White dwarfs as a probe of exceptionally light QCD axions

Fuente: arXiv
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Main Authors: Balkin, Reuven, Serra, Javi, Springmann, Konstantin, Stelzl, Stefan, Weiler, Andreas
Format: Preprint
Published: 2022
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author Balkin, Reuven
Serra, Javi
Springmann, Konstantin
Stelzl, Stefan
Weiler, Andreas
author_facet Balkin, Reuven
Serra, Javi
Springmann, Konstantin
Stelzl, Stefan
Weiler, Andreas
contents We study the effects of exceptionally light QCD axions on the stellar configuration of white dwarfs. At finite baryon density, the non-derivative coupling of the axion to nucleons displaces the axion from its in-vacuum minimum which implies a reduction of the nucleon mass. This dramatically alters the composition of stellar remnants. In particular, the modifications of the mass-radius relationship of white dwarfs allow us to probe large regions of unexplored parameter space without requiring that axions are dark matter.
format Preprint
id arxiv_https___arxiv_org_abs_2211_02661
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle White dwarfs as a probe of exceptionally light QCD axions
Balkin, Reuven
Serra, Javi
Springmann, Konstantin
Stelzl, Stefan
Weiler, Andreas
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
We study the effects of exceptionally light QCD axions on the stellar configuration of white dwarfs. At finite baryon density, the non-derivative coupling of the axion to nucleons displaces the axion from its in-vacuum minimum which implies a reduction of the nucleon mass. This dramatically alters the composition of stellar remnants. In particular, the modifications of the mass-radius relationship of white dwarfs allow us to probe large regions of unexplored parameter space without requiring that axions are dark matter.
title White dwarfs as a probe of exceptionally light QCD axions
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2211.02661