Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion
hep-ph, astro-ph.CO, astro-ph.HE
Submitted: 2026-05-14
Updated: 2026-09-21
Comments: 8 pages, 3 figures; Supplemental Material: 7 pages, 4 figures
Journal ref: Phys.Rev.Lett. 137 (2026) 12, 121002
DOI: 10.1103/bqpl-zyr8
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The landscape of QCD axion models
- Cosmology of axion dark matter
- String Axiverse
- The type IIB string axiverse and its low-energy phenomenology
- The Kreuzer-Skarke Axiverse
- On String Theory Expectations for Photon Couplings to Axion-Like Particles
- PQ Axiverse
- Glimmers from the Axiverse
- Experimental Searches for the Axion and Axion-like Particles
- New experimental approaches in the search for axion-like particles
- Invisible Axion Search Methods
- New Technologies for Axion and Dark Photon Searches
- Turbulent axion-photon conversions in the Milky-Way
- Supernova axions convert to gamma-rays in magnetic fields of progenitor stars
- Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
- Stripped-Envelope Supernovae for QCD Axion Detection
- A distance to the Large Magellanic Cloud that is precise to one per cent
- Supernova Simulations Confront SN 1987A Neutrinos
- Searching for the QCD Dark Matter Axion
- Search for Axions in Magnetic White Dwarf Polarization at Lick and Keck Observatories
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