Nucleosynthesis in X-ray bursts
Journal Article
·
· Bulletin of the American Physical Society
OSTI ID:255501
- and others
The origin of the most abundant p-nuclei {sup 92}Mo, {sup 94}Mo, {sup 96}Ru and {sup 98}Ru in the solar system is still not understood. We examined the possibility that these nuclei had been synthesized in the rp-process under high density and temperature conditions typical for explosive hydrogen burning on accreting neutron stars (X-ray bursts).
- OSTI ID:
- 255501
- Report Number(s):
- CONF-9510116--
- Journal Information:
- Bulletin of the American Physical Society, Journal Name: Bulletin of the American Physical Society Journal Issue: 10 Vol. 40; ISSN BAPSA6; ISSN 0003-0503
- Country of Publication:
- United States
- Language:
- English
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