Slowly Rotating Black Holes with Nonlinear Electrodynamics | Zendy

S. H. Hendi | Zendy; Masoud Allahverdizadeh | Zendy

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Slowly Rotating Black Holes with Nonlinear Electrodynamics

Author(s) -

S. H. Hendi,

Masoud Allahverdizadeh

Publication year - 2014

Publication title -

advances in high energy physics

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.59

H-Index - 49

eISSN - 1687-7365

pISSN - 1687-7357

DOI - 10.1155/2014/390101

Subject(s) - physics , nonlinear system , black hole (networking) , horizon , angular momentum , classical mechanics , quantum mechanics , computer science , computer network , routing protocol , routing (electronic design automation) , astronomy , link state routing protocol

We study charged slowly rotating black hole with a nonlinear electrodynamics (NED) in the presence of cosmological constant. Starting from the static solutions of Einstein-NED gravity as seed solutions, we use the angular momentum as the perturbative parameter to obtain slowly rotating black holes. We perform the perturbations up to the linear order for black holes in4 dimensions. These solutions are asymptotically AdS and their horizon has spherical topology. We calculate the physical properties of these black holes and study their dependence on the rotation parameter a as well as the nonlinearity parameter β. In the limit β→∞, the solution describes slowly rotating AdS type black holes

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