Dynamic and Thermodynamic Stability of Black Holes and Black Branes

2014 ◽  
pp. 229-238
Author(s):  
Robert M. Wald
Keyword(s):  
Black Holes ◽  
Thermodynamic Stability

scholarly journals Thermodynamic stability of warped AdS3 black holes

2011 ◽  
Vol 697 (1) ◽  
pp. 80-84 ◽  
Author(s):  
Danny Birmingham ◽  
Susan Mokhtari
Keyword(s):  
Black Holes ◽  
Thermodynamic Stability

scholarly journals Thermodynamics of non-commutative scalar-tensor-vector gravity black holes

2020 ◽  
pp. 2150024
Author(s):  
Sara Saghafi ◽  
Kourosh Nozari ◽  
Milad Hajebrahimi
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Coherent State ◽  
Thermodynamic Stability ◽  
Modified Gravity ◽  
Final Stage ◽  
Tunneling Mechanism ◽  
Massive Particles

In this paper, we analyze the thermodynamic stability of Schwarzschild Modified Gravity (MOG) black holes in a non-commutative framework. We show that, unlike a commutative MOG black hole, in the coherent state picture of non-commutativity MOG black holes are thermodynamically stable. At the final stage of evaporation a stable remnant with zero temperatures and finite entropy is left in this non-commutative framework. Also, we consider the Parikh–Wilczek tunneling mechanism of massive particles from non-commutative MOG black holes and demonstrate that information leaks out of non-commutative MOG black holes in the form of some non-thermal correlations.

Revisit on the thermodynamic stability of the noncommutative Schwarzschild black hole

2017 ◽  
Vol 26 (03) ◽  
pp. 1750018 ◽  
Author(s):  
Meng-Sen Ma ◽  
Yan-Song Liu ◽  
Huai-Fan Li
Keyword(s):  
Black Holes ◽  
Heat Capacity ◽  
Black Hole ◽  
Thermodynamic Stability ◽  
Black Hole Thermodynamics ◽  
Positive Temperature ◽  
Schwarzschild Black Hole ◽  
Horizon Thermodynamics ◽  
Thermodynamics Of Black Holes ◽  
Thermodynamic Curvature

In two frameworks, we discuss the thermodynamic stability of noncommutative geometry inspired Schwarzschild black hole (NCSBH). Under the horizon thermodynamics of black holes, we show that the NCSBH cannot be thermodynamically stable if requiring positive temperature. We note the inconsistency in the work of Larrañaga et al. and propose an effective first law of black hole thermodynamics for the NCSBH to eliminate the inconsistency. Based on the effective first law, we recalculate the heat capacity and the thermodynamic curvature by means of geometrothermodynamics (GTD) to revisit the thermodynamic stability.

Thermodynamic stability of pure black holes

1993 ◽  
Vol 10 (7) ◽  
pp. 1323-1339 ◽  
Author(s):  
J Katz ◽  
I Okamoto ◽  
O Kaburaki
Keyword(s):  
Black Holes ◽  
Thermodynamic Stability

Thermodynamic stability of BTZ dilaton black holes

2014 ◽  
Vol 89 (10) ◽  
pp. 105003 ◽  
Author(s):  
A Sheykhi ◽  
S H Hendi ◽  
S Salarpour
Keyword(s):  
Black Holes ◽  
Thermodynamic Stability ◽  
Dilaton Black Holes
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