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- W2332793173 abstract "Proton-unbound excited states of ${}^{31}$S have been populated with the ${}^{32}$S($d,t$)${}^{31}$S reaction at a beam energy of 24 MeV. Tritons corresponding to ${}^{31}$S states with ${E}_{x}{(}^{31}S)ensuremath{approx}6.3$--$7.1$ MeV were momentum analyzed with a high resolution quadrupole-dipole-dipole-dipole (Q3D) magnetic spectrograph at six angles ranging from ${ensuremath{theta}}_{mathrm{lab}}={15}^{ensuremath{circ}}$ to $58.{5}^{ensuremath{circ}}$. We report a statistically significant detection of an astrophysically important state at ${E}_{x}{(}^{31}S)=6402$ (2) keV, whose existence as a third state in this region has been under debate. Using updated $A=31$ nuclear structure information, we present a new set of proposed ${}^{31}$S-${}^{31}$P mirror assignments for ${}^{31}$S, in which this state is tentatively assigned a spin of 7/2. This level, corresponding to a ${}^{30}$P + $p$ resonance at 271 keV, is likely to have a significant influence on the ${}^{30}$P($p,ensuremath{gamma}$)${}^{31}$S reaction rate in explosive hydrogen burning in classical novae." @default.
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- W2332793173 date "2013-11-27" @default.
- W2332793173 modified "2023-10-18" @default.
- W2332793173 title "Evidence for the existence of the astrophysically important 6.40-MeV state of<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msup><mml:mrow /><mml:mn>31</mml:mn></mml:msup></mml:math>S" @default.
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- W2332793173 doi "https://doi.org/10.1103/physrevc.88.055803" @default.
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