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NSR database version of April 27, 2024.

Search: Author = K.Yokoi

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1987TA16      Phys.Rev. C36, 1522 (1987)

K.Takahashi, R.N.Boyd, G.J.Mathews, K.Yokoi

Bound-State Beta Decay of Highly Ionized Atoms

RADIOACTIVITY ³H, ¹⁴C, ³²Si, ³³P, ³⁵S, ⁴⁵Ca, ^63,66Ni, ⁹³Zr, ⁹⁵Nb, ¹⁰⁶Ru, ¹⁰⁷Pd, ^110mAg, ¹⁵¹Sm, ¹⁵⁵Eu, ¹⁶³Dy, ¹⁷¹Tm, ¹⁸⁷Re, ¹⁹¹Os, ¹⁹³Ir, ²⁰⁵Tl, ²¹⁰Pb, ²²⁸Ra, ²²⁷Ac, ²⁴¹Pu; calculated β-decay rates, T_1/2. Highly ionized atoms.

doi: 10.1103/PhysRevC.36.1522
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1987TA28      At.Data Nucl.Data Tables 36, 375 (1987)

K.Takahashi, K.Yokoi

Beta-Decay Rates of Highly Ionized Heavy Atoms in Stellar Interiors

COMPILATION Z=26-83; A=59-210; calculated β-decay rates for stellar environments.

doi: 10.1016/0092-640X(87)90010-6
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1984BE69      Astrophys.J. 278, 388 (1984)

H.Beer, F.Kappeler, K.Yokoi, K.Takahashi

The s-process branching at ¹⁵¹Sm

NUCLEAR REACTIONS ¹⁵²Sm, ¹⁵¹Eu, ^152,158,160Gd(n, γ), E=spectrum; measured Maxwellian-averaged σ. Astrophysical implications discussed.

doi: 10.1086/161804
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22603.

1983TA10      Nucl.Phys. A404, 578 (1983)

K.Takahashi, K.Yokoi

Nuclear β-Decays of Highly Ionized Heavy Atoms in Stellar Interiors

RADIOACTIVITY ¹⁶³Dy, ¹⁸⁷Re(β^-); calculated bound state β-decay rates; deduced nonunique transition importance in stellar interiors. Saha ionization equation, finite temperature Thomas-Fermi model.

doi: 10.1016/0375-9474(83)90277-4
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