Search results for "Space telescope"

showing 10 items of 123 documents

A note on the computation of geometrically defined relative velocities

2011

We discuss some aspects about the computation of kinematic, spectroscopic, Fermi and astrometric relative velocities that are geometrically defined in general relativity. Mainly, we state that kinematic and spectroscopic relative velocities only depend on the 4-velocities of the observer and the test particle, unlike Fermi and astrometric relative velocities, that also depend on the acceleration of the observer and the corresponding relative position of the test particle, but only at the event of observation and not around it, as it would be deduced, in principle, from the definition of these velocities. Finally, we propose an open problem in general relativity that consists on finding intr…

PhysicsMathematics - Differential GeometryPhysics and Astronomy (miscellaneous)General relativityComputationOpen problemRelative velocityFOS: Physical sciences83C99 53B30Observer (special relativity)KinematicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyClassical mechanicsDifferential Geometry (math.DG)FOS: MathematicsTest particleAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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Competition between Allowed and First-Forbidden β Decay: The Case of Hg208→Tl208

2020

The β decay of ^{208}Hg into the one-proton hole, one neutron-particle _{81}^{208}Tl_{127} nucleus was investigated at CERN-ISOLDE. Shell-model calculations describe well the level scheme deduced, validating the proton-neutron interactions used, with implications for the whole of the N>126, Z<82 quadrant of neutron-rich nuclei. While both negative and positive parity states with spin 0 and 1 are expected within the Q_{β} window, only three negative parity states are populated directly in the β decay. The data provide a unique test of the competition between allowed Gamow-Teller and Fermi, and first-forbidden β decays, essential for the understanding of the nucleosynthesis of heavy nuclei in…

PhysicsNuclear TheoryGeneral Physics and AstronomyParity (physics)01 natural sciences7. Clean energyNeutron capturemedicine.anatomical_structureNucleosynthesisExcited state0103 physical sciencesmedicineNeutronAtomic physicsNuclear Experiment010306 general physicsNucleusFermi Gamma-ray Space TelescopePhysical Review Letters
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Production of excited double hypernuclei via Fermi breakup of excited strange systems

2011

Precise spectroscopy of multi-strange hypernuclei provides a unique chance to explore the hyperon-hyperon interaction. In the present work we explore the production of excited states in double hypernuclei following the micro-canonical break-up of an initially excited double hypernucleus which is created by the absorption and conversion of a stopped $\Xi^{-}$ hyperon. Rather independent on the spectrum of possible excited states in the produced double hypernuclei the formation of excited states dominates in our model. For different initial target nuclei which absorb the $\Xi^-$, different double hypernuclei nuclei dominate. Thus the ability to assign the various observable $\gamma$-transitio…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsNuclear TheoryHyperonFOS: Physical sciencesObservableHypernucleus01 natural sciencesSpectral lineNuclear physicsPionExcited state0103 physical sciencesNuclear Experiment (nucl-ex)Atomic physics010306 general physicsSpectroscopyNuclear ExperimentNuclear ExperimentFermi Gamma-ray Space Telescope
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Electromagnetic Production of the Hypertriton

1996

Kaon photoproduction on He3, gamma + He3 --&gt; K+ + Hypertriton, is studied in the framework of the impulse approximation. Realistic He3 wave functions obtained as solutions of Faddeev equations with the Reid soft-core potential are used along with different Hypertriton wave functions. Results are compared for several elementary operator models, which can successfully describe the elementary kaon production off the proton up to a photon lab energy of k = 2.2 GeV. It is found that the corresponding cross sections are small, of the order of several nanobarns. It is also shown that the influence of Fermi motion is important, while the effect of different off-shell assumptions on the cross sec…

PhysicsNuclear and High Energy PhysicsFaddeev equationsPhotonNuclear TheoryNuclear TheoryFOS: Physical sciencesImpulse (physics)Nuclear physicsNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Atomic and Molecular ClustersWave functionNuclear ExperimentHypertritonFermi Gamma-ray Space Telescope
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Microscopic quasiparticle-phonon description of odd-mass127−133Xeisotopes and their β decay

1998

Quasiparticle-phonon equations of motion are solved starting from a microscopic realistic many-body Hamiltonian. In this microscopic quasiparticle-phonon model (MQPM) the relevant part of the three-quasiparticle Hilbert space may possibly be taken into account even in calculations using large single-particle bases. As an example, the MQPM is applied to the calculation of energy levels and Fermi and Gamow-Teller beta-decay transition amplitudes for transitions between odd-mass ${}^{127\ensuremath{-}133}\mathrm{Xe}$, ${}^{127\ensuremath{-}133}\mathrm{I}$, and ${}^{127\ensuremath{-}133}\mathrm{Cs}$ isotopes. Considering the fully microscopic nature of the MQPM, comparison of its results and da…

