Search results for " gamma-ray"

showing 10 items of 172 documents

Pairing gap and in-gap excitations in trapped fermionic superfluids

2004

We consider trapped atomic Fermi gases with Feshbach-resonance enhanced interactions in pseudogap and superfluid temperatures. We calculate the spectrum of RF(or laser)-excitations for transitions that transfer atoms out of the superfluid state. The spectrum displays the pairing gap and also the contribution of unpaired atoms, i.e. in-gap excitations. The results support the conclusion that a superfluid, where pairing is a many-body effect, was observed in recent experiments on RF spectroscopy of the pairing gap.

FOS: Physical sciencesRoton01 natural sciences010305 fluids & plasmasSuperfluiditySuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsSuperfluid state0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Physics::Atomic Physics010306 general physicsFeshbach resonanceSpectroscopyCondensed Matter - Statistical MechanicsPhysicsCondensed Matter::Quantum GasesQuantum PhysicsMultidisciplinaryCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsStatistical Mechanics (cond-mat.stat-mech)Strongly Correlated Electrons (cond-mat.str-el)Condensed Matter::OtherCondensed Matter - SuperconductivityPairingPseudogapQuantum Physics (quant-ph)Fermi Gamma-ray Space Telescope
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A radiometric and petrographic interpretation of discrepancies on uranium content in samples collected at Alte Madonie Mounts region (Sicily, Italy)

2013

Abstract The main goal of this work is to evaluate a correlation between anomalous Uranium (U) content and petrographic features of some soil and rock samples collected at Alte Madonie Mounts region (North-central Sicily, Italy). A total of 41 samples of selected soils and rocks were collected, powdered, dried and sealed in “Marinelli” beakers for 20 days before the measurement to ensure that radioactive equilibrium between 226 Ra and 214 Bi was reached. Gamma-ray spectrometric analysis was used to quantify radioactivity concentrations. Mineralogical and chemical features of the samples were determined by X-ray Fluorescence (XRF), X-ray Diffractometry (XRD), Attenuated Total Reflection-Four…

Geological PhenomenaSettore ING-IND/20 - Misure E Strumentazione NucleariHealth Toxicology and MutagenesisAnalytical chemistryMineralogyX-ray fluorescencechemistry.chemical_elementPetrographyRadiation MonitoringSoil Pollutants RadioactiveEnvironmental ChemistryRadiometryWaste Management and DisposalGamma ray spectrometryRadioisotopesSettore GEO/07 - Petrologia E PetrografiaGeneral MedicineUraniumPollutionSpectrometry GammaItalychemistryEnvironmental radioactivity Radiation monitoring Gamma-ray spectrometry X-rayfluorescence X-ray diffractometryEnergy dispersive spectrometrySoil waterUraniumEnvironmental radioactivityEnvironmental scienceRadiometric datingBismuthJournal of Environmental Radioactivity
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ORIGIN: metal creation and evolution from the cosmic dawn

2012

Herder, Jan-Willem den et al.

HOT INTERGALACTIC MEDIUMUNIVERSEChemical evolutionMission7. Clean energy01 natural sciencesSpectral lineSettore FIS/05 - Astronomia E Astrofisica010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NUCLEOSYNTHESISCOSMIC cancer databaseClusters of galaxiesSatellite MissionEpoch (reference date)Astrophysics::Instrumentation and Methods for AstrophysicsFORESTGALAXIESGamma-ray burstsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-ray Mission Gamma-ray bursts Clusters of galaxies Warm-hot intergalactic medium Chemical evolutionWarm-hot intergalactic mediumAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics and AstronomyStructure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Clusters of galaxiemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaREDSHIFTFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray Mission Gamma-ray bursts Clusters of galaxies Warm-hot intergalactic medium Chemical evolutionABSORPTION-SPECTRA010309 opticsX-rayYIELDS0103 physical sciencesGamma-ray burstInstrumentation and Methods for Astrophysics (astro-ph.IM)X-ray; Mission; Gamma-ray bursts; Clusters of galaxies; Warm-hot intergalactic medium; Chemical evolutionAstronomyAstronomy and AstrophysicsRedshiftGalaxyUniverse13. Climate actionChemical evolution; Clusters of galaxies; Gamma-ray bursts; Mission; Warm-hot intergalactic medium; X-ray; Astronomy and Astrophysics; Space and Planetary ScienceSpace and Planetary ScienceGamma-ray burstCLUSTERSExperimental Astronomy
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Search for gamma-ray spectral lines with the DArk Matter Particle Explorer

