Comment on The Preprint ``Neutrino Flavor Evolution Near A Supernova's Core'' (Astro-Ph 9405008) by J. Pantaleone
Yong-Zhong Qian, George M. Fuller

TL;DR
This paper critiques a previous preprint on neutrino flavor evolution near supernova cores, identifying errors that invalidate its conclusions about neutrino transformations in such environments.
Contribution
It provides a critical correction to a prior work, clarifying the inaccuracies in the original analysis of neutrino flavor evolution.
Findings
Identified two errors in the previous preprint.
Demonstrated that these errors lead to incorrect conclusions.
Clarified the correct understanding of neutrino flavor transformation.
Abstract
The revised version of the widely circulated preprint ``Neutrino Flavor Evolution Near A Supernova's Core'' by J. Pantaleone (astro-ph 9405008 on the Bulletin Board, Indiana University preprint IUHET-276) is wrong. It contains two errors which lead to incorrect conclusions regarding neutrino flavor transformation in the supernova environment. In this short note we discuss these errors.
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae
