Search results for "nuclear reaction"

showing 10 items of 449 documents

Large-angle production of charged pions by 3 GeV/c-12 GeV/c protons on carbon, copper and tin targets

2008

A measurement of the double-differential pi(+/-) production cross-section in proton-carbon, proton-copper and proton-tin collisions in the range of pion momentum 100 MeV/c <= p <800 MeV/c and angle 0.35 rad <= theta < 2.15 rad is presented. The data were taken with the HARP detector in the T9 beam line of the CERN PS. The pions were produced by proton beams in a momentum range from 3 GeV/c to 12 GeV/c hitting a target with a thickness of 5% of a nuclear interaction length. The tracking and identification of the produced particles was done using a small-radius cylindrical time projection chamber (TPC) placed in a solenoidal magnet. An elaborate system of detectors in the beam line ensured th…

Nuclear reactionParticle physicsPhysics and Astronomy (miscellaneous)ProtonMesonPhysics::Instrumentation and DetectorsHadronNuclear TheoryFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Pion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear interaction length010306 general physicsNuclear ExperimentEngineering (miscellaneous)PhysicsTime projection chamberLarge Hadron Collidercross section010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleFísicaSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Physics::Accelerator PhysicsHigh Energy Physics::ExperimentParticle Physics - ExperimentEUROPEAN PHYSICAL JOURNAL C
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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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Measurement of the production cross-section of positive pions in the collision of 8.9 GeV/c protons on beryllium

2007

The double-differential production cross-section of positive pions, $d^2\sigma^{\pi^{+}}/dpd\Omega$, measured in the HARP experiment is presented. The incident particles are 8.9 GeV/c protons directed onto a beryllium target with a nominal thickness of 5% of a nuclear interaction length. The measured cross-section has a direct impact on the prediction of neutrino fluxes for the MiniBooNE and SciBooNE experiments at Fermilab. After cuts, 13 million protons on target produced about 96,000 reconstructed secondary tracks which were used in this analysis. Cross-section results are presented in the kinematic range 0.75 GeV/c < $p_{\pi}$ < 6.5 GeV/c and 30 mrad < $\theta_{\pi}$ < 210 mrad in the l…

Nuclear reactionParticle physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics and Astronomy (miscellaneous)HadronFOS: Physical scienceschemistry.chemical_elementddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsMiniBooNEHigh Energy Physics - Experiment (hep-ex)Pion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsNuclear ExperimentEngineering (miscellaneous)PhysicsTime projection chamber010308 nuclear & particles physicsSettore FIS/01 - Fisica Sperimentalecross section particle physicsFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]chemistryHigh Energy Physics::ExperimentBerylliumNeutrinoParticle Physics - Experiment
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Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

2014

The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as we…

Nuclear reactionPhysics - Instrumentation and DetectorsProtonneutrino: solarPhysics::Instrumentation and Detectors01 natural sciences7. Clean energynuclear reactionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)PositronstarPrimary (astronomy)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysicsSPECTROSCOPYInstrumentation and Detectors (physics.ins-det)SOLAR NEUTRINOSAstrophysics - Solar and Stellar AstrophysicsBorexinoNeutrinomodel: solardeuteronGRAN SASSOParticle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]talk: Conca Specchiulla 2014/09/07[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationDETECTORSolar and Stellar Astrophysics (astro-ph.SR)neutrino: modelp p: fusion010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDeuterium13. Climate actionspectralHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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Be7(n,α)He4Reaction and the Cosmological Lithium Problem: Measurement of the Cross Section in a Wide Energy Range at n_TOF at CERN

2016

The energy-dependent cross section of the (7)Bed(n,alpha)He-4 reaction, of interest for the so-called cosmological lithium problem in big bang nucleosynthesis, has been measured for the first time from 10 meV to 10 keV neutron energy. The challenges posed by the short half-life of Be-7 and by the low reaction cross section have been overcome at n_TOF thanks to an unprecedented combination of the extremely high luminosity and good resolution of the neutron beam in the new experimental area (EAR2) of the n_TOF facility at CERN, the availability of a sufficient amount of chemically pure Be-7, and a specifically designed experimental setup. Coincidences between the two alpha particles have been…

Nuclear reactionPhysics010308 nuclear & particles physicsGeneral Physics and Astronomychemistry.chemical_elementAlpha particleNeutron radiation7. Clean energy01 natural sciencesNeutron temperatureNuclear physicsBig Bang nucleosynthesischemistry13. Climate actionNucleosynthesis0103 physical sciencesNeutronLithiumNuclear Experiment010306 general physicsPhysical Review Letters
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Experimental Neutron Capture Rate Constraint Far from Stability

