Probing Axions with Event Horizon Telescope Polarimetric Measurements
Résumé
With high spatial resolution, polarimetric imaging of a supermassive black hole, like M87⋆ or Sgr A⋆, by the Event Horizon Telescope can be used to probe the existence of ultralight bosonic particles, such as axions. Such particles can accumulate around a rotating black hole through the superradiance mechanism, forming an axion cloud. When linearly polarized photons are emitted from an accretion disk near the horizon, their position angles oscillate due to the birefringent effect when traveling through the axion background. In particular, the observations of supermassive black holes M87⋆ (Sgr A⋆) can probe the dimensionless axion-photon coupling c=2πgaγfa for axions with mass around O(10-20) eV [O(10-17) eV] and decay constant fa
INSPIRE HEP : Connectez-vous pour contacter le contributeur
https://hal.science/hal-02144328
Soumis le : jeudi 30 mai 2019-01:28:13
Dernière modification le : samedi 16 mars 2024-10:36:06
Dates et versions
Identifiants
- HAL Id : hal-02144328 , version 1
- ARXIV : 1905.02213
- DOI : 10.1103/PhysRevLett.124.061102
- INSPIRE : 1733706
Citer
Yifan Chen, Jing Shu, Xiao Xue, Qiang Yuan, Yue Zhao. Probing Axions with Event Horizon Telescope Polarimetric Measurements. Physical Review Letters, 2020, 124 (6), pp.061102. ⟨10.1103/PhysRevLett.124.061102⟩. ⟨hal-02144328⟩
Collections
86
Consultations
0
Téléchargements