Photon paths in the hyperbolic topological black hole spacetime of conformal Weyl gravity
arXiv:1608.02979
Abstract
In this work we find analytical solutions to the null geodesics in the hyperbolic topological black hole spacetime of conformal Weyl gravity in an invariant -plane given by the orbits of an azimuthal Killing vector. Exact expressions for the (non-compact) horizons are found, which depend on the cosmological constant and the coupling constants of conformal Weyl gravity. The angular motion is examined qualitatively by means of an effective potential; quantitatively, the equation of motion is solved in terms of the -Weierstraß elliptic function. Thus, we find the deflection angle for photons without using any approximation, which is a novel result for this topology.
arXiv comment13 pages, 4 figures
References in corpus (10)
- The Contribution of the Cosmological Constant to the Relativistic Bending of Light Revisited
- AdS and Lifshitz Black Holes in Conformal and Einstein-Weyl Gravities
- Classical tests for Weyl gravity: deflection of light and time delay
- Conformal Weyl gravity and perihelion precession
- Cosmological Perturbations in Conformal Gravity
- More on Lensing by a Cosmological Constant
- Light Bending as a Probe of the Nature of Dark Energy
- Exact Static Cylindrical Solution to Conformal Weyl Gravity
- Spherical Structures in Conformal Gravity and its Scalar-Tensor Extension
- Rindler Modified Schwarzschild Geodesics