Projected bounds on ALPs from Athena
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Publication Date
2018-02Journal Title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN
0035-8711
Volume
473
Issue
4
Pages
4932-4936
Type
Article
Metadata
Show full item recordCitation
Conlon, J. P., Day, F., Jennings, N., Krippendorf, S., & Muia, F. (2018). Projected bounds on ALPs from Athena. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 473 (4), 4932-4936. https://doi.org/10.1093/mnras/stx2652
Abstract
Galaxy clusters represent excellent laboratories to search for axion-like particles (ALPs). They contain magnetic fields which can induce quasi-sinusoidal oscillations in the X-ray spectra of active galactic nuclei situated in or behind them. Due to its excellent energy resolution, the X-ray Integral Field Unit instrument on board the Athena X-ray Observatory will be far more sensitive to ALP-induced modulations than current detectors. As a first analysis of the sensitivity of Athena to the ALP–photon coupling gaγγ, we simulate observations of the Seyfert galaxy NGC 1275 (hosting the radio source 3C 84) in the Perseus cluster using the SIXTE simulation software. We estimate that for a 200 ks exposure, a non-observation of spectral modulations will constrain gaγγ ≲ 1.5 × 10^-13 GeV^-1 for ma ≲ 10− 12 eV, representing an order of magnitude improvement over constraints derived using the current generation of satellites.
Keywords
astroparticle physics, elementary particles, galaxies: clusters: individual: Perseus
Sponsorship
European Research Council
Identifiers
External DOI: https://doi.org/10.1093/mnras/stx2652
This record's URL: https://www.repository.cam.ac.uk/handle/1810/280017
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