Nuclear Structure Properties and Stellar Weak Rates for 76Se: Unblocking of the Gamow Teller Strength

Jameel-Un Nabi, Mavra Ishfaq, Mahmut Boyukata +1

At finite temperatures ($\ge 10^7$K), ${}^{76}$Se is abundant in the core of massive stars and electron capture on ${}^{76}$Se has a consequential role to play in the dynamics of core…