Collective C2 transitions in 32S with higher-energy configurations

Abstract EN

Collective C2 transitions in 32S are discussed for higher energy configurations by comparing the calculations of transition strength B (CJ) with the experimental data.

These configurations are taken into account through a microscopic theory including excitations from the core orbits and the model space orbits with no ω excitations up to n = 10 are considered.

However n = 6 seems to be large enough for a sufficient convergence.

The calculations include the lowest seven 2 + 0 states of 32S.