Asymptotic Schwarzschild solutions in gravity and their observable effects on the photon sphere of black holes
arXiv:2510.00702 · doi:10.1016/j.dark.2025.102189
Abstract
We investigate asymptotic Schwarzschild exterior solutions in the context of modified gravity theories, specifically within the framework of gravity, where the asymptotic behavior recovers the standard Schwarzschild solution of General Relativity. Unlike previous studies that rely mainly on analytical approximations, our approach combines asymptotic analysis with numerical integration of the underlying differential equations. Using these solutions, we analyze strong lensing effects to obtain the photon sphere radius and the corresponding capture parameter. Considering rings produced by total reflection, we define the photon sphere width as the difference between the first total reflection and the capture parameter; and study how it is modified in the scenario. Our results show that the photon sphere width increases in the presence of -type modifications, indicating deviations from GR that could be observable in the strong-field regime.
14 pages, 13 figures
References in corpus (18)
- f(R) Theories Of Gravity
- Modified Gravity and Cosmology
- f(R) theories
- Testing General Relativity with Present and Future Astrophysical Observations
- Testing the nature of dark compact objects: a status report
- Dark Energy vs. Modified Gravity
- Observing the Inner Shadow of a Black Hole: A Direct View of the Event Horizon
- The realistic models of relativistic stars in f(R) = R + alpha R^2 gravity
- On neutron stars in f(R) theories: small radii, large masses and large energy emitted in a merger
- Photon rings of spherically symmetric black holes and robust tests of non-Kerr metrics
- Spherically Symmetric Solutions to Fourth-Order Theories of Gravity
- A new framework for studying spherically symmetric static solutions in f(R) gravity
- The Photon Ring in M87*
- How narrow is the M87* ring? II. A new geometric model
- A new spectral apparent horizon finder for 3D numerical relativity
- Rotating black hole in theory
- Gravity versus astrophysics in black hole images and photon rings: Equatorial emissions and spherically symmetric space-times
- Some exact relativistic star solutions in gravity