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RESEARCH PRODUCT
Gamow-Teller decay ofZn80: Shell structure and astrophysical implications
V. HarmsKarl KratzPeter MöllerA. Wöhrsubject
PhysicsNuclear and High Energy PhysicsNuclear TheorySHELL modelShell (structure)QuasiparticleBeta (velocity)Atomic physicsWave functiondescription
Gamow-Teller \ensuremath{\beta} decay of $^{80}\mathrm{Zn}$ to levels in $^{80}\mathrm{Ga}$ has been calculated from a random-phase-approximation shell model with Nilsson model wave functions. The predicted features are compared to existing experimental results. Gross \ensuremath{\beta}-decay properties as well as quasiparticle structure indicate shape coexistence for $^{80}\mathrm{Ga}$. This result implies a rather rapid weakening of the shell strength far from \ensuremath{\beta} stability above $_{28}^{78}\mathrm{Ni}_{50}$. The nuclear properties of $^{80}\mathrm{Zn}$ as an astrophysical ``waiting-point'' nucleus suggest that the r-process scenario which is responsible for the solar r abundances has attained an (n,\ensuremath{\gamma})-(\ensuremath{\gamma},n) equilibrium.
year | journal | country | edition | language |
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1988-07-01 | Physical Review C |