New bounds on axion-like particles in the ultraviolet from legacy data

Abstract We use legacy data from the Hubble Space Telescope (HST) and the International Ultraviolet Explorer (IUE) to search for a spectral line from the spontaneous decay of axion-like particle (ALP) dark matter. The HST data consist of blank sky observations taken with the Faint Object Spectrograph in the 165–240 nm wavelength range, while the IUE data consist of observations of the Virgo Cluster obtained with the long- and short-wavelength spectrographs, covering 195–325 nm and 123–200 nm, respectively. We set a 95% C.L. upper limit on the ALP-photon coupling g aγ ≲ 10 -11 GeV -1 across the whole probed ALP mass range. Notably, we rule out values of g aγ above 2.3 × 10 -12 GeV -1 for ALP masses between 12.4 and 14.5 eV, improving upon previous limits by a factor of seven.

Authors

Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2026-04-01
DOI
https://doi.org/10.1088/1475-7516/2026/04/063
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

New bounds on axion-like particles in the ultraviolet from legacy data

Elisa Todarello
Journal of Cosmology and Astroparticle Physics
Dark Matter and Cosmic Phenomena
article

New bounds on axion-like particles in the ultraviolet from legacy data

Elisa Todarello
article en

Abstract

Abstract We use legacy data from the Hubble Space Telescope (HST) and the International Ultraviolet Explorer (IUE) to search for a spectral line from the spontaneous decay of axion-like particle (ALP) dark matter. The HST data consist of blank sky observations taken with the Faint Object Spectrograph in the 165–240 nm wavelength range, while the IUE data consist of observations of the Virgo Cluster obtained with the long- and short-wavelength spectrographs, covering 195–325 nm and 123–200 nm, respectively. We set a 95% C.L. upper limit on the ALP-photon coupling g aγ ≲ 10 -11 GeV -1 across the whole probed ALP mass range. Notably, we rule out values of g aγ above 2.3 × 10 -12 GeV -1 for ALP masses between 12.4 and 14.5 eV, improving upon previous limits by a factor of seven.

Journal of Cosmology and Astroparticle PhysicsVol. 2026(04)
Openalex Percentile: Top 99%
Dark Matter and Cosmic Phenomena
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