Constraining the $^{30}$P($p,\gamma)^{31}$S reaction rate in ONe novae via the weak, low-energy, $\beta$-delayed proton decay of $^{31}$Cl

TL;DR

This study measures the weakest known beta-delayed proton emission below 400 keV to better constrain the $^{30}$P$(p, extgamma)^{31}$S reaction rate, improving nucleosynthesis models in oxygen-neon novae.

Contribution

It provides the first measurement of extremely weak beta-delayed proton decay of $^{31}$Cl, reducing uncertainties in the $^{30}$P$(p, extgamma)^{31}$S reaction rate.

Findings

Measured the weakest beta-delayed proton emission below 400 keV.

Reduced uncertainty in the $^{30}$P$(p, extgamma)^{31}$S reaction rate.

Predicted $^{30}$Si/$^{28}$Si excesses in presolar nova grains.

Abstract

The $^{30}$P$(p,\gamma)^{31}$S reaction plays an important role in understanding nucleosynthesis of $A\geq 30$ nuclides in oxygen-neon novae. The Gaseous Detector with Germanium Tagging was used to measure $^{31}$Cl $\beta$-delayed proton decay through the key $J^{\pi}=3/2^{+}$, 260-keV resonance. The intensity $I^{260}_{\beta p} = 8.3^{+1.2}_{-0.9} \times 10^{-6}$ represents the weakest $\beta$-delayed, charged-particle emission ever measured below 400 keV, resulting in a proton branching ratio of $\Gamma_p / \Gamma = 2.5^{+0.4}_{-0.3} \times 10^{-4}$. By combining this measurement with shell-model calculations for $\Gamma_{\gamma}$ and past work on other resonances, the total $^{30}$P$(p,\gamma)^{31}$S rate has been determined with reduced uncertainty. The new rate has been used in hydrodynamic simulations to model the composition of nova ejecta, leading to a concrete prediction of $^{30}$Si/$^{28}$Si excesses in presolar nova grains and the calibration of nuclear thermometers.