Search results for "Nuclear Reactions"

showing 10 items of 57 documents

Hypernuclear spectroscopy of products from Li-6 projectiles on a carbon target at 2 A GeV

2013

WOS: 000322848900009

Nuclear reaction(Li-6E=2 GeV/nucleonNuclear and High Energy PhysicsMaximum likelihoodWEAK DECAYFOS: Physical sciencesLIFETIMET-1/2. Compared with other datadeduced Lambda massC-12(LAMBDA)H-4)T-1/2measured Lambda H-3H-4 Lambda-hypernuclei invariant mass distribution T-1/2measured LambdaInvariant massNuclear Experiment (nucl-ex)LIGHT HYPERFRAGMENTSSpectroscopyNuclear ExperimentX)PhysicsH-4 Lambda-hypernuclei invariant mass distributionH-3ProjectileSignificance valueslifetime measurementdeduced Lambda mass H-3H-4 Lambda-hypernuclei mass T-1/2. Compared with other data lifetime measurementNUCLEAR REACTIONS C(Li-6Decay timeLAMBDA-HYPERNUCLEIAtomic physicst)NUCLEAR REACTIONS C(Li-6 X) (Li-6 t) (Li-6 H-4) E=2 GeV/nucleonH-4 Lambda-hypernuclei massHypertritonRELATIVISTIC HYPERNUCLEINuclear Physics A
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The Nuclear astrophysics program at n_TOF (CERN)

2017

An important experimental program on Nuclear Astrophysics is being carried out at the n_TOF since several years, in order to address the still open issues in stellar and primordial nucleosynthesis. Several neutron capture reactions relevant to s-process nucleosynthesis have been measured so far, some of which on important branching point radioisotopes. Furthermore, the construction of a second experimental area has recently opened the way to challenging measurements of (n, charged particle) reactions on isotopes of short half-life. The Nuclear Astrophysics program of the n_TOF Collaboration is here described, with emphasis on recent results relevant for stellar nucleosynthesis, stellar neut…

Nuclear reactionAstrofísicaAstrophysics and AstronomyCross-sectionnTOFQC1-999Astrophysics::High Energy Astrophysical PhenomenaNeutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Astrophysics01 natural sciences7. Clean energyn_TOF nuclear astrophysics CERNNuclear physicsPhysics and Astronomy (all)Stellar nucleosynthesisBig Bang nucleosynthesisNucleosynthesis0103 physical sciencesCERNNuclear astrophysicsAstrophysics::Solar and Stellar AstrophysicsNuclear Physics - ExperimentNeutronNeutron induced nuclear reactions010306 general physicsNuclear ExperimentAstrophysics::Galaxy AstrophysicsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Neutrons:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear reactionNeutron capture13. Climate actionNeutron sourceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]NucleosynthesisNucleosíntesi
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Spatially resolved X-ray study of supernova remnants that host magnetars: Implication of their fossil field origin

2019

Magnetars are regarded as the most magnetized neutron stars in the Universe. Aiming to unveil what kinds of stars and supernovae can create magnetars, we have performed a state-of-the-art spatially resolved spectroscopic X-ray study of the supernova remnants (SNRs) Kes 73, RCW 103, and N49, which host magnetars 1E 1841-045, 1E 161348-5055, and SGR 0526-66, respectively. The three SNRs are O- and Ne-enhanced and are evolving in the interstellar medium with densities of >1--2 cm$^{-3}$. The metal composition and dense environment indicate that the progenitor stars are not very massive. The progenitor masses of the three magnetars are constrained to be < 20 Msun (11--15 Msun for Kes 73, …

Nuclear reactionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsMagnetar7. Clean energy01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarNucleosynthesispulsars: general0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)ISM: supernova remnantPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsInterstellar mediumNeutron starSupernovaStarsAstrophysics - Solar and Stellar Astrophysicsnuclear reactions nucleosynthesis abundance13. Climate actionSpace and Planetary Sciencestars: magnetarAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Editorial: The Future of Nuclear Structure: Challenges and Opportunities in the Microscopic Description of Nuclei

2021

The past two decades have witnessed tremendous progress in the microscopic description of atomic nuclei. The Topical Review `The Future of Nuclear Structure' aims at summarizing the current state-of-the-art microscopic calculations in Nuclear Theory and to give a useful reference for young researches who wish to learn more about this exciting discipline.

Nuclear reactionMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Physics and AstronomyMicroscopic descriptionnuclear reactionNuclear Theory (nucl-th)Theoretical physicsnuclear theoryeffective field theorieseffective field theoriemany-body physicsPhysical and Theoretical ChemistryNuclear theorynuclear reactionsMathematical PhysicsPhysicsAb initio (calculations)Nuclear structurelcsh:QC1-999Topical reviewmany-body physicAtomic nucleusnuclear structurelcsh:Physics
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Proton emission off nuclei induced by kaons in flight

2010

We study the (K-, p) reaction on nuclei with a 1 GeV/c momentum kaon beam, paying special attention to the region of emitted protons having kinetic energy above 600 MeV, which was used to claim a deeply attractive kaon nucleus optical potential. Our model describes the nuclear reaction in the framework of a local density approach and the calculations are performed following two different procedures: one is based on a many-body method using the Lindhard function and the other is based on a Monte Carlo simulation. The simulation method offers flexibility to account for processes other than kaon quasielastic scattering, such as K- absorption by one and two nucleons, producing hyperons, and all…

