Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star

Details Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star

2010-05-11

arxiv.org/abs/1005.1845v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

5pages, 1 table. To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA at

Scientific paper

Based on the steady state equilibrium condition for
neutron-proton-electron-positron gas in the neutrino-driven wind from
protoneutron star, we estimate the initial electron fraction in the wind in a
simple and effective way. We find that the condition in the wind might be
propriate for the r-process nucleosynthesis.

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