Inside spherically symmetric black holes or how a uniformly accelerated particle may slow down

Andrzej Radosz, Pawel Gusin, Andy T. Augousti*, Filip Formalik

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

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.

Original languageEnglish (US)
Article number876
JournalEuropean Physical Journal C
Volume79
Issue number10
DOIs
StatePublished - Oct 1 2019

ASJC Scopus subject areas

  • Engineering (miscellaneous)
  • Physics and Astronomy (miscellaneous)

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