Work

α -unbound levels in Ar34 from Ar36(p,t)Ar34 reaction measurements and implications for the astrophysical S30(α,p)Cl33 reaction rate

Year: 2018
Type: article
Abstract: The $^{30}\mathrm{S}(\ensuremath{\alpha},p)^{33}\mathrm{Cl}$ reaction has been identified in several type-1 x-ray burst (XRB) sensitivity studies as a significant reaction within the $\ensuremath{\alpha}p$ process, possibly influencing not only the abundances of burst ashes but also the bolometric shape of double-peaked light curves coming from certain XRB systems. Given the dearth of experimental data on the $^{30}\mathrm{S}(\ensuremath{\alpha},p)$ $^{33}\mathrm{Cl}$ reaction at burst temperatures, we have performed high energy-resolution forward-angle $^{36}\mathrm{Ar}(p,t)^{34}\mathrm{Ar}$ measurements in order to identify levels in $^{34}\mathrm{Ar}$ that could appear as resonances in the $^{30}\mathrm{S}(\ensuremath{\alpha},p)^{33}\mathrm{Cl}$ reaction. Energies of levels identified in this work, along with model-based assumptions for spin assignments and spectroscopic factors, were then used to determine a rate for the $^{30}\mathrm{S}(\ensuremath{\alpha},p)^{33}\mathrm{Cl}$ reaction based on a narrow-resonance formalism. The rates determined in this work are then compared with two standard Hauser-Feshbach model predictions over a range of XRB temperatures.
Language: English
Open Access status: green
OpenAlex ID: W2803557097
FWCI: 0.708
Cites: 49
Cited by: 11
Related to: 10