Search results for "Space telescope"

showing 10 items of 123 documents

Antihyperon potentials in nuclei via exclusive antiproton–nucleus reactions

2015

Abstract The exclusive production of hyperon–antihyperon pairs close to their production threshold in p ‾ -nucleus collisions offers a unique and hitherto unexplored opportunity to elucidate the behavior of antihyperons in nuclei. For the first time we analyze these reactions in a microscopic transport model using the Giesen Boltzmann–Uehling–Uhlenbeck transport model. The calculation takes the delicate interplay between the strong absorption of antihyperons, their rescattering and mean field deflection as well as the Fermi motion of the struck nucleon into account. We find a substantial sensitivity of transverse momentum correlations of coincident Λ ‾ Λ -pairs to the assumed depth of the Λ…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear Theorylcsh:QC1-999IonNuclear physicsmedicine.anatomical_structureDeflection (physics)Mean field theoryAntiprotonmedicineFacility for Antiproton and Ion ResearchNuclear ExperimentNucleonNucleuslcsh:PhysicsFermi Gamma-ray Space TelescopePhysics Letters B
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Relativistic direct Urca processes in cooling neutron stars

2001

We derive a relativistic expression for neutrino energy losses caused by the direct Urca processes in degenerate baryon matter of neutron stars. We use two different ways to calculate the emissivity caused by the reactions to our interest. First we perform a standard calculation by Fermi's ''golden'' rule. The second calculation, resulting in the same expression, is performed with the aid of polarization functions of the medium. Our result for neutrino energy losses strongly differs from previous non-relativistic results. We also discuss nonconservation of the baryon vector current in reactions through weak charged currents in the medium, when the asymmetry between protons and neutrons is c…

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear Theorymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Degenerate energy levelsNuclear TheoryFOS: Physical sciencesFísicaAstrophysicsPolarization (waves)AsymmetryNuclear Theory (nucl-th)BaryonHigh Energy Physics - PhenomenologyNeutron starHigh Energy Physics - Phenomenology (hep-ph)NeutronNeutrinoNuclear Experimentmedia_commonFermi Gamma-ray Space Telescope
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Nuclear medium effects inν(ν¯)-nucleus deep inelastic scattering

2011

We study nuclear medium effects in the weak structure functions ${F}_{2}(x,{Q}^{2})$ and ${F}_{3}(x,{Q}^{2})$ in the deep inelastic neutrino and antineutrino induced reactions in nuclei. We use a theoretical model for the nuclear spectral functions which incorporates the conventional nuclear effects, such as Fermi motion, binding, and nucleon correlations. We also consider the pion and rho meson cloud contributions calculated from a microscopic model for meson-nucleus self-energies. The calculations have been performed using relativistic nuclear spectral functions. Our results are compared with the experimental data of the NuTeV and the CERN Dortmund Heidelberg Saclay Warsaw (CDHSW) collabo…

PhysicsNuclear and High Energy PhysicsParticle physicsRho mesonLarge Hadron Collider010308 nuclear & particles physicsNuclear TheoryDeep inelastic scattering01 natural sciences7. Clean energyNuclear physicsPionDeuterium0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoNuclear Experiment010306 general physicsNucleonFermi Gamma-ray Space TelescopePhysical Review C
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Extended Thomas - Fermi expansion from nuclear linear response

1996

The coefficients of the successive orders of the extended Thomas - Fermi expansion of the kinetic energy density are obtained to the leading order in the density inhomogeneities. This is done by comparing the corresponding static polarizability with the exact value in two cases: a non-interacting nuclear infinite system and symmetric nuclear matter with a Skyrme interaction.

PhysicsNuclear and High Energy PhysicsPolarizabilityQuantum electrodynamicsQuantum mechanicsNuclear TheoryOrder (group theory)Kinetic energyFermi gasNuclear matterFermi Gamma-ray Space TelescopeJournal of Physics G: Nuclear and Particle Physics
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Multiparticle emission in the decay ofAr31

2014

A multihit capacity setup was used to study the decay of the dripline nucleus Ar-31, produced at the ISOLDE facility at CERN. A spectroscopic analysis of the beta-delayed three-proton decay of Ar-31 is presented for the first time together with a quantitative analysis of the beta-delayed 2p gamma decay. A new method for determination of the spin of low-lying levels in the beta p daughter 30S using proton-proton angular correlations is presented and used to determine that the spin of the 5.2-MeV level is most likely 3(+) with 4(+) also possible. The half-life of Ar-31 is found to be 15.1(3) ms. An improved analysis of the Fermi beta strength including the beta 3p-decay mode gives a total mea…

PhysicsNuclear and High Energy PhysicsProton010308 nuclear & particles physicsBranching fractionGamma ray7. Clean energy01 natural sciencesNuclear physicsmedicine.anatomical_structure0103 physical sciencesmedicineIsobaric processBeta (velocity)Atomic physics010306 general physicsNucleusSpin-½Fermi Gamma-ray Space TelescopePhysical Review C
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Recoil-beta tagging: A novel technique for studying proton-drip-line nuclei

