Thermonuclear Reaction Rate of 23Mg(p,gamma)24$Al

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dc.creatorHerndl, H.
dc.creatorFantini, M.
dc.creatorIliades, C.
dc.creatorEndt, P. M.
dc.creatorOberhummer, H.
dc.date1998-06-05
dc.date.accessioned2026-07-07T11:11:44Z
dc.date.available2026-07-07T11:11:44Z
dc.descriptionUpdated stellar rates for the reaction 23Mg(p,gamma)24Al are calculated by using all available experimental information on 24Al excitation energies. Proton and gamma-ray partial widths for astrophysically important resonances are derived from shell model calculations. Correspondences of experimentally observed 24Al levels with shell model states are based on application of the isobaric multiplet mass equation. Our new rates suggest that the 23Mg(p,gamma)24Al reaction influences the nucleosynthesis in the mass A>20 region during thermonuclear runaways on massive white dwarfs.
dc.description13 pages (uses Revtex) including 3 postscript figures (uses epsfig.sty), accepted for publication in Phys. Rev. C
dc.identifierhttps://arxiv.org/abs/nucl-th/9806018
dc.identifierhttp://arxiv.org/abs/nucl-th/9806018
dc.identifierPhys.Rev.C58:1798-1803,1998
dc.identifierdoi:10.1103/PhysRevC.58.1798
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191194
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleThermonuclear Reaction Rate of 23Mg(p,gamma)24$Al
dc.typetext

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