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Astron. Astrophys. 342, 464-473 (1999)

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Rapid proton capture on accreting neutron stars - effects of uncertainty in the nuclear process

O. Koike 1, M. Hashimoto 1, K. Arai 2 and S. Wanajo 3

1 Department of Physics, Kyushu University, Ropponmatsu, Fukuoka 810-8560, Japan
2 Department of Physics, Kumamoto University, Kurokami, Kumamoto 860-8555, Japan
3 Division of Theoretical Astrophysics, National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan

Received 19 August 1998 / Accepted 2 October 1998

Abstract

The rapid proton capture process on accreting neutron stars is investigated with the use of the current nuclear data and extended nuclear reaction networks. A simple but crucial model is adopted to investigate the detailed nucleosynthesis during the burst: the plane parallel (one zone) model. Compared with the results of Hanawa et al. (1983), significant differences are found. The peak temperature becomes higher due to the rapid break out from the hot CNO cycle. The amount of the fuel left after the burst depends on the still uncertain Q-values of [FORMULA] reactions for nuclei like [FORMULA]. It is also demonstrated that the uncertainties in the nuclear data should influence significantly the profile of the light curve in the burst models.

Key words: nuclear reactions, nucleosynthesis, abundances – stars: neutron – X-rays: bursts

Send offprint requests to: M. Hashimoto

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© European Southern Observatory (ESO) 1999

Online publication: February 22, 1999
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