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Constraints on axionlike particles from 16.5 years of Fermi-LAT data and prospects for VLAST

Zhi-Qi Guo1,2,*, Yue-Lin Sming Tsai2,3,†, Lei Wu1,4,‡, and Zi-Qing Xia2,§

  • *Contact author: zhiqiguo@njnu.edu.cn
  • †Contact author: smingtsai@pmo.ac.cn
  • ‡Contact author: leiwu@njnu.edu.cn
  • §Contact author: xiazq@pmo.ac.cn

Phys. Rev. D 112, 075008 – Published 6 October, 2025

DOI: https://doi.org/10.1103/r7vp-3gv2

Abstract

Axionlike particles (ALPs), hypothetical particles beyond the Standard Model (SM), are considered as promising dark matter candidates. ALPs can convert into photons and vice versa in a magnetic field via the Primakoff effect, potentially generating detectable oscillation in γ-ray spectra. This study analyzes 16.5 years of data from the Fermi Large Area Telescope (Fermi-LAT) on NGC 1275, the brightest galaxy in the Perseus cluster, to constrain the ALP parameter space. Our results improve the previous 95% exclusion limits of the photon-ALP coupling gaγ by a factor of 2 in the ALP mass range of 4×10−10  eV≲ma≲5×10−9  eV. Moreover, we investigate the projected sensitivity of the future Very Large Area γ-ray Space Telescope (VLAST) on searching for ALPs. We find that (i) the expected sensitivity on the photon-ALP coupling gaγ can be stronger than that from the upcoming International Axion Observatory in the ALP mass range of 2×10−11  eV≲ma≲1×10−7  eV, with the best sensitivity of gaγ∼7×10−13  GeV−1 at ma∼2×10−10  eV; (ii) VLAST can extend the sensitivity of the ALP masses below 5×10−12  eV, where the photon-ALP coupling gaγ≳1.5×10−11  GeV−1 will be excluded; (iii) the entire parameter space of ALP accounting for TeV transparency can be fully tested. These results demonstrate that VLAST will offer an excellent opportunity for ALPs searches.

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