Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87

We perform one of the most sensitive searches to date for the existence of ultralight axions using data from the NuSTAR telescope. We search for stellar axion production in the M82 starburst galaxy and the M87 central galaxy of the Virgo cluster and then the subsequent conversion into hard x-rays in the surrounding magnetic fields. We sum over the full stellar populations in these galaxies when computing the axion luminosity, and we account for the conversion of axions to photons by using magnetic field profiles in simulated IllustrisTNG analog galaxies. We show that analyzing NuSTAR data toward these targets between roughly 30 and 70 keV shows no evidence for axions and leads to robust constraints on the axion-photon coupling at the level of |g_{aγγ}|≲7.8×10^{-13} GeV^{-1} for m_{a}≲10^{-10} eV at 95% confidence.

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Publication Details

Journal
Physical Review Letters
Published
2025-05-01
DOI
https://doi.org/10.1103/physrevlett.134.171003
Citations
16
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
29.92

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article

Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87

Orion Ning, Benjamin R. Safdi
16 citations
Physical Review Letters
Dark Matter and Cosmic Phenomena
29.92
article

Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87

Orion Ning, Benjamin R. Safdi
article en
16 citations

Abstract

We perform one of the most sensitive searches to date for the existence of ultralight axions using data from the NuSTAR telescope. We search for stellar axion production in the M82 starburst galaxy and the M87 central galaxy of the Virgo cluster and then the subsequent conversion into hard x-rays in the surrounding magnetic fields. We sum over the full stellar populations in these galaxies when computing the axion luminosity, and we account for the conversion of axions to photons by using magnetic field profiles in simulated IllustrisTNG analog galaxies. We show that analyzing NuSTAR data toward these targets between roughly 30 and 70 keV shows no evidence for axions and leads to robust constraints on the axion-photon coupling at the level of |g_{aγγ}|≲7.8×10^{-13} GeV^{-1} for m_{a}≲10^{-10} eV at 95% confidence.

Physical Review LettersVol. 134(17)
Lawrence Berkeley National Laboratory (US), University of California System (US)
National Science Foundation, U.S. Department of Energy, National Energy Research Scientific Computing Center, Office of Science, Lawrence Berkeley National Laboratory
Openalex Percentile: Top 0%
Dark Matter and Cosmic Phenomena
29.92
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