Publication Date:
2015-01-14
Description:
Author(s): C. Fry, C. Wrede, S. Bishop, B. A. Brown, A. A. Chen, T. Faestermann, R. Hertenberger, A. Parikh, D. Pérez-Loureiro, H.-F. Wirth, A. García, and R. Ortez Background: The thermonuclear 34g,m Cl(p,γ) 35 Ar reaction rates are unknown due to a lack of experimental nuclear physics data. Uncertainties in these rates translate to uncertainties in 34 S production in models of classical novae on oxygen-neon white dwarfs. 34 S abundances have the potential to aid i... [Phys. Rev. C 91, 015803] Published Tue Jan 13, 2015
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
Permalink