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Constraining Axions with ZTF J1901+1458

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arxiv 2208.00405 v1 pith:CTN2W62M submitted 2022-07-31 astro-ph.HE astro-ph.SRhep-ph

classification astro-ph.HEastro-ph.SRhep-ph
keywords axionsj1901couplingphotonsproducedtargettextrmaxion-nucleon
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abstract

The axion-nucleon coupling enables the production of axions through the decay of excited ${}^{57}\textrm{Fe}$ isotopes, and axions produced in the Sun through this process are often a target of helioscope searches. We show for the first time that hot, highly magnetic white dwarfs such as ZTF J1901+1458 are a viable target to search for the X-ray signature of axions that were produced by the ${}^{57}\textrm{Fe}$ transition in the core and then converted to photons in the magnetosphere. We calculate that a 100 ks observation of ZTF J1901+1458 with NuSTAR would constrain the coupling of axions to nucleons and photons at a level below the bounds of both current and future planned helioscopes.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Axion lines from nuclear de-excitations in galactic stellar populations

    hep-ph 2025-09 conditional novelty 6.0 of 10

    No 14.4 keV axion line from 57Fe de-excitations is seen by NuSTAR toward M87, M82, M31, or the Galactic Center, yielding |g_ann x g_aγγ| < 1.1e-22 GeV^-1 for m_a < 1e-10 eV.

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