The Axion-Electron Coupling from White Dwarf Cooling Set Against DFSZ Scales in the Bounce Frame

The coupling falls from 1.70e-13 at a decay constant of 10^9 GeV to 1.70e-16 at 10^12 GeV. Requiring it to stay below 2.80e-13 forces the decay constant above 6.08e+08 GeV, corresponding to a QCD axion mass below 9.37e+03 micro-electronvolts. These are strong statements about the DFSZ line specifically; a KSVZ axion, whose tree-level electron coupling vanishes, is untouched by them. The bound density of 9.72e+54 g per cubic centimetre appears nowhere in the cooling calculation, whose densest point is the white-dwarf core. This study is computed from stated assumptions and published comparison values; it is not a measurement.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-11
DOI
https://doi.org/10.5281/zenodo.24138661
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

The Axion-Electron Coupling from White Dwarf Cooling Set Against DFSZ Scales in the Bounce Frame

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Dark Matter and Cosmic Phenomena
article

The Axion-Electron Coupling from White Dwarf Cooling Set Against DFSZ Scales in the Bounce Frame

William Alexander Aldred
article en

Abstract

The coupling falls from 1.70e-13 at a decay constant of 10^9 GeV to 1.70e-16 at 10^12 GeV. Requiring it to stay below 2.80e-13 forces the decay constant above 6.08e+08 GeV, corresponding to a QCD axion mass below 9.37e+03 micro-electronvolts. These are strong statements about the DFSZ line specifically; a KSVZ axion, whose tree-level electron coupling vanishes, is untouched by them. The bound density of 9.72e+54 g per cubic centimetre appears nowhere in the cooling calculation, whose densest point is the white-dwarf core. This study is computed from stated assumptions and published comparison values; it is not a measurement.

Zenodo (CERN European Organization for Nuclear Research)
Dark Matter and Cosmic Phenomena
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