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arXiv · 1903.05119

D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole

H. Hadi·F. Darabi·K. Atazadeh·Y. Heydarzade
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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 vi{\th}able cosmological field.

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H. Hadi, F. Darabi, K. Atazadeh, Y. Heydarzade. 2019-03-12. D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole. https://doi.org/10.1140/epjc%2Fs10052-020-08699-w

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