WEAK CHARGE-CHANGING FLOW IN EXPANDING R-PROCESS ENVIRONMENTS

Citation
Gc. Mclaughlin et Gm. Fuller, WEAK CHARGE-CHANGING FLOW IN EXPANDING R-PROCESS ENVIRONMENTS, The Astrophysical journal, 489(2), 1997, pp. 766-771
Citations number
34
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
489
Issue
2
Year of publication
1997
Part
1
Pages
766 - 771
Database
ISI
SICI code
0004-637X(1997)489:2<766:WCFIER>2.0.ZU;2-1
Abstract
We assess the prospects for attaining steady nuclear-flow equilibrium in expanding r-process environments where beta decay and/or neutrino c apture determine the nuclear charge-changing rates. For very rapid exp ansions, we find that weak steady flow equilibrium normally cannot be attained. However, even when neutron-capture processes freeze out in s uch nonequilibrium conditions, abundance ratios of nuclear species in the r-process peaks might still mimic those attained in weak steady fl ow. This result suggests that the r-process yield in a regime of rapid expansion can be calculated reliably only when all neutron-capture, p hotodisintegration, and weak interaction processes are fully coupled i n a dynamical calculation. We discuss the implications of these result s for models of the r-process sited in rapidly expanding neutrino-heat ed ejecta.