S_eff(E) and the 7Be(p,gamma)8B reaction

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dc.creatorJennings, B. K.
dc.creatorKarataglidis, S.
dc.date1998-07-02
dc.date.accessioned2026-07-07T11:11:46Z
dc.date.available2026-07-07T11:11:46Z
dc.descriptionWe explore approximations to the effective $S$ factor for the $^7Be(p,γ)^8B$ reaction using different approximation for the integral over the Gamov peak. In the temperature range of interest for solar neutrino production, $S_{eff}(E)$ may be determined to within 0.5% from S(20) with no direct information on the derivatives of S(E).
dc.identifierhttps://arxiv.org/abs/nucl-th/9807007
dc.identifierhttp://arxiv.org/abs/nucl-th/9807007
dc.identifierPhys.Rev.C58:3002-3003,1998
dc.identifierdoi:10.1103/PhysRevC.58.3002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191207
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleS_eff(E) and the 7Be(p,gamma)8B reaction
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