2006

Abstract Tagging with charged particles and γ -rays at the focal plane of recoil separators has proven, over the last two decades, to be a very powerful tool for the identification of excited states in exotic nuclei produced with very low cross-sections. One of the key areas so far unexplored in terms of the tagging methodology has been performing correlations with β -particles at the focal plane of a recoil separator. A new technique entitled Recoil-Beta Tagging (RBT) has been developed, this technique exploits the unusual properties of Fermi super-allowed β emitters, which have both a short half-life ( ∼ 100 ms ) and high β + -endpoint energy. Correlating with such β -particles using a do…

PhysicsNuclear and High Energy PhysicsProton010308 nuclear & particles physicsDetector[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesCharged particleSemiconductor detectorNuclear physicsRecoilPositronExcited state27.50.þe; 29.30.Kv; 29.40.Wk0103 physical sciencesAtomic physics010306 general physicsNuclear ExperimentInstrumentationFermi Gamma-ray Space Telescope
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THE UFFO SLEWING MIRROR TELESCOPE FOR EARLY OPTICAL OBSERVATION FROM GAMMA RAY BURSTS

2013

While some space born observatories, such as SWIFT and FERMI, have been operating, early observation of optical after grow of GRBs is still remained as an unexplored region. The Ultra-Fast Flash Observatory (UFFO) project is a space observatory for optical follow-ups of GRBs, aiming to explore the first 60 seconds of GRBs optical emission. Using fast moving mirrors to redirect our optical path rather than slewing the entire spacecraft, UFFO is utilized to catch early optical emissions from GRB within 1 sec. We have developed the UFFO Pathfinder Telescope which is going to be on board of the Lomonosov satellite and launched in middle of 2012. We will discuss about scientific potentials of t…

PhysicsNuclear and High Energy PhysicsSpacecraftbusiness.industryPayloadAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsGeneral Physics and AstronomyAstronomyAstronomy and AstrophysicsAstrophysicslaw.inventionTelescopeOptical pathlawObservatorySatelliteGamma-ray burstbusinessFermi Gamma-ray Space TelescopeModern Physics Letters A
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Tz=−1→0βdecays ofNi54,Fe50,Cr46, andTi42and comparison with mirror(He3,t)measurements

2015

We have studied the β decay of the Tz=−1, f7/2 shell nuclei Ni54, Fe50, Cr46, and Ti42 produced in fragmentation reactions. The proton separation energies in the daughter Tz=0 nuclei are relatively large (≈4–5 MeV) so studies of the γ rays are essential. The experiments were performed at GSI as part of the Stopped-beam campaign with the RISING setup consisting of 15 Euroball Cluster Ge detectors. From the newly obtained high precision β-decay half-lives, excitation energies, and β branching ratios, we were able to extract Fermi and Gamow-Teller transition strengths in these β decays. With these improved results it was possible to compare in detail the Gamow-Teller (GT) transition strengths …

PhysicsNuclear physicsNuclear and High Energy PhysicsFragmentation (mass spectrometry)High resolutionGamma spectroscopySensitivity limitAtomic physicsBeta decayExcitationCharge exchangeFermi Gamma-ray Space TelescopePhysical Review C
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Corrections for positon annihilation in flight in nuclear spectrometry

1973

Abstract Theories of positon single- and two-quanta annihilation in flight, the Fermi beta-decay theory, and theories of positon energy loss are used in calculations of total probabilities of annihilation in flight of positons in continuous spectra. The results are given in a nomogram useful in correcting for positon annihilation in flight in various nuclear-spectrometry experiments. Confirmation of the theoretical basis employed was obtained by comparing total absolute probabilities for annihilation in flight of 62 Cu positons in Perspex, copper, cadmium and lead, using a new differential method. The agreement with the theory was found to be excellent. A method for obtaining “correct” posi…

PhysicsNuclear physicsScintillationNonlinear Sciences::Exactly Solvable and Integrable SystemsAnnihilationContinuous spectrumGamma spectroscopyGeneral MedicineAtomic physicsSpectroscopySpectral lineSemiconductor detectorFermi Gamma-ray Space TelescopeNuclear Instruments and Methods
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Microscopic calculations of isospin-breaking corrections to superallowed beta-decay

2011

The superallowed beta-decay rates that provide stringent constraints on physics beyond the Standard Model of particle physics are affected by nuclear structure effects through isospin-breaking corrections. The self-consistent isospin- and angular-momentum-projected nuclear density functional theory is used for the first time to compute those corrections for a number of Fermi transitions in nuclei from A=10 to A=74. The resulting leading element of the CKM matrix, |V_{ud}|= 0.97447(23), agrees well with the recent result by Towner and Hardy [Phys. Rev. C {\bf 77}, 025501 (2008)].

PhysicsParticle physicsNuclear Theoryta114Physics beyond the Standard ModelHigh Energy Physics::PhenomenologyNuclear TheoryNuclear structureGeneral Physics and AstronomyFOS: Physical sciencesNuclear matterBeta decayNuclear physicsNuclear Theory (nucl-th)Standard Model (mathematical formulation)IsospinNuclear ExperimentNuclear densityFermi Gamma-ray Space Telescope
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