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QCD Axion Star Collapse with the Chiral Potential

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arxiv 1702.05504 v1 pith:7KLPXIJF submitted 2017-02-17 hep-ph

Joshua Eby , Madelyn Leembruggen , Peter Suranyi , L.C.R. Wijewardhana This is my paper · ORCID
classification hep-ph
keywords axionpotentialchiralcollapsingstarsalwaysanalyzedaxions
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In a previous work, we analyzed collapsing axion stars using the low-energy instanton potential, showing that the total energy is always bounded and that collapsing axion stars do not form black holes. In this paper, we provide a proof that the conclusions are unchanged when using instead the more general chiral potential for QCD axions.

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  1. Properties of QCD axion in two-flavor color superconductive matter with massive quarks

    hep-ph 2025-01 conditional novelty 6.0 of 10

    In a two-flavor NJL model with chiral and diquark condensates, the axion mass and quartic coupling increase at the chiral phase transition when color superconductivity is present.

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