momenta, the overlap is typically above 90%. For intermediate angular momenta, mixing between states complicates the picture and leads to small ground-state overlaps at s…

PhysicsCondensed Matter::Quantum GasesCondensed Matter - Mesoscale and Nanoscale PhysicsFOS: Physical sciencesFermionAtomic and Molecular Physics and OpticsMany bodyUniversality (dynamical systems)Condensed Matter - Other Condensed MatterQuantum mechanicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)Mathematics::Metric GeometryWave functionGround stateOther Condensed Matter (cond-mat.other)BosonFermi Gamma-ray Space Telescope
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Scissors modes of two-component degenerate gases: Bose-Bose and Bose-Fermi mixtures

2003

We investigate the scissors modes in binary mixtures of degenerate dilute quantum gases, for both Bose-Bose and Bose-Fermi mixtures. For the latter we consider both the superfluid and normal hydrodynamic and collisionless regimes. We analyze the dependence of the frequencies of the scissors modes and their character as a function of the Bose-Fermi coupling and the trap geometry. We show that the scissors mode can reveal a clear trace of the hydrodynamic behavior of the Fermi gas.

PhysicsCondensed Matter::Quantum GasesCondensed matter physicsComponent (thermodynamics)Condensed Matter::OtherDegenerate energy levelsFOS: Physical sciencesFermionCondensed Matter - Soft Condensed MatterAtomic and Molecular Physics and Opticslaw.inventionSuperfluidityCoupling (physics)lawSoft Condensed Matter (cond-mat.soft)Fermi gasBose–Einstein condensateFermi Gamma-ray Space Telescope
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Free-fall expansion of finite-temperature Bose-Einstein condensed gas in the non Thomas-Fermi regime

2008

We report on our study of the free-fall expansion of a finite-temperature Bose-Einstein condensed cloud of 87Rb. The experiments are performed with a variable total number of atoms while keeping constant the number of atoms in the condensate. The results provide evidence that the BEC dynamics depends on the interaction with thermal fraction. In particular, they provide experimental evidence that thermal cloud compresses the condensate.

PhysicsCondensed Matter::Quantum GasesCondensed matter physicsCondensed Matter::OtherFOS: Physical sciencesFraction (chemistry)Condensed Matter PhysicsAtomic and Molecular Physics and Opticslaw.inventionCondensed Matter - Other Condensed MatterlawThermalConstant (mathematics)Bose–Einstein condensateOther Condensed Matter (cond-mat.other)Fermi Gamma-ray Space TelescopeVariable (mathematics)
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Coherence and clock shifts in ultracold fermi gases with resonant interactions.

2007

Using arguments based on sum rules, we derive a general result for the average shifts of rf lines in Fermi gases in terms of interatomic interaction strengths and two-particle correlation functions. We show that near an interaction resonance shifts vary inversely with the atomic scattering length, rather than linearly as in dilute gases, thus accounting for the experimental observation that clock shifts remain finite at Feshbach resonances.

PhysicsCondensed Matter::Quantum GasesStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - SuperconductivityGeneral Physics and AstronomyResonanceFOS: Physical sciencesScattering lengthSuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsAtomic physicsFermi gasFeshbach resonanceFermi Gamma-ray Space TelescopeCoherence (physics)Physical review letters
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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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