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At finite temperatures (≥ 107K), 76Se is abundant in the core of massive stars and electron capture on 76Se has a consequential role to play in the dynamics of core-collapse. The present work may be classified into two main categories. In the first phase we study the nuclear structure properties of 76Se using the interacting boson model-1 (IBM-1). The IBM-1 investigations include the energy levels,...
We investigate even–even nuclei in the A∼70 mass region within the framework of the proton–neutron quasi-particle random phase approximation (pn-QRPA) and the interacting boson model-1 (IBM-1). Our work includes calculation of the energy spectra and the potential energy surfaces V(β,γ) of Zn, Ge, Se, Kr and Sr nuclei with the same proton and neutron number, N=Z. The parametrization of the IBM-1 Hamiltonian...
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