2021

The DArk Matter Particle Explorer (DAMPE) is well suitable for searching for monochromatic and sharp $\gamma$-ray structures in the GeV$-$TeV range thanks to its unprecedented high energy resolution. In this work, we search for $\gamma$-ray line structures using five years of DAMPE data. To improve the sensitivity, we develop two types of dedicated data sets (including the BgoOnly data which is the first time to be used in the data analysis for the calorimeter-based gamma-ray observatories) and adopt the signal-to-noise ratio optimized regions of interest (ROIs) for different DM density profiles. No line signals or candidates are found between 10 and 300 GeV in the Galaxy. The constraints o…

High Energy Astrophysical Phenomena (astro-ph.HE)Line-like structureHigh Energy Physics - Experiment (hep-ex)MultidisciplinaryAstrophysics::High Energy Astrophysical PhenomenaDAMPE Dark matter Gamma-ray Line-like structureSettore FIS/01 - Fisica SperimentaleDAMPEDark matterFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaGamma-rayHigh Energy Physics - ExperimentScience Bulletin
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A Connection Between Apparent VLBA Jet Speeds and Initial Active Galactic Nucleus Detections Made by the Fermi Gamma-ray Observatory

2009

In its first three months of operations, the Fermi Gamma-Ray Observatory has detected approximately one quarter of the radio-flux-limited MOJAVE sample of bright flat-spectrum active galactic nuclei (AGNs) at energies above 100 MeV. We have investigated the apparent parsec-scale jet speeds of 26 MOJAVE AGNs measured by the Very Long Baseline Array (VLBA) that are in the LAT bright AGN sample (LBAS). We find that the gamma-ray bright quasars have faster jets on average than the non-LBAS quasars, with a median of 15 c, and values ranging up to 34 c. The LBAS AGNs in which the LAT has detected significant gamma-ray flux variability generally have faster jets than the nonvariable ones. These fi…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleus010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Astrophysics of GalaxiesGalaxyLuminositySpace and Planetary ScienceObservatoryAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesBlazarAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsVery Long Baseline ArrayAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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The unusual multiwavelength properties of the gamma-ray source PMN J1603-4904

2013

We investigate the nature and classification of PMNJ1603-4904, a bright radio source close to the Galactic plane, which is associated with one of the brightest hard-spectrum gamma-ray sources detected by Fermi/LAT. It has previously been classified as a low-peaked BL Lac object based on its broadband emission and the absence of optical emission lines. Optical measurements, however, suffer strongly from extinction and the absence of pronounced short-time gamma-ray variability over years of monitoring is unusual for a blazar. We are combining new and archival multiwavelength data in order to reconsider the classification and nature of this unusual gamma-ray source. For the first time, we stud…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrofísicaActive galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Very-long-baseline interferometryAstronomiaSpectral energy distributionAstrophysics - High Energy Astrophysical PhenomenaBlazarAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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X-RAY AND OPTICAL OBSERVATIONS OF A 0535+26

2011

We present recent contemporaneous X-ray and optical observations of the Be/X-ray binary system A\,0535+26 with the \textit{Fermi}/Gamma-ray Burst Monitor (GBM) and several ground-based observatories. These new observations are put into the context of the rich historical data (since $\sim$1978) and discussed in terms of the neutron star Be-disk interaction. The Be circumstellar disk was exceptionally large just before the 2009 December giant outburst, which may explain the origin of the unusual recent X-ray activity of this source. We found a peculiar evolution of the pulse profile during this giant outburst, with the two main components evolving in opposite ways with energy. A hard 30-70 mH…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsBrightnessOscillationAstrophysics::High Energy Astrophysical PhenomenaX-rayFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)AstrophysicsNeutron starSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsGeneral patternAstrophysics - High Energy Astrophysical PhenomenaLine (formation)Fermi Gamma-ray Space TelescopeThe Astrophysical Journal
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A new population of terrestrial gamma‐ray flashes in the RHESSI data

