0000000000722592

AUTHOR

Toshitaka Kajino

showing 3 related works from this author

Determination of beta-delayed neutron emission probability limits of rhodium isotopes by gamma-ray spectroscopy

2019

9 pags., 5 figs., 5 tabs. -- 27th International Nuclear Physics Conference (INPC2019) 29 July - 2 August 2019, Glasgow, UK

PaperHistoryFissionNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear Theorychemistry.chemical_element[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesEducationNuclear physics0103 physical sciencesGamma spectroscopyNuclear drip lineNuclide010306 general physicsNuclear ExperimentPhysicsIsotope010308 nuclear & particles physics3. Good healthComputer Science Applicationsddc:chemistryPhysics::Accelerator PhysicsBerylliumDelayed neutron
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β-Decay Half-Lives of 110 Neutron-Rich Nuclei across theN=82Shell Gap: Implications for the Mechanism and Universality of the AstrophysicalrProcess

2015

The $\ensuremath{\beta}$-decay half-lives of 110 neutron-rich isotopes of the elements from $_{37}\mathrm{Rb}$ to $_{50}\mathrm{Sn}$ were measured at the Radioactive Isotope Beam Factory. The 40 new half-lives follow robust systematics and highlight the persistence of shell effects. The new data have direct implications for $r$-process calculations and reinforce the notion that the second ($A\ensuremath{\approx}130$) and the rare-earth-element ($A\ensuremath{\approx}160$) abundance peaks may result from the freeze-out of an $(n,\ensuremath{\gamma})\ensuremath{\rightleftarrows}(\ensuremath{\gamma},n)$ equilibrium. In such an equilibrium, the new half-lives are important factors determining t…

Nuclear physicsPhysicsStarsIsotopeDouble beta decayGeneral Physics and Astronomyr-processNeutron7. Clean energyUniversality (dynamical systems)Physical Review Letters
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Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions

2010

The rp‐process nucleosynthesis proceeds through nuclei near the proton drip‐line, in which Gamow‐Teller (GT) transitions starting from unstable pf‐shell nuclei play important roles. In the β‐decay study of these nuclei, half‐lives can be measured rather accurately. On the other hand, in the high‐resolution (3He, t) charge‐exchange reactions on mirror nuclei, individual GT transitions can be studied up to high excitations. For the accurate study of the GT transition strengths in the A = 52, T = 2, system, we compare and combine the β‐decay study of the proton‐rich nucleus 52Ni and the 52Cr(3He, t) measurement assuming the isospin symmetry of the Tz = ±2→±1 transitions.

PhysicsNuclear reactionNuclear physicsProtonNucleosynthesisHadronr-processMirror nucleiAtomic physicsNucleonIsotopes of heliumAIP Conference Proceedings
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