scholarly journals Physical and thermodynamic properties of quartic quasitopological black holes and rotating black branes with a nonlinear source

2019 ◽  
Vol 100 (6) ◽  
Author(s):  
A. Bazrafshan ◽  
F. Naeimipour ◽  
M. Ghanaatian ◽  
A. Khajeh
Keyword(s):  
Black Holes ◽  
Thermodynamic Properties ◽  
Nonlinear Source

scholarly journals Logarithmic corrections of charged hairy black holes in (2 + 1) dimensions

2014 ◽  
Vol 92 (12) ◽  
pp. 1638-1642 ◽  
Author(s):  
J. Sadeghi ◽  
B. Pourhassan ◽  
F. Rahimi
Keyword(s):  
Field Theory ◽  
Black Holes ◽  
Black Hole ◽  
Conformal Field Theory ◽  
Scalar Field ◽  
Thermodynamic Properties ◽  
Conformal Field ◽  
Logarithmic Corrections ◽  
Hairy Black Holes ◽  
Metric Function

We consider a charged black hole with a scalar field that is coupled to gravity in (2 + 1)-dimensions. We compute the logarithmic corrections to the corresponding system using two approaches. In the first method we take advantage of thermodynamic properties. In the second method we use the metric function that is suggested by conformal field theory. Finally, we compare the results of the two approaches.

scholarly journals Solutions and Thermodynamics of Charged Rotating Black Holes in a Fuzzy Space

2013 ◽  
Vol 2013 ◽  
pp. 1-6
Author(s):  
Abderrahman El Boukili ◽  
Mourad Nach ◽  
Hamid Chaqsare ◽  
Moulay Driss Aouragh ◽  
Moulay Brahim Sedra
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Thermodynamic Properties ◽  
Fuzzy Space ◽  
Rotating Black Holes ◽  
Different Types

We investigate the effect of fuzzy space on black hole and its thermodynamic Properties; we also present our results in different types of black holes according to the parameters and representing electric and magnetic charges.

scholarly journals How many universes are necessary for an ice cream to melt?

2003 ◽  
pp. 55-59
Author(s):  
Milan Cirkovic
Keyword(s):  
Black Holes ◽  
Thermodynamic Properties ◽  
Ice Cream ◽  
Arrow Of Time

We investigate a quantitative consequence of the Acausal-Anthropic approach to solving the long-standing puzzle of the thermo dynamical arrow of time. Notably, the size of the required multiverse is estimated on the basis of the classical Boltzmann connection between entropy and probability, as well as the thermodynamic properties of black holes.

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