Nuclear reactionNuclear and High Energy PhysicsParticle physicsNuclear TheoryMesonHadronNuclear TheoryFOS: Physical sciencesElementary particle7. Clean energy01 natural sciencesNuclear Theory (nucl-th)MomentumNuclear physics0103 physical sciencesProton emission010306 general physicsNuclear ExperimentBosonPhysicsReaccions nuclears010308 nuclear & particles physicsSpecific reactions and phenomenologyFísicaFenomenologia (Física)High Energy Physics::ExperimentNuclear reactionsNucleon
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Probing the limit of nuclear existence: Proton emission from 159Re

2006

WOS: 000240847400007

Nuclear reactionNuclear and High Energy PhysicsSi detectorsProtonNuclear Theory[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]measured E (p) (t)1 / 201 natural sciences7. Clean energyNuclear physicsEp0103 physical sciencesEnriched targetsNeutronNuclideProton emissionNuclear Experiment010306 general physics106Cd at 300 MeV beam energyPhysicsIsotope010308 nuclear & particles physics21.10.Hw; 21.10.Tg; 23.50.+z; 27.70.+q58Nit1/2NUCLEAR REACTIONS Ni-58+Cd-106 at 300 MeV beam energy13. Climate actionNuclear reactionsGas-filled recoil separatorAtomic physicsNucleonMeasuredRadioactive decayPhysics Letters B
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Neutrino-nuclear responses for astro-neutrinos, single beta decays and double beta decays

2019

Abstract Neutrino–nuclear responses associated with astro-neutrinos, single beta decays and double beta decays are crucial in studies of neutrino properties of interest for astro-particle physics. The present report reviews briefly recent studies of the neutrino–nuclear responses from both experimental and theoretical points of view in order to obtain a consistent understanding of the many facets of the neutrino–nuclear responses. Subjects discussed in this review include (i) experimental studies of neutrino–nuclear responses by means of single beta decays, charge-exchange nuclear reactions, muon- photon- and neutrino–nuclear reactions, and nucleon-transfer reactions, (ii) implications of a…

Nuclear reactionParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoastrofysiikkasingle beta decaysNuclear TheoryGeneral Physics and Astronomyneutrino-nucleus interactionsnuclear matrix elements01 natural sciences7. Clean energyastro-neutrinosNucleosynthesisDouble beta decay0103 physical sciencesBeta (velocity)Nuclear Experiment010306 general physicsPhysicsdouble beta decaysMuonta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologymuon captureneutriinotMuon capturephoto-nuclear reactionsHigh Energy Physics::Experimentcharge-exchange reactionsNeutrinoPhysics Reports
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Lifetimes of intruder states in 186Pb, 188Pb and 194Po

2008

Abstract Lifetimes of prolate intruder states in 186Pb and 188Pb and oblate intruder states in 194Po have been determined through recoil distance Doppler-shift lifetime measurements. Deformation parameters of | β 2 | = 0.29 ( 5 ) and | β 2 | = 0.17(3) have been extracted from experimental B ( E 2 ) values for the prolate and the oblate bands, respectively. The present study addresses the phenomenon of shape coexistence typical for the nuclei near Z = 82 and N = 104 , providing information on configuration mixing of intrinsic structures of the nuclei of interest. The results are compared with the available lifetime data and theoretical results for neutron-deficient Po, Pb, Hg and Pt nuclei. …

Nuclear reactionPhysicsNuclear and High Energy Physics21.10.Tg; 23.20.Lv; 27.70.+q; 27.80.+wquadrupole moment[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]010308 nuclear & particles physics114Cd(83Kr 3n)Prolate spheroid7. Clean energy01 natural sciencesdeformation parametersE=340–375 MeVRecoil108Pd106Pd0103 physical sciencesQuadrupoleOblate spheroidDeformation (engineering)Atomic physics010306 general physicsnuclear reactionsMixing (physics)
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Few-body problems in nuclear astrophysics

2005

Few-body methods provide very useful tools to solve different problems important for nuclear astrophysics. Some of them are discussed below.

Nuclear reactionPhysicsNuclear and High Energy PhysicsComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATIONComputingMethodologies_SIMULATIONANDMODELINGNuclear TheoryAstrophysics::Instrumentation and Methods for AstrophysicsNuclear structure8B formation; nuclear reactions; triple collisionsComputerApplications_COMPUTERSINOTHERSYSTEMSFew-body systemsNuclear physicsNuclear astrophysicsNuclear ExperimentJournal of Physics G: Nuclear and Particle Physics
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Decay of the high-spin isomer in 160Re: Changing single-particle structure beyond the proton drip line

2011

WOS: 000286708700015

Nuclear reactionPhysicsNuclear and High Energy PhysicsProtonta114Gas-filled recoil separator Si and Ge strip detectorsNUCLEAR REACTIONS Ni-58+Cd-106 at 290300 MeV beam energy enriched targetsMeasured E gamma t1/2ParticleNeutronNuclear reactionsAtomic physicsProton emissionGround stateMeasuredLine (formation)Spin-½Physics Letters B
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