Enhancement of Resonant Thermonuclear Reaction Rates in Extremely Dense Stellar Plasmas

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dc.creatorItoh, Naoki
dc.creatorTomizawa, Nami
dc.creatorWanajo, Shinya
dc.creatorNozawa, Satoshi
dc.date2002-08-03
dc.date2002-12-06
dc.date.accessioned2026-07-07T11:46:01Z
dc.date.available2026-07-07T11:46:01Z
dc.descriptionThe enhancement factor of the resonant thermonuclear reaction rates is calculated for the extremely dense stellar plasmas in the liquid phase. In order to calculate the enhancement factor we use the screening potential which is deduced from the numerical experiment of the classical one-component plasma. It is found that the enhancement is tremendous for white dwarf densities if the ^{12}C + ^{12}C fusion cross sections show resonant behavior in the astrophysical energy range. We summarize our numerical results by accurate analytic fitting formulae.
dc.description13 pages, 3 figures, accepted for publication in ApJ, replaced with revised version
dc.identifierhttps://arxiv.org/abs/astro-ph/0208071
dc.identifierhttp://arxiv.org/abs/astro-ph/0208071
dc.identifierAstrophys.J.586:1436-1440,2003
dc.identifierdoi:10.1086/367720
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202079
dc.subjectAstrophysics
dc.titleEnhancement of Resonant Thermonuclear Reaction Rates in Extremely Dense Stellar Plasmas
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