Gamow-Teller strength distributions and stellar weak-interaction rates for $^{76}$Ge and $^{82}$Se using the deformed pn-QRPA model

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Hauptverfasser: Nabi, Jameel-Un, Ishfaq, Mavra
Format: Preprint
Veröffentlicht: 2025
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author Nabi, Jameel-Un
Ishfaq, Mavra
author_facet Nabi, Jameel-Un
Ishfaq, Mavra
contents We calculate Gamow-Teller strength distributions for $ββ$-decay nuclei $^{76}$Ge and $^{82}$Se using the deformed pn-QRPA model. We use a deformed Nilsson basis and consider pairing correlations within the deformed BCS theory. Ground state correlations and two-particle and two-hole mixing states were included in our pn-QRPA model. Our calculated strength distributions were compared with experimental data and previous calculation. The total Gamow-Teller strength and centroid placement calculated in our model compares well with the measured value. We calculate $β$-decay and positron capture rates on $^{76}$Ge and $^{82}$Se in supernovae environments and compare them to those obtained from experimental data and previous calculation. Our study shows that positron capture rates command the total weak rates at high stellar temperatures. We also calculate energy rates of $β$-delayed neutrons and their emission probabilities.
format Preprint
id arxiv_https___arxiv_org_abs_2505_06967
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Gamow-Teller strength distributions and stellar weak-interaction rates for $^{76}$Ge and $^{82}$Se using the deformed pn-QRPA model
Nabi, Jameel-Un
Ishfaq, Mavra
Nuclear Theory
We calculate Gamow-Teller strength distributions for $ββ$-decay nuclei $^{76}$Ge and $^{82}$Se using the deformed pn-QRPA model. We use a deformed Nilsson basis and consider pairing correlations within the deformed BCS theory. Ground state correlations and two-particle and two-hole mixing states were included in our pn-QRPA model. Our calculated strength distributions were compared with experimental data and previous calculation. The total Gamow-Teller strength and centroid placement calculated in our model compares well with the measured value. We calculate $β$-decay and positron capture rates on $^{76}$Ge and $^{82}$Se in supernovae environments and compare them to those obtained from experimental data and previous calculation. Our study shows that positron capture rates command the total weak rates at high stellar temperatures. We also calculate energy rates of $β$-delayed neutrons and their emission probabilities.
title Gamow-Teller strength distributions and stellar weak-interaction rates for $^{76}$Ge and $^{82}$Se using the deformed pn-QRPA model
topic Nuclear Theory
url https://arxiv.org/abs/2505.06967