Revised result for the 32 Cl ( p , γ ) 33 Ar reaction rate for astrophysical rp - process calculations
نویسندگان
چکیده
H. Schatz,1,2,3 C. A. Bertulani,1,∗ B. A. Brown,1,2 R. R. C. Clement,1,2,† A. A. Sakharuk,1,3 and B. M. Sherrill1,2,3 1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA 2Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA 3Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA (Received 4 April 2005; revised manuscript received 20 October 2005; published 30 December 2005)
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