Non-equilibrium thermodynamics of dark energy on the power-law entropy corrected apparent horizon
arXiv:1111.6510 · doi:10.1139/p11-126
Abstract
We investigate the Friedmann-Robertson-Walker (FRW) universe (containing dark energy) as a non-equilibrium (irreversible) thermodynamical system by considering the power-law correction to the horizon entropy. By taking power-law entropy area law which appear in dealing with the entanglement of quantum fields in and out the horizon, we determine the power-law entropy corrected apparent horizon of the FRW universe.
9 pages, online first at Canadian Journal of Physics
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Cited by in corpus (5)
- Generalized Second Law of Thermodynamics for FRW Cosmology with Power-Law Entropy Correction
- Thermodynamics of a Schwarzschild Black Hole in Phantom Cosmology with Entropy Corrections
- Will there be future deceleration? A study of particle creation mechanism in non-equilibrium thermodynamics
- Thermodynamics of an Evolving Lorentzian Wormhole with Entropy Corrections
- Thermodynamics of the most generalized form of Holographic Dark Energy and some particular cases with Corrected Entropies