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Physics Beyond the Standard Model with Future X-Ray Observatories: Projected Constraints on Very-light Axion-like Particles with Athena and AXIS

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Peer-reviewed

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Abstract

jats:titleAbstract</jats:title> jats:pAxion-like particles (ALPs) are well-motivated extensions of the Standard Model of Particle Physics and a generic prediction of some string theories. X-ray observations of bright active galactic nuclei (AGNs) hosted by rich clusters of galaxies are excellent probes of very-light ALPs, with masses jats:inline-formula jats:tex-math

</jats:tex-math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> mml:milog</mml:mi> <mml:mo stretchy="false">(</mml:mo> mml:msub mml:mrow mml:mim</mml:mi> </mml:mrow> mml:mrow <mml:mi mathvariant="normal">a</mml:mi> </mml:mrow> </mml:msub> mml:mrow <mml:mo stretchy="true">/</mml:mo> </mml:mrow> mml:mieV</mml:mi> <mml:mo stretchy="false">)</mml:mo> mml:mo<</mml:mo> mml:mo−</mml:mo> mml:mn12.0</mml:mn> </mml:math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjacd116ieqn1.gif" xlink:type="simple" /> </jats:inline-formula>. We evaluate the potential of future X-ray observatories, particularly Athena and the proposed AXIS, to constrain ALPs via observations of cluster-hosted AGNs, taking NGC 1275 in the Perseus cluster as our exemplar. Assuming perfect knowledge of the instrument calibration, we show that a modest exposure (200 ks) of NGC 1275 by Athena permits us to exclude all photon–ALP couplings jats:italicg</jats:italic> jats:subajats:italicγ</jats:italic> </jats:sub> > 6.3 × 10jats:sup−14</jats:sup> GeVjats:sup−1</jats:sup> at the 95% confidence level, as previously shown by Conlon et al., representing a factor of 10 improvement over current limits. We then proceed to assess the impact of realistic calibration uncertainties on the Athena projection by applying a standard Cash likelihood procedure, showing the projected constraints on jats:italicg</jats:italic> jats:subajats:italicγ</jats:italic> </jats:sub> weaken by a factor of 10 (back to the current most sensitive constraints). However, we show how the use of a deep neural network can disentangle the energy-dependent features induced by instrumental miscalibration and those induced by photon–ALP mixing, allowing us to recover most of the sensitivity to the ALP physics. In our explicit demonstration, the machine learning applied allows us to exclude jats:italicg</jats:italic> jats:subajats:italicγ</jats:italic> </jats:sub> > 2.0 × 10jats:sup−13</jats:sup> GeVjats:sup−1</jats:sup>, complementing the projected constraints of next-generation ALP dark matter birefringent cavity searches for very-light ALPs. Finally, we show that a 200 ks AXIS/on-axis observation of NGC 1275 will tighten the current best constraints on very-light ALPs by a factor of 3.</jats:p>

Description

Keywords

5106 Nuclear and Plasma Physics, 5107 Particle and High Energy Physics, 51 Physical Sciences

Journal Title

Astrophysical Journal

Conference Name

Journal ISSN

0004-637X
1538-4357

Volume Title

Publisher

American Astronomical Society
Sponsorship
UKRI ∣ Science and Technology Facilities Council (STFC) (ST/V50659X/1)
UKRI ∣ Science and Technology Facilities Council (STFC) (ST/S000623/1)
EC ∣ Horizon 2020 Framework Programme (H2020) (834203)
European Space Agency (ESA) (Individual Fellowship)
Royal Society (The Royal Society) (URF)
Herchel Smith Foundation (Individual Fellowship)
EC ∣ European Research Council (ERC) (742104)
Swedish Research Council (2018-03641)
Swedish Research Council (2019-02337)