6533b82ffe1ef96bd1295aaf

RESEARCH PRODUCT

Gamow-Teller decay ofZn80: Shell structure and astrophysical implications

V. HarmsKarl KratzPeter MöllerA. Wöhr

subject

PhysicsNuclear and High Energy PhysicsNuclear TheorySHELL modelShell (structure)QuasiparticleBeta (velocity)Atomic physicsWave function

description

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.

https://doi.org/10.1103/physrevc.38.278