scholarly journals Black Hole Solutions in Gauss-Bonnet-Massive Gravity in the Presence of Power-Maxwell Field

2018 ◽  
Vol 66 (3) ◽  
pp. 1800005 ◽  
Author(s):  
S. H. Hendi ◽  
B. Eslam Panah ◽  
S. Panahiyan
Keyword(s):  
Black Hole ◽  
Massive Gravity ◽  
Maxwell Field ◽  
Black Hole Solutions

scholarly journals Perturbations of cosmological and black hole solutions in massive gravity and bi-gravity

2016 ◽  
Vol 2016 (10) ◽  
pp. 103E02 ◽  
Author(s):  
Tsutomu Kobayashi ◽  
Masaru Siino ◽  
Masahide Yamaguchi ◽  
Daisuke Yoshida
Keyword(s):  
Black Hole ◽  
Massive Gravity ◽  
Black Hole Solutions

scholarly journals Thermodynamics and reentrant phase transition for logarithmic nonlinear charged black holes in massive gravity

2020 ◽  
Vol 29 (12) ◽  
pp. 2050081
Author(s):  
S. Rajaee Chaloshtary ◽  
M. Kord Zangeneh ◽  
S. Hajkhalili ◽  
A. Sheykhi ◽  
S. M. Zebarjad
Keyword(s):  
Phase Transition ◽  
Black Holes ◽  
Black Hole ◽  
Quantum Effect ◽  
Massive Gravity ◽  
Nonlinear Electrodynamics ◽  
Model Parameters ◽  
Thermodynamic Quantities ◽  
Field Equations ◽  
Black Hole Solutions

We investigate a new class of [Formula: see text]-dimensional topological black hole solutions in the context of massive gravity and in the presence of logarithmic nonlinear electrodynamics. Exploring higher-dimensional solutions in massive gravity coupled to nonlinear electrodynamics is motivated by holographic hypothesis as well as string theory. We first construct exact solutions of the field equations and then explore the behavior of the metric functions for different values of the model parameters. We observe that our black holes admit the multi-horizons caused by a quantum effect called anti-evaporation. Next, by calculating the conserved and thermodynamic quantities, we obtain a generalized Smarr formula. We find that the first law of black holes thermodynamics is satisfied on the black hole horizon. We study thermal stability of the obtained solutions in both canonical and grand canonical ensembles. We reveal that depending on the model parameters, our solutions exhibit a rich variety of phase structures. Finally, we explore, for the first time without extending thermodynamics phase space, the critical behavior and reentrant phase transition for black hole solutions in massive gravity theory. We realize that there is a zeroth-order phase transition for a specified range of charge value and the system experiences a large/small/large reentrant phase transition due to the presence of nonlinear electrodynamics.

EXACT SOLUTIONS OF DILATON GRAVITY WITH (ANTI)-DE SITTER ASYMPTOTICS

2014 ◽  
Vol 29 (02) ◽  
pp. 1450010 ◽  
Author(s):  
S. MIGNEMI
Keyword(s):  
Black Hole ◽  
Exact Solutions ◽  
Maxwell Field ◽  
Spherically Symmetric ◽  
Dilaton Gravity ◽  
De Sitter ◽  
Asymptotically Flat ◽  
Black Hole Solutions

We present a technique for obtaining exact spherically symmetric asymptotically de Sitter (dS) or anti-de Sitter (adS) black hole solutions of dilaton gravity with generic coupling to Maxwell field, starting from asymptotically flat solutions and adding a suitable dilaton potential to the action.

scholarly journals Black hole solutions in massive gravity

2009 ◽  
Vol 2009 (04) ◽  
pp. 100-100 ◽  
Author(s):  
Michael V Bebronne ◽  
Peter G Tinyakov
Keyword(s):  
Black Hole ◽  
Massive Gravity ◽  
Black Hole Solutions

scholarly journals Erratum: Black hole solutions in massive gravity

2011 ◽  
Vol 2011 (6) ◽  
Author(s):  
Michael V. Bebronne ◽  
Peter G. Tinyakov
Keyword(s):  
Black Hole ◽  
Massive Gravity ◽  
Black Hole Solutions

scholarly journals ON TOPOLOGICAL CHARGED BRANEWORLD BLACK HOLES

2009 ◽  
Vol 24 (31) ◽  
pp. 2531-2538 ◽  
Author(s):  
AHMAD SHEYKHI ◽  
BIN WANG
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Gauge Field ◽  
Event Horizon ◽  
Extra Dimension ◽  
Weyl Tensor ◽  
Black Hole Thermodynamics ◽  
The Other ◽  
Maxwell Field ◽  
Black Hole Solutions

We study a class of topological black hole solutions in RSII braneworld scenario in the presence of a localized Maxwell field on the brane. Such a black hole can carry two types of charge, one arising from the extra dimension, the tidal charge, and the other from a localized gauge field confined to the brane. We find that the localized charge on the brane modifies the bulk geometry and in particular the bulk Weyl tensor. The bulk geometry does not depend on different topologies of the horizons. We present the temperature and entropy expressions associated with the event horizon of the braneworld black hole and by using the first law of black hole thermodynamics we calculate the mass of the black hole.

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