A Unified Equation for the Reaction Rate in Dense Matter Stars

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dc.contributor.authorGasques , Leandro
dc.contributor.authorWiescher, M.
dc.contributor.authorYakovlev, D.G.
dc.coverage.spatialCusco Peru
dc.date.accessioned2015-12-10T22:23:21Z
dc.date.createdJune 11-16 2007
dc.date.issued2007
dc.date.updated2015-12-09T09:07:06Z
dc.description.abstractWe analyze thermonuclear and pycnonuclear reaction rates in multi-component dense stellar plasma. First we describe calculations of the astrophysical S-factor at low energies using the São Paulo potential on the basis of the barrier penetration model. Th
dc.identifier.isbn9780735404618
dc.identifier.urihttp://hdl.handle.net/1885/52749
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofseriesLatin American Symposium on Nuclear Physics and Applications 2007
dc.sourceAIP Conference Proceedings Volume 947: VII Latin American Symposium on Nuclear Physics and Applications
dc.subjectKeywords: Astrophysical S-factor; Multi-component plasma stellar matter; Reaction rate in different buming regimes
dc.titleA Unified Equation for the Reaction Rate in Dense Matter Stars
dc.typeConference paper
local.bibliographicCitation.lastpage347
local.bibliographicCitation.startpage341
local.contributor.affiliationGasques , Leandro , College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWiescher, M., University of Notre Dame
local.contributor.affiliationYakovlev, D.G., University of Notre Dame
local.contributor.authoremailrepository.admin@anu.edu.au
local.contributor.authoruidGasques , Leandro , u4352530
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020203 - Particle Physics
local.identifier.ariespublicationu4155331xPUB254
local.identifier.doi10.1063/1.2813828
local.identifier.scopusID2-s2.0-36849031150
local.identifier.uidSubmittedByu4155331
local.type.statusPublished Version

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