Astrophysical weak-interaction processes and nuclear effective field theory

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dc.creatorKubodera, K.
dc.date2004-04-09
dc.date.accessioned2026-07-07T05:40:18Z
dc.date.available2026-07-07T05:40:18Z
dc.descriptionLow-energy nuclear weak-interaction processes play important roles in many astrophysical contexts, and effective field theory is believed to be a highly useful framework for describing these processes in a model-independent manner. I present a brief account of the basic features of the nuclear effective theory approach, and some examples of actual calculations carried out in this method.
dc.description13 pages, Invited talk at the KIAS-APCTP Astro-Hadron Symposium, KIAS, Seoul, Korea, November 10-14, 2003
dc.identifierhttps://arxiv.org/abs/nucl-th/0404027
dc.identifierhttp://arxiv.org/abs/nucl-th/0404027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82210
dc.subjectNuclear Theory
dc.titleAstrophysical weak-interaction processes and nuclear effective field theory
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