The r-process in neutrino-driven winds from a typical neutron star with M = 1.4Msolar

Details The r-process in neutrino-driven winds from a typical neutron star with M = 1.4Msolar The r-process in neutrino-driven winds from a typical neutron star with M = 1.4Msolar

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..641t&link_type=abstract

Nuclear Physics A, Volume 718, p. 641-643.

Physics

Nuclear Physics

Scientific paper

We study the effects of the outer boundary conditions in neutrino-driven winds on the r-process nucleosynthesis. Varying the boundary condition, we obtain various asymptotic thermal temperature of expanding material. As a result, we find that the slightly lower asymptotic temperature than those in the previous studies of the neutrino-driven winds can lead to a successful r-process even for the typical proto-neutron star mass MNS 1.4Msolar. We also discuss the relation between the boundary condition and neutron star mass, which is related to the progenitor mass, for the successful r-process

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