Coulomb displacement energy and the low-energy astrophysical S factor for the Be7(p,gamma)B8 reaction

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dc.creatorBrown, B. A.
dc.creatorCsoto, A.
dc.creatorSherr, R.
dc.date1995-06-06
dc.date1995-06-20
dc.date.accessioned2026-07-07T10:35:22Z
dc.date.available2026-07-07T10:35:22Z
dc.descriptionThe relationship between the Coulomb displacement energy for the A=8, J=2+, T=1 state and the low-energy astrophysical S factor for the Be7(p,gamma)B8 reaction is discussed. The displacement energy is interpreted in a particle-hole model. The dependence of the particle displacement energy on the potential well geometry is investigated and is used to relate the particle displacement energy to the rms radius and the asymptotic normalization of the valence proton wave function in B8. The asymptotic normalization is used to calculate the astrophysical S factor for the Be7(p,gamma)B8 reaction. The relationship to the Li7(n,gamma) reaction, the B8 quadrupole moment, radial density, and break-up momentum distribution are also discussed.
dc.descriptionLatex with Revtex, 26 pages, 8 figures are added in a uuencoded tar-compressed file
dc.identifierhttps://arxiv.org/abs/nucl-th/9506004
dc.identifierhttp://arxiv.org/abs/nucl-th/9506004
dc.identifierNucl.Phys.A597:66-84,1996
dc.identifierdoi:10.1016/0375-9474(95)00417-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179730
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleCoulomb displacement energy and the low-energy astrophysical S factor for the Be7(p,gamma)B8 reaction
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