https://doi.org/10.1140/epjc/s10052-019-7372-5
Regular Article - Theoretical Physics
Inside spherically symmetric black holes or how a uniformly accelerated particle may slow down
1
Department of Quantum Technologies, Wroclaw University of Science and Technology, Wroclaw, Poland
2
Faculty of Technology and Computer Science, Wroclaw University of Science and Technology, Wroclaw, Poland
3
Faculty of Science, Engineering and Computing, Kingston University London, London, UK
4
Faculty of Chemistry, Wroclaw University of Science and Technology, Wroclaw, Poland
* e-mail: augousti@kingston.ac.uk
Received:
31
May
2019
Accepted:
3
October
2019
Published online:
24
October
2019
Three types of phenomena occurring on both sides of the event horizon of spherically symmetric black holes are analyzed and discussed here. These phenomena are: a light ray orbiting a photon sphere and its analogue, the motion of a uniformly accelerated massive particle and a generalized Doppler effect. The results illustrate how the anisotropic dynamics of the interior of black holes, distinct in the cases both with and without an additional internal horizon, affect non-quantum behaviour.
© The Author(s), 2019
