Testing extended theories of gravity via black hole photon rings

As a unique observational feature in strong gravitational fields, photon rings around black holes provide a method to evaluate general relativity and alternative gravity theories. This research delves into the optical characteristics of stationary, spherically symmetric black holes. These black holes follow the Konoplya–Zhidenko deformation rule in arbitrary gravity theories. This black hole is characterized by three independent parameters (ε , ( ε , a₂, a 2 , b₂) b 2 ) to describe its divergence from the Schwarzschild geometry. This paper derives the geodesic equation and effective potential function from the Lagrangian, determines the photon sphere radius (unstable orbit), and analyzes the null geodesics using the reverse ray-tracing technique. This research finds that the effects of a₂ a 2 and b₂ b 2 on photon orbital dynamics exhibit observational degeneracy, while ε ε significantly governs photon capture characteristics. As ε ε increases, the radius of the photon sphere rₚₕ r ph and the critical impact parameter bₚₕ, b ph , and the innermost stable circular orbit radius risco r isco all increase. The event horizon rₕ r h corresponds to that of the Schwarzschild black hole, while the impact parameter range for the lens and photon rings is reduced. Black hole shadow and photon ring analyses across three emission models show that increasing ε ε shifts the peak rightward while enlarging the photon ring radius. The closer ε ε is to zero, the more the results approach the Schwarzschild case, the more the results approach the Schwarzschild case. Additionally, by combining EHT observational data on the shadow diameters of M87 and Sgr A*, we imposed constraints on the correlation parameter ε ε in the theoretical model(at the confidence level anchored by dₛₕ(M87^*), d sh ( M 87 ∗ ) , the parameter ε ε is confined to the interval -0.09 ε 0.19. - 0.09 ≲ ε ≲ 0.19 . For dₛₕ(Sgr A^*), d sh ( S g r A ∗ ) , the constraint on ε ε is delineated as -0.280 ε 0.047). - 0.280 ≲ ε ≲ 0.047 ) . The results show that within the observationally allowed range of ε ε (such as $$[-0.04, 0.04]),$$ [ - 0.04 , 0.04 ] ) , the characteristics of the black hole exhibit specific regularities with changes in ε . ε . In summary, the photon rings of this type of black hole do not exhibit degeneracy, and can theoretically distinguish different spacetime metrics, providing a new approach to constrain extended theories of gravity.