Coulomb dissociation, a tool for nuclear astrophysics

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dc.creatorBaur, G.
dc.creatorTypel, S.
dc.date2007-05-23
dc.date2007-08-07
dc.date.accessioned2026-07-07T11:16:17Z
dc.date.available2026-07-07T11:16:17Z
dc.descriptionA short status report on Coulomb dissociation, an indirect method for nuclear astrophysics is given. An analytically solvable approach to study electromagnetic excitation in ^{11}Be, the archetype of a halo nucleus, is proposed.
dc.description6 pages, contribution to Nuclear Physics in Astrophysics III, 26-31 March 2007, Dresden, Germany, typos corrected, accepted for publication in J.Phys. G
dc.identifierhttps://arxiv.org/abs/0705.3307
dc.identifierhttp://arxiv.org/abs/0705.3307
dc.identifierJ.Phys.G35:014003,2008; J.Phys.G35:014028,2008
dc.identifierdoi:10.1088/0954-3899/35/1/014003 10.1088/0954-3899/35/1/014028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192625
dc.subjectNuclear Theory
dc.subjectNuclear Experiment
dc.titleCoulomb dissociation, a tool for nuclear astrophysics
dc.typetext

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