A study of nuclei of astrophysical interest in the continuum shell model

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dc.creatorBennaceur, K.
dc.creatorNowacki, F.
dc.creatorOkolowicz, J.
dc.creatorPloszajczak, M.
dc.date1998-02-18
dc.date.accessioned2026-07-07T10:54:46Z
dc.date.available2026-07-07T10:54:46Z
dc.descriptionWe present here the first application of realistic shell model (SM) including coupling between many-particle (quasi-)bound states and the continuum of one-particle scattering states to the spectroscopy of 8B and to the calculation of astrophysical factors in the reaction 7Be(p,gamma)8B.
dc.description9 pages incl. 3 figures, LaTeX with iopart class and epsf. Invited talk at the Int. Workshop on Physics with Radioactive Nuclear Beams, Jan. 12-17, 1998, Puri, India. Shortened version will be published in proceedings to apear as a separate J. Phys. G volume
dc.identifierhttps://arxiv.org/abs/nucl-th/9802054
dc.identifierhttp://arxiv.org/abs/nucl-th/9802054
dc.identifierJ.Phys.G24:1631-1636,1998
dc.identifierdoi:10.1088/0954-3899/24/8/043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185902
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleA study of nuclei of astrophysical interest in the continuum shell model
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