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

Andrzej Radosz; Pawel Gusin; Andy T. Augousti; Filip Formalik

doi:10.1140/epjc/s10052-019-7372-5

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

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

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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 language	English
Article number	876
Journal	European Physical Journal C (The)
Volume	79
Early online date	24 Oct 2019
DOIs	https://doi.org/10.1140/epjc/s10052-019-7372-5
Publication status	Published - 31 Oct 2019

Keywords

Physics

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10.1140/epjc/s10052-019-7372-5

Augousti-A-44198-VoRFinal published version, 667 KBLicence: CC BY

https://doi.org/10.1140/epjc/s10052-019-7372-5

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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.",

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Y1 - 2019/10/31

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AB - 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.

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DO - 10.1140/epjc/s10052-019-7372-5

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

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