Dilatonic Entropic Force
arXiv:1103.1728 · doi:10.1007/s10773-011-0731-0
Abstract
We show in detail that the entropic force of the static spherically symmetric spacetimes with unusual asymptotics can be calculated through the Verlinde's arguments. We introduce three different holographic screen candidates, which are first employed thoroughly by Myung and Kim [Phys. Rev. D 81, 105012 (2010)] for Schwarzschild black hole solutions, in order to identify the entropic force arising between a charged dilaton black hole and a test particle. The significance of the dilaton parameter on the entropic force is highlighted, and shown graphically.
In v1 the figure was missing; It is fixed; to be appeared in IJTP, 2011
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Cited by in corpus (15)
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- Entangled Particles Tunneling From a Schwarzschild Black Hole immersed in an Electromagnetic Universe with GUP
- The Effect of the Gauss-Bonnet term to Hawking Radiation from arbitrary dimensional Black Brane
- Quantization of rotating linear dilaton black holes
- Entropic force approach to noncommutative Schwarzschild black holes signals a failure of current physical ideas
- de Sitter Swampland Conjecture in String Field Inflation
- Entropic force approach in a noncommutative charged black hole and the equivalence principle
- Absorption Cross-section and Decay Rate of Rotating Linear Dilaton Black Holes
- On a Particular Thin-shell Wormhole
- Hawking Radiation of Mass Generating Particles From Dyonic Reissner Nordström Black Hole
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- Thermodynamical features of Verlinde's approach for a non-commutative Schwarzschild-anti-deSitter black hole in a broad range of scales
- Entropic force law in the presence of a noncommutative inspired spacetime for a solar system scale