Shell-model studies of the astrophysicalrpreaction29P(p,γ)30S
Author:
Funder
National Science Foundation
Publisher
American Physical Society (APS)
Subject
Nuclear and High Energy Physics
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.87.065803/fulltext
Reference17 articles.
1. Level structure of30S and its importance in the26Si(α,p)29P and29P(p,γ)30S reaction rates
2. Level structure of30S: Implications for the astrophysical29P(p,γ)30S reaction rate in ONe novae and x-ray bursts
3. Properties ofMg26andSi26in thesdshell model and the determination of theAl25(p,γ)Si26reaction rate
4. New “USD” Hamiltonians for thesdshell
5. Empirical isospin-nonconserving hamiltonians for shell-model calculations
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