2017
DOI: 10.1007/s10773-017-3501-9
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The Thermodynamic Efficiency in Static and Dynamic Black Holes

Abstract: We note that, in extended phase space the cosmological constant is a thermodynamic variable. In this paper, this cosmological constant lead us to consider a black hole as a heat engine. So, here we take advantage from holographic heat engine and study two kind of different black holes. We first investigate a static black hole (Dyonic BH) and consider the necessary condition to have high efficiency. Also we continue our investigation for dynamic black hole (rotating charged black hole) and study the effect of r… Show more

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Cited by 19 publications
(6 citation statements)
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“…Furthermore, heat engines behaviours of the AdS black holes have been studied. For example, in [38] two kind of heat engines were proposed by Johnson for charged AdS black holes and heat engines were studied for various black hole solutions in [39][40][41][42][43][44][45][46][47][48][49]. 2 More recently, adiabatic processes [53] and Rankine cycle [54] have been studied for the charged AdS black holes.…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, heat engines behaviours of the AdS black holes have been studied. For example, in [38] two kind of heat engines were proposed by Johnson for charged AdS black holes and heat engines were studied for various black hole solutions in [39][40][41][42][43][44][45][46][47][48][49]. 2 More recently, adiabatic processes [53] and Rankine cycle [54] have been studied for the charged AdS black holes.…”
Section: Introductionmentioning
confidence: 99%
“…However, most authors only discuss the case with the horizon being a positive constant curvature hypersurface [9][10][11][12][13][14][15][16][17][18][19][20][21][22]. Note that there are huge differences in the thermal stability of black holes in AdS spaces with different curvatures.…”
Section: Introductionmentioning
confidence: 99%
“…In other words, conditions for existence/non-existence of Meissner effect phase transition is discussed. Phase transition for the Kerr-Newman-AdS black hole in quintessence matter as a model of dark energy is discussed in [17]. Extension of the model including nonlinear magnetic charge is given in [18].…”
Section: Introductionmentioning
confidence: 99%