Search results for "shell model"

showing 10 items of 146 documents

First-forbidden transitions in the reactor anomaly

2018

We study the dominant forbidden transitions in the antineutrino spectra of the fission actinides from 4 MeV onward using the nuclear shell model. Through explicit calculation of the shape factor, taking into account Coulomb corrections, we show the expected changes on cumulative electron and antineutrino spectra. Compared to the usual allowed approximation this results in a minor decrease of electron spectra from 4 MeV and onward, whereas an increase of several percent is observed in antineutrino spectra. We show that, despite their limited number, forbidden transitions dominate the spectral flux for most of the experimentally accessible range. Based on the shell model calculations we attem…

Nuclear TheoryMonte Carlo methodAb initioFOS: Physical sciencesElectronhiukkasfysiikka7. Clean energy01 natural sciencesSpectral lineHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)0103 physical sciencesCoulombfissionNuclear Experiment (nucl-ex)Nuclear Experiment010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsneutrino interactionsshell modelNuclear shell modelComputational physicselectroweak interactions in nuclear physicsnuclear reactorsbeta decayAnomaly (physics)ydinfysiikkaParametrization
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Evidence for a spin-aligned neutron-proton paired phase from the level structure of (92)Pd

2011

4 páginas, 4 figuras.-- El Pdf es la versión pre-print.-- et al.

Nuclear TheoryProton[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]pairingNuclear Theory (nucl-th)Magic number (programming)spin-alignementPhysics::Atomic and Molecular ClustersNuclear forceNeutronNuclear structureNuclear Experiment (nucl-ex)Spin (physics)Nuclear ExperimentNuclear ExperimentPhysicsMultidisciplinaryta114Nuclear structureNuclear shell modelAtomic nucleusFísica nuclearAtomic physics
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Shell-model calculation of isospin-symmetry breaking correction to superallowed Fermi beta-decay

2016

We investigate the radial-overlap part of the isospin-symmetry breaking correction to superallowed $0^+\to 0^+$-decay using the shell-model approach similar to that of Refs. [1, 2]. The 8 sd-shell emitters with masses between $A=22$ and $A=38$ have been re-examined. The Fermi matrix element is evaluated with realistic spherical single-particle wave functions, obtained from spherical Woods-Saxon (WS) or Hartree-Fock (HF) potentials, fine-tuned to reproduce the experimental data on charge radii and separation energies for nuclei of interest. The elaborated adjustment procedure removes any sensitivity of the correction to a specific parametrisation of the WS potential or to various versions of…

Nuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]SHELL modelNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences23.40.-sNuclear physicsNuclear Theory (nucl-th)21.60.Cs0103 physical sciences21.10.PcSensitivity (control systems)Symmetry breakingWave function010303 astronomy & astrophysics[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]Physicsta114010308 nuclear & particles physicsCharge (physics)Beta decay21.10.JxIsospinQuantum electrodynamics23.40.Bwbeta decayisospin-symmetry breakingFermi Gamma-ray Space Telescope
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High-spin bands in117,119I and118Xe

1984

Excited states in117I,118Xe and119I were populated in the reactions106Pd+16O and108, 110Cd+12C. The groundstate band in118Xe was observed to its (18+) member and the 11/2− bands in117I and119I to their (35/2−) and (43/2−) members, respectively. The structure of the bands in the I isotopes is interpreted as aπ h11/2 proton coupled to an even-even band structure in Xe, and the band crossings observed in118Xe and119I are interpreted in the Cranked Shell Model framework asABn ofv h11/2.

