E0 emission in alpha + ^12C fusion at astrophysical energies

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dc.creatorBaur, G.
dc.creatorSnover, K. A.
dc.creatorTypel, S.
dc.date2007-01-10
dc.date2007-03-28
dc.date.accessioned2026-07-07T10:22:42Z
dc.date.available2026-07-07T10:22:42Z
dc.descriptionWe show that E0 emission in alpha + ^12C fusion at astrophysically interesting energies is negligible compared to E1 and E2 emission.
dc.descriptionsubmitted to Phys. Rev. C, Brief Reports
dc.identifierhttps://arxiv.org/abs/nucl-th/0701027
dc.identifierhttp://arxiv.org/abs/nucl-th/0701027
dc.identifierPhys.Rev.C75:058801,2007
dc.identifierdoi:10.1103/PhysRevC.75.058801
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175604
dc.subjectNuclear Theory
dc.subjectNuclear Experiment
dc.titleE0 emission in alpha + ^12C fusion at astrophysical energies
dc.typetext

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