Nucleosynthesis in the Neutrino-Driven Winds from Rotating Proto-Neutron Stars

Details Nucleosynthesis in the Neutrino-Driven Winds from Rotating Proto-Neutron Stars Nucleosynthesis in the Neutrino-Driven Winds from Rotating Proto-Neutron Stars

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..291y&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

Scientific paper

We examine the effects of proto-neutron star rotation on r-process
nucleosynthesis in the neutrino-driven winds. Finding steady,
axisymmetric, rotating wind solutions, we argue the possibility that
such a nucleosynthesis effectively takes place there.

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