Nuclear and High Energy PhysicsIsotopeProtonChemistryExcited stateSHELL modelNuclear fusionElementary particleAtomic physicsElectronic band structureSpin (physics)Zeitschrift f�r Physik A Atoms and Nuclei
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Three beta-decaying states in 128In and 130In resolved for the first time using Penning-trap techniques

2020

Isomeric states in 128In and 130In have been studied with the JYFLTRAP Penning trap at the IGISOL facility. By employing state-of-the-art ion manipulation techniques, three different beta-decaying states in 128In and 130In have been separated and their masses measured. JYFLTRAP was also used to select the ions of interest for identification at a post-trap decay spectroscopy station. A new beta-decaying high-spin isomer feeding the isomer in 128Sn has been discovered in 128In at 1797.6(20) keV. Shell-model calculations employing a CD-Bonn potential re-normalized with the perturbative G-matrix approach suggest this new isomer to be a 16⁺ spin-trap isomer. In 130In, the lowest-lying (10⁻) isom…

Nuclear and High Energy PhysicsPenning trapAstronomy & Astrophysics01 natural sciencesIonPhysics Particles & Fieldsbeta-decay spectroscopyIsomersShell model0103 physical sciencesPhysics::Atomic and Molecular ClustersNuclear Experiment010306 general physicsSpectroscopyCouplingPhysicsScience & TechnologyNUCLEI010308 nuclear & particles physicsPhysicsPRECISION MASS-SPECTROMETRYNuclear shell modelR-PROCESSshell modelpenning trapRAMSEY METHODPenning traplcsh:QC1-999Physics NuclearExcited stateBeta (plasma physics)Physical SciencesSHELL-MODELTRANSITION-PROBABILITIESisomersAtomic physicsBeta-decay spectroscopylcsh:PhysicsIon cyclotron resonancePhysics Letters B
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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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Spins, Electromagnetic Moments, and Isomers of $^{107-129}Cd$

2013

The neutron-rich isotopes of cadmium up to the N=82 shell closure have been investigated by high-resolution laser spectroscopy. Deep-UV excitation at 214.5 nm and radioactive-beam bunching provided the required experimental sensitivity. Long-lived isomers are observed in 127Cd and 129Cd for the first time. One essential feature of the spherical shell model is unambiguously confirmed by a linear increase of the 11/2- quadrupole moments. Remarkably, this mechanism is found to act well beyond the h11/2 shell. The neutron-rich isotopes of cadmium up to the N=82 shell closure have been investigated by high-resolution laser spectroscopy. Deep-uv excitation at 214.5 nm and radioactive-beam bunchin…

Nuclear momentsNuclear Theoryddc:550FOS: Physical sciencesPhysics::Accelerator PhysicsNuclear Physics - ExperimentNuclear Experiment (nucl-ex)Laser spectroscopyNuclear ExperimentNuclear shell model
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Gamow-Teller Beta Decay of Neutron Rich Tc, Ru, Rh and Pd Isotopes

1988

During recent experiments at the IGISOL-facility several new neutron rich nuclides have been discovered, including the first direct observations of the beta decays of 111Tc, 112Ru, 113Ru, 114Ru, 113Rh, 115Rh, 116Rh and 118Pd. The role of the νg7/2 → πg9/2 transformation in the beta decays of the odd-odd 110–116Rh and the even-even 114–118Pd isotopes is shown to be dominant. The experimental results are compared with shell model calculations including deformation and pairing.

Nuclear physicsPhysicsIsotopePairingBeta (plasma physics)SHELL modelNeutronNuclideBeta decay
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Properties of heavy nuclei measured at the GSI SHIP

2004

Abstract The nuclear shell model predicts that the next doubly magic shell-closure beyond 208 Pb is at a proton number Z = 114, 120, or 126 and at a neutron number N = 172 or 184. The outstanding aim of experimental investigations is the exploration of this region of spherical ‘Super-Heavy Elements’ (SHEs). The measured decay data reveal that for the heaviest elements, the dominant decay mode is α emission, not fission. Decay properties as well as reaction cross-sections are compared with results of theoretical investigations. Finally, plans are presented for the further development of the experimental set-up and the application of new techniques.At a higher sensitivity, the exploration of …

Nuclear physicsPhysicsNuclear and High Energy PhysicsFissionNeutron numberNuclear TheoryNuclear shell modelAtomic numberAtomic physicsNuclear ExperimentNuclear Physics A
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