Shell-model studies of the astrophysical rp -process reactions S 34 (p,γ) Cl 35 and Cl 34g,m (p,γ) Ar 35

1,2Richter, W.A.,3,9Brown, B.A.,4,5Longland, R.,3,9Wrede,C.,6Denissenkov, P.,3Fry, C.,5,9Herwig, F.,7Kurtulgil, D.,8,9,10Pignatari, M.,6Reifarth, R.
Physical Review C 102, 025801 Link to Article [DOI: 10.1103/PhysRevC.102.025801]
1University of Stellenbosch, Stellenbosch, 7600, South Africa
2IThemba LABS, Somerset West, 7130, South Africa
3Department of Physics and Astronomy, National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI 48824-1321, United States
4Department of Physics, North Carolina State University, Raleigh, NC 27695, United States
5Triangle Universities Nuclear Laboratory, Duke University, Durham, NC 27710, United States
6Department of Physics and Astronomy, University of Victoria, Victoria, BC V8W 2Y2, Canada
7Goethe University Frankfurt, Max-von-Laue-Strasse 1, Frankfurt am Main, 60438, Germany
8E.A. Milne Center for Astrophysics, Department of Physics and Mathematics, University of Hull, Hull, HU6 7RX, United Kingdom
9Konkoly Observatory, Research Center for Astronomy and Earth Sciences, Hungarian Academy of Sciences, Konkoly Thege Miklos ut 15-17, Budapest, H-1121, Hungary
10Joint Institute for Nuclear Astrophysics, Center for the Evolution of the Elements, Michigan State University, East Lansing, MI 48824, United States

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