Published October 2019 | Version v1
Journal article Metadata-only

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

Creators

  • 1. Department of Quantum Technologies, Wroclaw University of Science and Technology (Poland)
  • 2. Faculty of Technology and Computer Science, Wroclaw University of Science and Technology (Poland)
  • 3. Faculty of Science, Engineering and Computing, Kingston University London (United Kingdom)
  • 4. Faculty of Chemistry, Wroclaw University of Science and Technology (Poland)

Description

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.

Availability note (English)

Available from: http://dx.doi.org/10.1140/epjc/s10052-019-7372-5

Additional details

Identifiers

DOI
10.1140/epjc/s10052-019-7372-5;

Publishing Information

Journal Title
European Physical Journal. C, Particles and Fields (Online)
Journal Volume
79
Journal Issue
10
Journal Page Range
p. 1-10
ISSN
1434-6052

INIS

Country of Publication
Germany
Country of Input or Organization
Germany
INIS RN
51036340
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ACCELERATION; ANISOTROPY; ANTI DE SITTER SPACE; BLACK HOLES; CENTRAL POTENTIAL; DOPPLER EFFECT; ELECTROMAGNETIC RADIATION; GEODESICS; ORBITS; PHOTONS; REST MASS; SCHWARZSCHILD METRIC; SPACE-TIME; TRAJECTORIES; WAVE PROPAGATION
Descriptors DEC
BOSONS; ELEMENTARY PARTICLES; MASS; MASSLESS PARTICLES; MATHEMATICAL SPACE; METRICS; POTENTIALS; RADIATIONS; SPACE

Optional Information

Notes
AID: 876