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arXiv · 2508.05456

Weak interaction rates of $sd$-shell Urca pairs in stellar environment using a shell-model approach

Shweta Sharma·Praveen C. Srivastava·Toshio Suzuki
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Abstract

In this work, the weak interaction rates of $sd$-shell nuclei in the hot and dense stellar environment are calculated using the shell model. The {\it ab initio} effective interactions are employed for the calculation of Gamow-Teller strengths and weak rates in addition to the phenomenological interaction. The weak rates are evaluated in a fine grid of density and temperature. The electron capture and $\beta^-$-decay rates of Urca pairs of nuclei with $A = 23, 25, 29, 31$ and 33 are evaluated as a function of $\log_{10} \rho Y_e$ and the corresponding Urca density is obtained. The screening effects are also included for the evaluation of these stellar weak rates. In addition, the intrinsic cooling strength is evaluated for $A=29,31$ and 33 Urca pairs in neutron star crusts. The stellar weak rates, along with the neutrino energy emitted and the gamma heat production, are tabulated for $A = 29-39$ nuclei.

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Shweta Sharma, Praveen C. Srivastava, Toshio Suzuki. 2025-08-07. Weak interaction rates of $sd$-shell Urca pairs in stellar environment using a shell-model approach. https://doi.org/10.1103/g4xl-rcmv

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