Search results for "Fermi Gamma-ray Space Telescope"

showing 10 items of 108 documents

Single molecules probe local density of modes (LDOS) around photonic nanostructures

2008

International audience; According to Fermi's golden rule, the fluorescence decay rate is directly proportional to the projected local density of photonic modes (LDOS) at the molecule location. The relevant LDOS depends on the molecule orientation. In this paper, the direct measurement of the fluorescence lifetime near gold dot photonic structures is investigated and compared to calculated LDOS. Detailed analysis of the decay channels is presented on the basis of numerical simulations.

HistologyNanostructureFLUORESCENCE LIFETIME[SPI.NANO] Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsPhysics::Optics02 engineering and technology01 natural sciencesPathology and Forensic MedicineELECTROMAGNETIC SCATTERINGMEDIACondensed Matter::Superconductivity0103 physical sciencesMolecule[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics010306 general physicsChemistrybusiness.industry021001 nanoscience & nanotechnologyCondensed Matter::Mesoscopic Systems and Quantum Hall EffectFluorescenceSPONTANEOUS-EMISSION[ SPI.NANO ] Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsPhotonicsAtomic physics0210 nano-technologybusinessFermi Gamma-ray Space Telescope
researchProduct

Conservative upper limits on WIMP annihilation cross section from Fermi-LAT $γ$-rays

2011

The spectrum of an isotropic extragalactic {\gamma}-ray background (EGB) has been measured by the Fermi-LAT telescope at high latitudes. Two new models for the EGB are derived from the subraction of unresolved point sources and extragalactic diffuse processes, which could explain from 30% to 70% of the Fermi-LAT EGB. Within the hypothesis that the two residual EGBs are entirely due to the annihilation of dark matter (DM) particles in the Galactic halo, we obtain stringent upper limits on their annihilation cross section. Severe bounds on a possible Sommerfeld enhancement of the annihilation cross section are set as well. Finally, we consider models for DM annihilation depending on the inver…

HistoryAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesEducationlaw.inventionGalactic haloTelescopeCross section (physics)WIMPlaw0103 physical sciences010306 general physicsAstrophysics::Galaxy AstrophysicsPhysicsastro-ph.HEAnnihilation010308 nuclear & particles physicsIsotropyhep-phComputer Science ApplicationsHigh Energy Physics - PhenomenologyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space Telescope
researchProduct

Nuclear medium modification of the structure function

2011

Abstract We study the nuclear effects in the electromagnetic structure function F 2 ( x , Q 2 ) in the deep inelastic lepton–nucleus scattering process by taking into account Fermi motion, binding, pion and rho meson cloud contributions. Calculations have been done in a local density approximation using relativistic nuclear spectral functions which include nucleon correlations. The ratios R F 2 A ( x , Q 2 ) = 2 F 2 A ( x , Q 2 ) A F 2 D ( x , Q 2 ) are obtained and compared with recent JLab results for light nuclei with special attention to the slope of the x distributions. This magnitude shows a non-trivial A dependence and it is insensitive to possible normalization uncertainties. The re…

Normalization (statistics)PhysicsNuclear and High Energy PhysicsRho meson010308 nuclear & particles physicsNuclear TheoryMagnitude (mathematics)Deep inelastic scattering7. Clean energy01 natural sciencesNuclear physicsPion0103 physical sciencesLocal-density approximationAtomic physicsNuclear Experiment010306 general physicsNucleonFermi Gamma-ray Space TelescopeNuclear Physics A
researchProduct

Nonlocalities and Fermi motion corrections in K- atoms

2002

We evaluate the p-wave $K^-N$ amplitudes from the chiral Lagrangians and from there construct the p-wave part of the $K^-$ nucleus optical potential plus a small s-wave part induced from the elementary p-wave amplitude and the nuclear Fermi motion. Simultaneously, the momentum and energy dependence of the s-wave optical potential, previously developed, are taken into account and shown to generate a small p-wave correction to the optical potential. All the corrections considered are small compared to the leading s-wave potential, and lead to changes in the shifts and widths which are smaller than the experimental errors. A thorough study of the threshold region and low densities is conducted…

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsAmplitudeNuclear TheoryQuantum electrodynamicsFOS: Physical sciencesMotion (geometry)FísicaEnergy–momentum relationOptical potentialFermi Gamma-ray Space Telescope
researchProduct

Photoproduction of the hypertriton

1997

In the framework of the impulse approximation we study the photoproduction of the hypertriton $^3_{\Lambda}$H by using realistic $^3$He wave functions obtained as solutions of Faddeev equations with the Reid soft-core potential for different $^3_{\Lambda}$H wave functions. We obtain relatively small cross sections of the order of 1 nb. We also find that the influence of Fermi motion is important, while the effect of different off-shell assumptions on the cross section is not too significant.

