D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole
arXiv:1903.05119 · doi:10.1140/epjc/s10052-020-08699-w
Abstract
We study the Vaidya black hole surrounded by the exotic quintessence-like, phantom-like and cosmological constant-like fields by means of entropic considerations. Explicitly, we show that for this thermodynamical system, the requirement for the identification of D-bound and Bekenstein entropy bound can be considered as a thermodynamical criterion by which one can rule out the quintessence-like and phantom-like fields, and prefer the cosmological constant as a viþable cosmological field.
arXiv comment12 pages, minor revision
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