Journal article
Discovery of 34g,mCl(p,γ)35Ar resonances activated at classical nova temperatures
Abstract
Background: The thermonuclear 34g,mCl(p,γ)35Ar reaction rates are unknown due to a lack of experimental nuclear physics data. Uncertainties in these rates translate to uncertainties in S34 production in models of classical novae on oxygen-neon white dwarfs. S34 abundances have the potential to aid in the classification of presolar grains. Purpose: Determine resonance energies for the 34g,mCl(p,γ)35Ar reactions within the region of astrophysical …
Authors
Fry C; Wrede C; Bishop S; Brown BA; Chen AA; Faestermann T; Hertenberger R; Parikh A; Pérez-Loureiro D; Wirth H-F
Journal
Physical Review C, Vol. 91, No. 1,
Publisher
American Physical Society (APS)
Publication Date
January 1, 2015
DOI
10.1103/physrevc.91.015803
ISSN
2469-9985