2016

Nuclear reactions where an exotic nucleus captures a neutron are critical for a wide variety of applications, from energy production and national security, to astrophysical processes, and nucleosynthesis. Neutron capture rates are well constrained near stable isotopes where experimental data are available; however, moving far from the valley of stability, uncertainties grow by orders of magnitude. This is due to the complete lack of experimental constraints, as the direct measurement of a neutron-capture reaction on a short-lived nucleus is extremely challenging. Here, we report on the first experimental extraction of a neutron capture reaction rate on ^{69}Ni, a nucleus that is five neutro…

Nuclear reactionPhysics010308 nuclear & particles physicsStable isotope ratioAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and Astronomy7. Clean energy01 natural sciencesStability (probability)Nuclear physicsNeutron captureOrders of magnitude (time)13. Climate actionValley of stabilityNucleosynthesis0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysical Review Letters
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Anomalous Behavior of High-Spin States inCm248

1981

The ground-state band of $^{248}\mathrm{Cm}$ has been studied up to spin ${28}^{+}$ and tentatively to ${30}^{+}$ by observing $\ensuremath{\gamma}$ rays following multiple Coulomb excitation with use of $^{208}\mathrm{Pb}$ ions at 5.3 MeV/u. A smooth, gradual increase in the effective moment of inertia is seen at lower spin with an anomalous forward bend above spin ${22}^{+}$. Calculations are presented which indicate that this behavior including the forward bend can be understood in terms of the alignment of single-particle angular momenta along the rotation axis.

Nuclear reactionPhysicsAngular momentumSpin statesGeneral Physics and AstronomyCoulomb excitationInelastic scatteringAtomic physicsMoment of inertiaExcitationSpin-½Physical Review Letters
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r-process chronometers

2004

Abstract We compare calculations of r-process abundances with recent astronomical observations from extremely metal-deficient, neutron-capture-rich halo stars. We derive criteria to determine Th and U chronometric ages, and deduce astrophysical conditions under which the observed abundance patterns can be obtained under r-like conditions.

Nuclear reactionPhysicsAstronomyAstronomy and AstrophysicsAstrophysicslaw.inventionGalactic haloStarsMarine chronometerSpace and Planetary ScienceNucleosynthesislawAbundance (ecology)Astrophysics::Solar and Stellar Astrophysicsr-processHaloAstrophysics::Galaxy AstrophysicsNew Astronomy Reviews
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Structure ofIn112nucleus

1988

The \ensuremath{\gamma}-ray spectra of the $^{112}\mathrm{Cd}$(p,n\ensuremath{\gamma}${)}^{112}$In and $^{109}\mathrm{Ag}$(\ensuremath{\alpha},n\ensuremath{\gamma}${)}^{112}$In reactions were measured with Ge(Li) spectrometers for bombarding energies of 4.8 MeV protons and 17.1 MeV \ensuremath{\alpha} particles. The energies and relative intensities of 79 $^{112}\mathrm{In}$ \ensuremath{\gamma}-ray transitions have been determined. The electron spectra were measured with combined magnet plus Si(Li) as well as superconducting magnetic lens plus Si(Li) spectrometers. Internal conversion coefficients of 40 $^{112}\mathrm{In}$ transitions have been determined, and the level scheme of $^{112}\ma…

Nuclear reactionPhysicsBaryonNuclear and High Energy PhysicsBranching fractionAstrophysics::High Energy Astrophysical PhenomenaQuadrupoleHadronElementary particleAtomic physicsNuclear ExperimentNucleonSpectral linePhysical Review C
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C12(γ,p)11B cross section from 80 to 157 MeV

1995

The $^{12}\mathrm{C}$(\ensuremath{\gamma},p${)}^{11}$B differential cross section has been measured over proton angles ranging from 58\ifmmode^\circ\else\textdegree\fi{} to 128\ifmmode^\circ\else\textdegree\fi{}, using tagged photons of energy 80--157 MeV, for low-lying regions of residual excitation energy in $^{11}\mathrm{B}$. The data have been compared with four different types of calculation. It is shown that scaling of the cross section with momentum mismatch occurs for both the ground-state and excited-state data.

Nuclear reactionPhysicsBaryonNuclear and High Energy PhysicsProtonHadronElementary particleIsotopes of boronAtomic physicsNucleonEnergy (signal processing)Physical Review C
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