Black Hole in Discrete Gravity
arXiv:2311.00406 · doi:10.1140/epjc/s10052-024-12648-2
Abstract
We study the metric corresponding to a three-dimensional coset space in the lattice setting. With the use of three integers , and , and a length scale, , the continuous metric is transformed into a discrete space. The numerical outcomes are compared with the continuous ones. The singularity of the black hole is explored and different domains are studied.
References in corpus (7)
- Black hole formation in the Friedmann universe: Formulation and computation in numerical relativity
- Shadows of spherically symmetric black holes and naked singularities
- Phase Structure of Four Dimensional Simplicial Quantum Gravity
- Tracking Black Holes in Numerical Relativity
- Discrete Gravity
- Scalar Curvature in Discrete Gravity
- Curvature Tensor in Discrete Gravity