PhysicsNuclear and High Energy PhysicsIsotopePhononHilbert spaceEquations of motionsymbols.namesakeAmplitudeQuantum mechanicsQuasiparticlesymbolsCondensed Matter::Strongly Correlated ElectronsAtomic physicsHamiltonian (quantum mechanics)Fermi Gamma-ray Space TelescopePhysical Review C
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Theoretical study of incoherent phi photoproduction on a deuteron target

2012

We study the photoproduction of phi mesons in deuteron, paying attention to the modification of the cross section from bound protons to the free ones with the aim of comparing with recent results at LEPS. For this purpose we take into account Fermi motion in single scattering and rescattering of the phi to account for phi absorption on a second nucleon as well as the rescattering of the proton. We find that the contribution of the double scattering is much smaller than the typical cross section of gamma p to phi p in free space, which implies a very small screening of the phi production in deuteron. The contribution from the proton rescattering, on the other hand, is found to be not negligi…

PhysicsNuclear and High Energy PhysicsMesonProtonNuclear Theory010308 nuclear & particles physicsScatteringNuclear TheoryFísicaFOS: Physical sciences01 natural sciences7. Clean energyNuclear physicsMomentumNuclear Theory (nucl-th)Cross section (physics)Phase space0103 physical sciences010306 general physicsNucleonNuclear ExperimentFermi Gamma-ray Space Telescope
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Conservative upper limits on WIMP annihilation cross section from Fermi-LAT γ rays

2012

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…

PhysicsNuclear and High Energy PhysicsParticle physicsAnnihilationdark matter theoryAstrophysics::High Energy Astrophysical PhenomenaDark matterGamma raysGamma rayAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalactic haloGamma rays; dark matter theoryPulsarWIMPHaloAstrophysics::Galaxy AstrophysicsFermi Gamma-ray Space Telescope
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Scalar isoscalar pion pairs in nuclei and theA(π,ππ)Xreaction

1999

The reaction A(pi,pi pi)X has been studied at low energies, paying particular attention to the interaction of the two final pions in the scalar isoscalar (I=J=0) channel. We have developed a microscopic model for the pion production, and then implemented the two pion final state interaction by using the results of a non-perturbative unitary coupled-channels method based in the standard chiral Lagrangians. The resulting model, describes well the reaction on the nucleon for all different isospin channels. Finally, we have considered the reaction in nuclei. Our calculation takes into account Fermi motion, Pauli blocking, pion absorption, and also the strong modification of the pi-pi interactio…

PhysicsNuclear and High Energy PhysicsParticle physicsIsoscalarNuclear TheoryScalar (mathematics)Nuclear physicssymbols.namesakePauli exclusion principlePionDeuteriumIsospinsymbolsNuclear ExperimentNucleonFermi Gamma-ray Space TelescopePhysical Review C
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Quasielastic neutrino (antineutrino) reactions in nuclei and the axial-vector form factor of the nucleon

1992

Abstract Quasielastic neutrino and antineutrino reactions in nuclei are studied to investigate the effect of the nuclear medium on the determination of axial dipole mass M A in nuclei. The calculations are done in the local density approximation and various nuclear effects like Pauli blocking, Fermi motion of nucleons and strong renormalization effects in the spin-isospin channel are taken into account. The nuclear effects are found to be quite large at low q 2 , but the data in this region are too meagre to influence the determination of M A . The experimental data on differential and total cross sections are found to be consistent with M A as determined from deuterium experiments and no c…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryForm factor (quantum field theory)Nuclear physicsDipolesymbols.namesakePauli exclusion principleDeuteriumsymbolsNeutrinoNuclear ExperimentNucleonPseudovectorFermi Gamma-ray Space TelescopeNuclear Physics A
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Mesonic and binding contributions to the EMC effect in a relativistic many-body approach

1996

We revise the conventional nuclear effects of Fermi motion, binding and pionic effects in deep inelastic lepton scattering using a relativistic formalism for an interacting Fermi sea and the local density approximation to translate results from nuclear matter to finite nuclei. In addition we also consider effects from rho-meson renormalization in the nucleus. The use of nucleon Green's functions in terms of their spectral functions offers a precise way to account for Fermi motion and binding. On the other hand the use of many body Feynman diagrams in a relativistic framework allows one to avoid using prescriptions given in the past to introduce relativistic corrections in a non relativistic…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryMesonHigh Energy Physics::PhenomenologyEMC effectNuclear TheoryFOS: Physical sciencesFísicaNuclear matterNuclear Theory (nucl-th)RenormalizationHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)symbolsFeynman diagramNucleonNuclear ExperimentFermi Gamma-ray Space TelescopeLepton
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