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- W41313103 abstract "The structure of proton unbound $^{30}mathrm{S}$ states is important for determining the $^{29}mathrm{P}$($p,ensuremath{gamma}$)$^{30}mathrm{S}$ reaction rate, which influences explosive hydrogen burning in classical novae and type I x-ray bursts. The reaction rate in this temperature regime had been previously predicted to be dominated by two low-lying, unobserved, ${J}^{ensuremath{pi}}=$ ${3}^{+}$ and ${2}^{+}$ resonances above the proton threshold in $^{30}mathrm{S}$. To search for these levels, the structure of $^{30}mathrm{S}$ was studied using the $^{32}mathrm{S}$($p,t$)$^{30}mathrm{S}$ transfer reaction with a magnetic spectrograph. We have confirmed a previous detection of a state near 4700 keV, which had tentatively been assigned ${J}^{ensuremath{pi}}={3}^{+}$. We have also discovered a new state at 4814(3) keV, which is a strong candidate for the other important resonance (${J}^{ensuremath{pi}}={2}^{+}$). The new $^{29}mathrm{P}$($p,ensuremath{gamma}$)$^{30}mathrm{S}$ reaction rate is up to 4--20 times larger than previously determined rates over the relevant temperature range. The uncertainty in the reaction rate due to uncertainties in the resonance energies has been significantly reduced." @default.
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- W41313103 date "2010-08-26" @default.
- W41313103 modified "2023-10-16" @default.
- W41313103 title "Structure ofS30withS32(p,t)S30and the thermonuclearP29(p,γ)S30reaction rate" @default.
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- W41313103 doi "https://doi.org/10.1103/physrevc.82.022801" @default.
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