New P30(p,γ)S31 resonances and oxygen-neon nova nucleosynthesis

Details New P30(p,γ)S31 resonances and oxygen-neon nova nucleosynthesis New P30(p,γ)S31 resonances and oxygen-neon nova nucleosynthesis

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phrvc..76e2802w&link_type=abstract

Physical Review C, vol. 76, Issue 5, id. 052802

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7

Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Charge-Exchange Reactions, 20<=A<=38

Scientific paper

Enriched isotopic abundance ratios of Si30/Si28 in several presolar SiC and graphite grains qualitatively indicate massive oxygen-neon (ONe) nova origins but fall short of hydrodynamic ONe nova model ejecta predictions by as much as an order of magnitude. The astrophysical P30(p,γ)S31 reaction rate uncertainty at ONe nova temperatures (0.10

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