Nuclear data sheets for A = 92

Luksch, Peter

doi:10.1016/s0090-3752(80)80057-3

Cited by 31 publications

(3 citation statements)

References 136 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The treatment of the pair correlations obviously suffers most from the truncation to the smallp1/2g9,2 space. For the 3.007 and 3.369MeV levels we suggest spin-parity assignments, 4-and 3-respectively, in disagreement with the assignments 5and (4) of Nuclear Data Sheets [31]. If the non-yrast experimental levels drawn in Fig.…”

Section: The Nucleus 9 2 ~~mentioning

confidence: 55%

Shell Model Description of theN= 50 Isotones Between⁸⁸Sr and¹⁰⁰Sn

Blomqvist¹,

Rydström²

1985

Phys. Scr.

View full text Add to dashboard Cite

A model consisting of protons filling the shells lg,,, and 2p,,, is leastsquares fitted to 63 low-lying energy levels in N = 50 isotones from 89Y to 96Pd. The single-particle energies and two-particle interaction matrix elements are treated as free parameters. A root-mean-square deviation of 64 keV is obtained for the levels included in the fit. Binding energies and excitation spectra for all the N = 50 nuclei between "Sr and '"Sn are calculated with the resulting effective interaction.

show abstract

Section: The Nucleus 9 2 ~~mentioning

confidence: 55%

Shell Model Description of theN= 50 Isotones Between⁸⁸Sr and¹⁰⁰Sn

Blomqvist¹,

Rydström²

1985

Phys. Scr.

View full text Add to dashboard Cite

show abstract

“…However, from the text in [23] it becomes obvious that the half-life is 0.62 ps, corresponding to M1 transition strengths of the order of several µ 2 N for the above mentioned transitions. Surprisingly, a half-life of 0.62 ns has been adopted in [5], and this value persists until now [1][2][3][4].…”

Section: Coupling Between the Ground State And The Isomer Via Intmentioning

confidence: 99%

“…Thus, direct electromagnetic M5 or E6 transitions to the J π = 7 + ground state are highly suppressed, and the 2 + isomer decays also by electron capture to 92 Zr with a short half-life of t 1/2 = 10.15 d which is 9 orders of magnitude smaller than the half-life of the 92 Nb ground state. Except explicitly noted, all properties of 92 Nb have been taken from the ENSDF database [1] which is based on the Nuclear Data Sheets [2][3][4][5].…”

Section: Introductionmentioning

confidence: 99%

Nucleosynthesis ofNb92and the relevance of the low-lying isomer at 135.5 keV

Mohr

2016

Phys. Rev. C

View full text Add to dashboard Cite

Background: Because of its half-life of about 35 million years, 92 Nb is considered as a chronometer for nucleosynthesis events prior to the birth of our sun. The abundance of 92 Nb in the early solar system can be derived from meteoritic data. It has to be compared to theoretical estimates for the production of 92 Nb to determine the time between the last nucleosynthesis event before the formation of the early solar system. Purpose Conclusions: The low-lying isomer in92 Nb does not affect the production of 92 Nb in explosive scenarios. In retrospect this validates all previous studies where the isomer was not taken into account. However, the dramatic reduction of the effective half-life at temperatures below 10 keV may affect the survival of 92 Nb after its synthesis in supernovae which are the most likely astrophysical site for the nucleosynthesis of 92 Nb.

show abstract