2022 journal article
Experimental study of the Si-30(He-3, d) P-31 reaction and thermonuclear reaction rate of Si-30(p, gamma)( 3)1P
PHYSICAL REVIEW C, 105(1).
arxiv.org (repository)
Source: Web Of Science
Added: March 7, 2022
Element abundance anomalies in globular star clusters may be used to understand their history and to identify the nature of the stars responsible for these anomalies. The ${}^{30}$Si($p$,$\ensuremath{\gamma}$)${}^{31}$P thermonuclear rate is a key ingredient in addressing that topic, and a high-resolution indirect measurement of this radiative proton-capture reaction has been undertaken at relevant stellar temperatures. The strength of key resonances has been determined, and the major contributions to the remaining uncertainty are now well known.
