Conference
Study of astrophysically important resonant states in 30S using the 32S(p,t)30S reaction
Abstract
The 29P(p,γ)30S reaction plays an important role in understanding the Si isotopic abundances in presolar grains of nova origin, which in turn provide us with information on the nature of the probable white dwarf progenitor's core, as well as the peak temperatures achieved during nova outbursts. This rate at nova temperatures is determined by two low-lying 3+ and 2+ resonances above the proton threshold at 4399 keV in 30S. We have studied the …
Authors
Setoodehnia K; Chen A-A; Chen J; Clark J-A; Deibel C; Kahl D; Lennard W-N; Parker P-D; Wrede C
Volume
834
Pagination
pp. 205c-207c
Publisher
Elsevier
Publication Date
March 2010
DOI
10.1016/j.nuclphysa.2009.12.041
Conference proceedings
Nuclear Physics A
Issue
1-4
ISSN
0375-9474