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Phys Rev Lett. 2011 Jun 24;106(25):252503. doi: 10.1103/PhysRevLett.106.252503. Epub 2011 Jun 24.

Ground-state proton decay of 69Br and implications for the 68Se astrophysical rapid proton-capture process waiting point.

Physical review letters

A M Rogers, M A Famiano, W G Lynch, M S Wallace, F Amorini, D Bazin, R J Charity, F Delaunay, R T de Souza, J Elson, A Gade, D Galaviz, M-J van Goethem, S Hudan, J Lee, S Lobastov, S Lukyanov, M Matoš, M Mocko, H Schatz, D Shapira, L G Sobotka, M B Tsang, G Verde

Affiliations

  1. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA. [email protected]

PMID: 21770637 DOI: 10.1103/PhysRevLett.106.252503

Abstract

We report on the first direct measurement of the proton separation energy for the proton-unbound nucleus (69)Br. Bypassing the (68)Se waiting point in the rp process is directly related to the 2p-capture rate through (69)Br, which depends exponentially on the proton separation energy. We find a proton separation energy for (69)Br of Sp((69)Br )= -785(-40)(+34) keV; this is less bound compared to previous predictions which have relied on uncertain theoretical calculations. The influence of the extracted proton separation energy on the rp process occurring in type I x-ray bursts is examined within the context of a one-zone burst model.

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