Nuclear reactions in hot stellar matter and nuclear surface deformation

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dc.creatorDenisov, V. Yu.
dc.date2006-11-13
dc.date.accessioned2026-07-07T10:20:47Z
dc.date.available2026-07-07T10:20:47Z
dc.descriptionCross-sections for capture reactions of charged particles in hot stellar matter turn out be increased by the quadrupole surface oscillations, if the corresponding phonon energies are of the order of the star temperature. The increase is studied in a model that combines barrier distribution induced by surface oscillations and tunneling. The capture of charged particles by nuclei with well-deformed ground-state is enhanced in stellar matter. It is found that the influence of quadrupole surface deformation on the nuclear reactions in stars grows, when mass and proton numbers in colliding nuclei increase.
dc.description12 pages, 10 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0611382
dc.identifierhttp://arxiv.org/abs/astro-ph/0611382
dc.identifierPhys.Rev.C74:055804,2006
dc.identifierdoi:10.1103/PhysRevC.74.055804
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/174965
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleNuclear reactions in hot stellar matter and nuclear surface deformation
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