Exploring the possibility of testing the no-hair theorem with Minkowski-deformed regular hairy black holes via photon rings

Autor: Xilong Yang, Meirong Tang, Zhaoyi Xu
Jazyk: angličtina
Rok vydání: 2024
Předmět:
Zdroj: European Physical Journal C: Particles and Fields, Vol 84, Iss 9, Pp 1-11 (2024)
Druh dokumentu: article
ISSN: 1434-6052
32528132
DOI: 10.1140/epjc/s10052-024-13343-y
Popis: Abstract In this paper, we investigate the optical appearance of a regular static spherically symmetric hairy black hole within the context of Minkowski deformation governed by the parameter $$\alpha $$ α . This black hole describes a hairy black hole with geometric deformations in the radial and temporal metric components, parameterized by $$\alpha $$ α . The optical appearance of the black hole, illuminated by a static thin accretion disk in three toy emission function models, exhibits distinctive shadows and photon rings. Our findings reveal that for static spherically symmetric hairy Minkowski-deformed regular black holes, the event horizon radius $$r_h$$ r h , photon sphere radius $$r_{ph}$$ r ph , critical impact parameter $$b_{ph}$$ b ph , and innermost stable circular orbit radius $$r_{isco}$$ r isco all have a positive correlation with $$\alpha $$ α . These parameters affect the null geodesic trajectories, shadows, and the optical appearance of the photon rings illuminated by a static thin accretion disk around the black hole. Utilizing this, we obtained the optical appearance of this black hole when observed in the forward direction of the optical and geometric thin accretion disk models. In all three models, the radius of the photon ring images also shows a positive correlation with the parameter $$\alpha $$ α . Therefore, under the static spherically symmetric hairy Minkowski-deformed regular black hole, there is no degeneracy of photon rings dependent on the parameter $$\alpha $$ α . Theoretically, this allows for the distinction of different spacetime metrics of hairy Minkowski-deformed regular black holes, providing a potential method for testing the no-hair theorem through future observations of black hole photon rings.
Databáze: Directory of Open Access Journals
Externí odkaz:
Nepřihlášeným uživatelům se plný text nezobrazuje