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsFaddeev equationsParticle physicsNuclear TheoryNuclear TheoryFOS: Physical sciencesImpulse (physics)Wave functionLambdaHypertritonFermi Gamma-ray Space TelescopeNuclear Physics A
researchProduct

Shell-model calculation of isospin-symmetry breaking correction to superallowed Fermi beta-decay

2016

We investigate the radial-overlap part of the isospin-symmetry breaking correction to superallowed $0^+\to 0^+$-decay using the shell-model approach similar to that of Refs. [1, 2]. The 8 sd-shell emitters with masses between $A=22$ and $A=38$ have been re-examined. The Fermi matrix element is evaluated with realistic spherical single-particle wave functions, obtained from spherical Woods-Saxon (WS) or Hartree-Fock (HF) potentials, fine-tuned to reproduce the experimental data on charge radii and separation energies for nuclei of interest. The elaborated adjustment procedure removes any sensitivity of the correction to a specific parametrisation of the WS potential or to various versions of…

Nuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]SHELL modelNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences23.40.-sNuclear physicsNuclear Theory (nucl-th)21.60.Cs0103 physical sciences21.10.PcSensitivity (control systems)Symmetry breakingWave function010303 astronomy & astrophysics[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]Physicsta114010308 nuclear & particles physicsCharge (physics)Beta decay21.10.JxIsospinQuantum electrodynamics23.40.Bwbeta decayisospin-symmetry breakingFermi Gamma-ray Space Telescope
researchProduct

Ultrafast Dynamics of Magnetic Domain Structures Probed by Coherent Free-Electron Laser Light

2013

Synchrotron radiation news 26(6), 27 - 32 (2013). doi:10.1080/08940886.2013.850384

Nuclear and High Energy PhysicsMagnetic domainMagnetismAstrophysics::High Energy Astrophysical Phenomena02 engineering and technology53001 natural scienceslaw.inventionOpticslaw0103 physical sciencesddc:530010306 general physicsComputingMilieux_MISCELLANEOUSPhysicsMagnetic circular dichroismbusiness.industryScatteringFree-electron laser021001 nanoscience & nanotechnologyLaserAtomic and Molecular Physics and Optics[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Physics::Accelerator PhysicsAtomic physics0210 nano-technologybusinessUltrashort pulseFermi Gamma-ray Space TelescopeSynchrotron Radiation News
researchProduct

Landau parameters for energy density functionals generated by local finite-range pseudopotentials

2017

In Landau theory of Fermi liquids, the particle-hole interaction near the Fermi energy in different spin-isospin channels is probed in terms of an expansion over the Legendre polynomials. This provides a useful and efficient way to constrain properties of nuclear energy density functionals in symmetric nuclear matter and finite nuclei. In this study, we present general expressions for Landau parameters corresponding to a two-body central local regularized pseudopotential. We also show results obtained for two recently adjusted NLO and N$^2$LO parametrizations. Such pseudopotentials will be used to determine mean-field and beyond-mean-field properties of paired nuclei across the entire nucle…

Nuclear and High Energy PhysicsNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]HARTREE-FOCK CALCULATIONSNuclear Theoryregularized pseudopotentialsFOS: Physical sciencesFinite range114 Physical sciences7. Clean energy01 natural sciencesenergy density functionalsNuclear Theory (nucl-th)PseudopotentialLandau parametersQuantum mechanics0103 physical sciencesNuclear Experiment010306 general physicsLegendre polynomialsNUCLEAR-MATTERPhysics010308 nuclear & particles physicsFermi energyNuclear matterLandau theoryEnergy densityFermi Gamma-ray Space TelescopeJournal of Physics G: Nuclear and Particle Physics
researchProduct

A search for time dependent neutrino emission from microquasars with the ANTARES telescope

2014

[EN] Results are presented on a search for neutrino emission from a sample of six microquasars, based on the data collected by the ANTARES neutrino telescope between 2007 and 2010. By means of appropriate time cuts, the neutrino search has been restricted to the periods when the acceleration of relativistic jets was taking place at the microquasars under study. The time cuts have been chosen using the information from the X-ray telescopes RXTE/ASM and Swift/BAT, and, in one case, the gamma-ray telescope Fermi/LAT. No statistically significant excess has been observed, thus upper limits on the neutrino fluences have been derived and compared to the predictions by models. Constraints have bee…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyLuminositylaw.inventionTelescopeneutrinoAstrophysical jetlawMicroquasars0103 physical sciencesmicroquasarNeutrinos010303 astronomy & astrophysicsAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyFísicaAstronomy and AstrophysicsSolar neutrino problemNeutrino detectorSpace and Planetary ScienceFISICA APLICADANuclear and High Energy Physics; Astronomy and Astrophysics; Space and Planetary ScienceHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaANTARES neutrino telescopeFermi Gamma-ray Space Telescope
researchProduct

T- and P-asymmetries in the (γ, π−) reaction on 13C and 15N

1995

Abstract A simultaneous theoretical analysis of the polarization observables for negative pion photoproduction off the 13 C and 15 N nuclei is performed. A sensitivity of the target and recoil asymmetries to different ingredients of the theory (the Fermi motion, the final state interaction and the nuclear model input) is investigated. The importance of the high (2 hω ) configurations in the nuclea ground states is shown.

Nuclear physicsPhysicsNuclear and High Energy PhysicsRecoilPionNuclear TheoryPolarization observablesState (functional analysis)Atomic physicsNuclear ExperimentFermi Gamma-ray Space TelescopeNuclear Physics A
researchProduct