Comment on “Stellar Reactions with Short-Lived Nuclei:F17(p,α)O14”
Author:
Publisher
American Physical Society (APS)
Subject
General Physics and Astronomy
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.84.1635/fulltext
Reference5 articles.
1. Stellar Reactions with Short-Lived Nuclei:17F(p,α)14O
2. Structure of low-lying positive-parity states ofO18
3. Configuration off18O}(7.12 MeV,4+)
4. Coulomb energies in18Ne
5. Structure ofNe18and the breakout from the hot CNO cycle
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1. Properties of excited 0+ states in C14 and O14;Physical Review C;2020-07-13
2. Measurement of theO14(α,p)F17cross section atEc.m.≈2.1–5.3MeV;Physical Review C;2015-09-01
3. Examination of the role of theO14(α,p)F17reaction rate in type-I x-ray bursts;Physical Review C;2014-08-12
4. Astrophysics studies relevant to stellar x-ray bursts;AIP Conference Proceedings;2014
5. Branching ratio of18Ne(7.06 MeV,4+);Physical Review C;2012-12-13
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