scholarly journals (2 + 1)-dimensional regular black holes with nonlinear electrodynamics sources

2017 ◽  
Vol 774 ◽  
pp. 229-234 ◽  
Author(s):  
Yun He ◽  
Meng-Sen Ma
Keyword(s):  
Black Holes ◽  
Nonlinear Electrodynamics ◽  
Regular Black Holes

scholarly journals Regular black holes inf(T) Gravity through a nonlinear electrodynamics source

2015 ◽  
Vol 2015 (10) ◽  
pp. 060-060 ◽  
Author(s):  
Ednaldo L.B. Junior ◽  
Manuel E. Rodrigues ◽  
Mahouton J.S. Houndjo
Keyword(s):  
Black Holes ◽  
Nonlinear Electrodynamics ◽  
Regular Black Holes

scholarly journals Regular black holes inf(R)gravity coupled to nonlinear electrodynamics

2016 ◽  
Vol 94 (2) ◽  
Author(s):  
Manuel E. Rodrigues ◽  
Ednaldo L. B. Junior ◽  
Glauber T. Marques ◽  
Vilson T. Zanchin
Keyword(s):  
Black Holes ◽  
Nonlinear Electrodynamics ◽  
Regular Black Holes

scholarly journals Publisher’s Note: Regular black holes inf(R)gravity coupled to nonlinear electrodynamics [Phys. Rev. D94, 024062 (2016)]

2016 ◽  
Vol 94 (4) ◽  
Author(s):  
Manuel E. Rodrigues ◽  
Ednaldo L. B. Junior ◽  
Glauber T. Marques ◽  
Vilson T. Zanchin
Keyword(s):  
Black Holes ◽  
Nonlinear Electrodynamics ◽  
Regular Black Holes

scholarly journals Nonpolynomial Lagrangian approach to regular black holes

2018 ◽  
Vol 27 (03) ◽  
pp. 1830002 ◽  
Author(s):  
Aimeric Colléaux ◽  
Stefano Chinaglia ◽  
Sergio Zerbini
Keyword(s):  
Black Holes ◽  
Special Property ◽  
Nonlinear Electrodynamics ◽  
Spherically Symmetric ◽  
Density Profiles ◽  
Regular Black Holes ◽  
Curvature Invariants ◽  
Symmetric Spacetimes ◽  
Central Singularity ◽  
Spherically Symmetric Spacetimes

We present a review on Lagrangian models admitting spherically symmetric regular black holes (RBHs), and cosmological bounce solutions. Nonlinear electrodynamics, nonpolynomial gravity, and fluid approaches are explained in details. They consist respectively in a gauge invariant generalization of the Maxwell–Lagrangian, in modifications of the Einstein–Hilbert action via nonpolynomial curvature invariants, and finally in the reconstruction of density profiles able to cure the central singularity of black holes. The nonpolynomial gravity curvature invariants have the special property to be second-order and polynomial in the metric field, in spherically symmetric spacetimes. Along the way, other models and results are discussed, and some general properties that RBHs should satisfy are mentioned. A covariant Sakharov criterion for the absence of singularities in dynamical spherically symmetric spacetimes is also proposed and checked for some examples of such regular metric fields.

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