Entropic force, holography and thermodynamics for static space-times
Creators
- 1. Eberhard-Karls University of Tuebingen, Theoretical Astrophysics, Tuebingen (Germany)
Description
Recently Verlinde has suggested a new approach to gravity which interprets gravitational interaction as a kind of entropic force. The new approach uses the holographic principle by stating that the information is kept on the holographic screens which coincide with equipotential surfaces. Motivated by this new interpretation of gravity (but not being limited by it) we study equipotential surfaces, the Unruh-Verlinde temperature, energy and acceleration for various static space-times: generic spherically symmetric solutions, axially symmetric black holes immersed in a magnetic field, traversable spherically symmetric wormholes of an arbitrary shape function, system of two and more extremely charged black holes in equilibrium. In particular, we have shown that the Unruh-Verlinde temperature of the holographic screen reaches absolute zero on the wormhole throat independently of the particular form of the wormhole solution. (orig.)
Availability note (English)
Available from: http://dx.doi.org/10.1140/epjc/s10052-010-1424-1Additional details
Identifiers
Publishing Information
- Journal Title
- European Physical Journal. C
- Journal Volume
- 69
- Journal Issue
- 3-4
- Journal Page Range
- p. 555-562
- ISSN
- 1434-6044
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 42000072
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANALYTICAL SOLUTION; AXIAL SYMMETRY; BLACK HOLES; ENTROPY; FIELD EQUATIONS; GRAVITATION; GRAVITATIONAL INTERACTIONS; HOLOGRAPHY; MAGNETIC FIELDS; METRICS; QUASI PARTICLES; SINGULARITY; SPACE-TIME; TEMPERATURE DISTRIBUTION; THERMAL EQUILIBRIUM; THERMODYNAMICS; THREE-BODY PROBLEM; TWO-BODY PROBLEM
- Descriptors DEC
- BASIC INTERACTIONS; EQUATIONS; EQUILIBRIUM; INTERACTIONS; MANY-BODY PROBLEM; MATHEMATICAL SOLUTIONS; PHYSICAL PROPERTIES; SYMMETRY; THERMODYNAMIC PROPERTIES