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Response to Comments on "Neutrino Flavor Evolution Near a Supernova's Core"

J. Pantaleone
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Abstract

In a recent paper I concluded that the neutrino background is important for calculating neutrino flavor evolution in supernovae, and including it weakens the connection between r-process nucleosynthesis and cosmologically relevant neutrino masses. Comments on this paper have been posted to this bulletin board; one by J. Cline and the other by Y.Z. Qian and G.M. Fuller. Here I briefly discuss these Comments and demonstrate that they are inaccurate and ill-considered. No corrections to my paper are necessary.

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J. Pantaleone. 1994-08-01. Response to Comments on "Neutrino Flavor Evolution Near a Supernova's Core". https://arxiv.org/abs/astro-ph/9408006

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