2015

Terrestrial gamma-ray flashes (TGFs) are the most energetic photon phenomenon occurring naturally on Earth. An outstanding question is as follows: Are these flashes just a rare exotic phenomenon or are they an intrinsic part of lightning discharges and therefore occurring more frequently than previously thought? All measurements of TGFs so far have been limited by the dynamic range and sensitivity of spaceborne instruments. In this paper we show that there is a new population of weak TGFs that has not been identified by search algorithms. We use the World Wide Lightning Location Network (WWLLN) to identify lightning that occurred in 2006 and 2012 within the 800 km field of view of Reuven Ra…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh energyGamma rayFOS: Physical sciencesAstronomyterrestrial gamma-ray flashesWorld wideLightningNew populationSpace Physics (physics.space-ph)GeophysicsPhysics - Space PhysicsGeneral Earth and Planetary Sciences:Matematikk og Naturvitenskap: 400 [VDP]Astrophysics - High Energy Astrophysical Phenomenalightningfluence distributionsProduction rateGeophysical Research Letters
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Enhanced detection of terrestrial gamma-ray flashes by AGILE

2015

Abstract At the end of March 2015 the onboard software configuration of the Astrorivelatore Gamma a Immagini Leggero (AGILE) satellite was modified in order to disable the veto signal of the anticoincidence shield for the minicalorimeter instrument. The motivation for such a change was the understanding that the dead time induced by the anticoincidence prevented the detection of a large fraction of Terrestrial Gamma‐Ray Flashes (TGFs). The configuration change was highly successful resulting in an increase of one order of magnitude in TGF detection rate. As expected, the largest fraction of the new events has short duration (<100 μs), and part of them has simultaneous association with light…

High Energy Astrophysical Phenomena (astro-ph.HE)Solar Physics Astrophysics and AstronomyAtmospheric ScienceFOS: Physical sciencesterrestrial gamma-ray flashesterrestrial gamma‐ray flashesatmospheric electricity; terrestrial gamma-ray flashesTGFSpace Physics (physics.space-ph)LightningResearch Lettersatmospheric electricityPhysics - Space PhysicsAtmospheric ProcessesResearch Letter:Matematikk og Naturvitenskap: 400 [VDP]Instruments and TechniquesAGILE TGFAstrophysics - High Energy Astrophysical Phenomena
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Universal transport dynamics in a quenched tunnel-coupled Luttinger liquid

2016

The transport dynamics of a quenched Luttinger liquid tunnel-coupled to a fermionic reservoir is investigated. In the transient dynamics, we show that for a sudden quench of the electron interaction universal power-law decay in time of the tunneling current occurs, ascribed to the presence of entangled compound excitations created by the quench. In sharp contrast to the usual non universal power-law behavior of a zero-temperature non-quenched Luttinger liquid, the steady state tunneling current is ohmic and can be explained in terms of an effective quench-activated heating of the system. Our study unveils an unconventional dynamics for a quenched Luttinger liquid that could be identified in…

High Energy Physics::LatticeElectron interactionFOS: Physical sciences01 natural sciences010305 fluids & plasmasCondensed Matter Physics; Electronic Optical and Magnetic MaterialsCondensed Matter - Strongly Correlated ElectronsLuttinger liquid0103 physical sciencesElectronicOptical and Magnetic MaterialsTunneling current010306 general physicsOhmic contactElectronic Optical and Magnetic Materials; Condensed Matter PhysicsPhysicsCondensed Matter::Quantum GasesCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Transport dynamicsCondensed Matter PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall EffectQuantum Gases (cond-mat.quant-gas)Condensed Matter::Strongly Correlated ElectronsTransient (oscillation)Condensed Matter - Quantum GasesFermi Gamma-ray Space Telescope
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