Generalized Einstein-Rosen bridge inside black holes
arXiv:2312.15870 · doi:10.31857/S0044451024060063
Abstract
We generalize the notion of Einstein-Rosen bridge by defining it as a space-like connection between two universes with regions of asymptotically minkowskian space-time infinities. The corresponding symmetry and asymmetry properties of the generalized Einstein-Rosen bridge are considered at the cases of Reissner-Nordström and Kerr metrics. We elucidate the versatility of intriguing symmetry and asymmetry phenomena outside and inside black holes. For description of the test particle (planet and photon) motion it is used the Kerr-Newman metric of the rotating and electrically charged black hole. In particular, it is demonstrated the symmetry and asymmetry of the one-way Einstein-Rosen bridge inside black hole toward and through the plethora of endless and infinite universes.
9 pages, 7 figures, corrected typos, published version
References in corpus (4)
- Geodesics of electrically and magnetically charged test particles in the Reissner-Nordström space-time: analytical solutions
- Analytic treatment of complete and incomplete geodesics in Taub-NUT space-times
- Event horizon silhouette: implications to supermassive black holes M87* and SgrA*
- Examining the Kerr Metric through Wave Fronts of Null Geodesics