Search results for "reactions"

showing 10 items of 631 documents

Measurements of forward proton production with incident protons and charged pions on nuclear targets at the CERN Proton Synchroton

2010

Measurements of the double-differential proton production cross-section d(2 sigma)/dpd Omega in the range of momentum 0.5 GeV/c <= p < 8.0 GeV/c and angle 0.05 rad <= theta < 0.25 rad in collisions of charged pions and protons on beryllium, carbon, aluminium, copper, tin, tantalum, and lead are presented. The data were taken with the large acceptance HARP detector in the T9 beam line of the CERN Proton Synchrotron. Incident particles were identified by an elaborate system of beam detectors and impinged on a target of 5% of a nuclear interaction length. The tracking and identification of the produced particles was performed using the forward spectrometer of the HARP experiment. Results are o…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsproton; nuclear targets; charged pionsFOS: Physical sciencesddc:500.201 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Basic research0103 physical sciencesCERN[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentInelastic proton scatteringPhysicsLarge Hadron Collider010308 nuclear & particles physicsOther reactions above meson production thresholds[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaPion-induced reactionsnuclear targetsResearch councilcharged pionsnuclear targetPhysics::Accelerator PhysicsHARP ExperimentHigh Energy Physics::ExperimentHumanitiesHARP Experiment; CERNParticle Physics - Experimentproton
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White paper: from bound states to the continuum

2020

This white paper reports on the discussions of the 2018 Facility for Rare Isotope Beams Theory Alliance (FRIB-TA) topical program ‘From bound states to the continuum: Connecting bound state calculations with scattering and reaction theory’. One of the biggest and most important frontiers in nuclear theory today is to construct better and stronger bridges between bound state calculations and calculations in the continuum, especially scattering and reaction theory, as well as teasing out the influence of the continuum on states near threshold. This is particularly challenging as many-body structure calculations typically use a bound state basis, while reaction calculations more commonly utili…

Nuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Structure (category theory)nucleus: structure functionFew-body systems[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesMany-body problemTheoretical physicsFew-body systems0103 physical sciencesBound stateReactionsNuclear structure010306 general physicsPhysicsBasis (linear algebra)010308 nuclear & particles physicsContinuum (topology)ScatteringscatteringNuclear structurePhysique atomique et nucléairebound statefew-body problemmany-body problem
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Single-particle shell strengths near the doubly magic nucleus 56Ni and the 56Ni(p,γ)57Cu reaction rate in explosive astrophysical burning

2019

Angle-integrated cross-section measurements of the $^{56}$Ni(d,n) and (d,p) stripping reactions have been performed to determine the single-particle strengths of low-lying excited states in the mirror nuclei pair $^{57}$Cu-$^{57}$Ni situated adjacent to the doubly magic nucleus $^{56}$Ni. The reactions were studied in inverse kinematics utilizing a beam of radioactive $^{56}$Ni ions in conjunction with the GRETINA $\gamma$-array. Spectroscopic factors are compared with new shell-model calculations using a full $pf$ model space with the GPFX1A Hamiltonian for the isospin-conserving strong interaction plus Coulomb and charge-dependent Hamiltonians. These results were used to set new constrain…

Nuclear and High Energy Physicsastro-ph.SRNuclear TheoryExplosive materialnucl-thStrong interactionnucl-ex01 natural sciencesIonReaction ratesymbols.namesake0103 physical sciencesCoulombMirror nuclei010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsradioactive beams010308 nuclear & particles physicsshell modellcsh:QC1-999Astrophysics - Solar and Stellar AstrophysicsExcited statesymbolsX-ray burststransfer reactionsAtomic physicsHamiltonian (quantum mechanics)ydinfysiikkalcsh:PhysicsPhysics Letters B
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Study of isomeric states in $^{198,200,202,206}$Pb and $^{206}$Hg populated in fragmentation reactions

2018

International audience; Isomeric states in isotopes in the vicinity of doubly-magic 208Pb were populatedfollowing reactions of a relativistic 208Pb primary beam impinging on a9Be fragmentation target. Secondary beams of 198,200,202,206Pb and 206Hg wereisotopically separated and implanted in a passive stopper positioned in thefocal plane of the GSI Fragment Separator. Delayed γ rays were detected withthe Advanced Gamma Tracking Array (AGATA). Decay schemes were reevaluatedand interpreted with shell-model calculations. The momentumdependentpopulation of isomeric states in the two-nucleon hole nuclei206Pb/206Hg was found to differ from the population of multi neutron-holeisomeric states in 198…

Nuclear and High Energy Physicsisomeric decaysAstrophysics::High Energy Astrophysical PhenomenaPopulationNuclear Theory[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesFragmentation (mass spectrometry)Subatomic Physics0103 physical sciencesGamma spectroscopyGamma-ray spectroscopy010306 general physicseducationNuclear ExperimentPhysicseducation.field_of_studyIsotope010308 nuclear & particles physicsNuclear shell modeldirect reactionsrelativistic projectile fragmentationelectromagnetic transitionsnuclear shell modelAGATAPreSPEC-AGATAAtomic physicsBeam (structure)
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Analysis of the Photoneutron Field Near the THz Dump of the CLEAR Accelerator at CERN With SEU Measurements and Simulations

2022

We study the radiation environment near the terahertz (THz) dump of the CERN Linear Electron Accelerator for Research (CLEAR) electron accelerator at CERN, using FLUktuierende KAskade in German (FLUKA) simulations and single-event upset (SEU) measurements taken with 32-Mbit Integrated Silicon Solution Inc. (ISSI) static random access memories (SRAMs). The main focus is on the characterization of the neutron field to evaluate its suitability for radiation tests of electronics in comparison with other irradiation facilities. Neutrons at CLEAR are produced via photonuclear reactions, mostly initiated by photons from the electromagnetic cascades that occur when the beam is absorbed by the dump …

Nuclear and High Energy Physicsphotonuclear reactionsSEUsfotonitacceleratorCLEARelectronsneutronsneutronitsäteilylaitteethiukkaskiihdyttimetAccelerators and Storage RingsNuclear Energy and EngineeringsäteilyfysiikkaCERNPhysics::Accelerator PhysicsphotonsR2ESRAMsElectrical and Electronic Engineeringradiation testing
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Systematic studies of correlations between different order flow harmonics in Pb-Pb collisions at √sNN = 2.76 TeV

2018

The correlations between event-by-event fluctuations of anisotropic flow harmonic amplitudes have been measured in Pb-Pb collisions at √ s NN = 2.76 TeV with the ALICE detector at the Large Hadron Collider. The results are reported in terms of multiparticle correlation observables dubbed symmetric cumulants. These observables are robust against biases originating from nonflow effects. The centrality dependence of correlations between the higher order harmonics (the quadrangular v 4 and pentagonal v 5 flow) and the lower order harmonics (the elliptic v 2 and triangular v 3 flow) is presented. The transverse momentum dependences of correlations between v 3 and v 2 and between v 4 and v 2 are …

Nuclear and High Energy Physicsviscous hydrodynamic modelsanisotropic flowharmonicsRelativistic heavy-ion collisionsheavy-ion collisionsNuclear reactionshiukkasfysiikkaParticle correlations & fluctuationsCollective flow
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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 &gt;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 &lt; 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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