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• W1696328114 abstract "A $ensuremath{gamma}$-ray spectroscopy study of ${}^{30}$S is presented. Excitation energies have been determined with improved precision over previous studies and firm spin-parity assignments have been made for key ${}^{29}text{P}+p$ resonant states. An evaluation of the ${}^{29}$P($p,ensuremath{gamma}$)${}^{30}$S reaction for $T=0.08$--2.5 GK shows that the 3${}^{+}$ and 2${}^{+}$ resonant states located at ${E}_{r}=289(3)$ and 410(3) keV, respectively, dominate the ${}^{29}$P($p$,$phantom{rule{0.16em}{0ex}}$$ensuremath{gamma}$)${}^{30}$S reaction rate in ONe novae, while the 410-keV resonance is expected to govern the rate in x-ray burster environments. These new, precise resonance energy measurements and firm spin-parity assignments have significantly reduced uncertainties in the ${}^{29}$P($p$,$phantom{rule{0.16em}{0ex}}$$ensuremath{gamma}$)${}^{30}$S reaction in ONe novae and x-ray bursts. In particular, the reaction rate is now specified precisely enough for calculations of isotopic abundances in ONe novae ejecta." @default.
• W1696328114 created "2016-06-24" @default.
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• W1696328114 date "2012-10-24" @default.
• W1696328114 modified "2023-09-27" @default.
• W1696328114 title "Level structure of30S: Implications for the astrophysical29P(p,γ)30S reaction rate in ONe novae and x-ray bursts" @default.
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• W1696328114 doi "https://doi.org/10.1103/physrevc.86.042801" @default.
• W1696328114 hasPublicationYear "2012" @default.
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