R-Process Nucleosynthesis in Neutrino-Driven Wind:. General Relativistic Effects and Short Dynamic Timescale Model

Details R-Process Nucleosynthesis in Neutrino-Driven Wind:. General Relativistic Effects and Short Dynamic Timescale Model R-Process Nucleosynthesis in Neutrino-Driven Wind:. General Relativistic Effects and Short Dynamic Timescale Model

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003omeg.conf..374o&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2000. Proceedings of the International Symposium. Held 19-21 January 2000 in Universi

Astronomy and Astrophysics

Astronomy

Scientific paper

Neutrino-driven wind from young hot neutron star, which is formed by supernova explosion, is the most promising candidate site for r-process nucleosynthesis. We use spherical steady state flow model in general relativistic framework. Exploring wide parameter region which determines the expansion dynamics of the wind, we can find interesting physical conditions which lead to successful r-process nucleosynthesis.

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