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Probing axionlike particles through the gamma-ray production from cosmic-ray scattering in the Milky Way dark matter halo

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Author(s):
Goncalves, Victor P. ; Moulin, Emmanuel ; Reis, Igor ; Viana, Aion
Total Authors: 4
Document type: Journal article
Source: PHYSICAL REVIEW D; v. 111, n. 4, p. 10-pg., 2025-02-15.
Abstract

Axionlike particles (ALPs) are promising candidates to comprise all the dark matter in the Universe. We investigate the ALP couplings to photons and electrons via astrophysical measurements through the search for very-high-energy gamma rays arising from high-energy cosmic-ray scattering off ALP populating the halo of the Milky Way. We show that gamma-ray signals from ALP couplings to photons and electrons via inverse Primakoff and Compton processes, respectively, can be probed by very-high-energy (greater than or similar to 100 GeV) gamma-ray ground-based observatories, providing an alternative and complementary avenue to probe ALP couplings in the eV mass range. Sensitivities of current and near-future ground-based gamma-ray observatories improves upon 1 order of magnitude the current constraints from gamma-ray satellite experiments for the ALP-photon couplings in the region of masses below 10-9 GeV. Their sensitivities reached on the ALP-electron couplings allow probing masses below 10-8 GeV, which are lower than the masses probed in gamma-ray satellite experiments. (AU)

FAPESP's process: 19/14893-3 - Extreme phenomena of the Galactic Center and indirect searches of dark matter with gamma rays
Grantee:Aion da Escóssia Melo Viana
Support Opportunities: Research Grants - Young Investigators Grants
FAPESP's process: 21/01089-1 - Cherenkov Telescope Array: construction and first discoveries
Grantee:Luiz Vitor de Souza Filho
Support Opportunities: Special Projects
FAPESP's process: 21/02027-0 - Study of the Galactic Center region and searches for dark matter signals with gamma-rays
Grantee:Igor Reis
Support Opportunities: Scholarships in Brazil - Doctorate (Direct)