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arXiv · 1005.1845

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

Men-Quan Liu·Ye-Fei Yuan
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Abstract

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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Men-Quan Liu, Ye-Fei Yuan. 2010-05-11. Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star. https://arxiv.org/abs/1005.1845

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