Braneworld Gravity under gravitational decoupling

Abstract

The main objective of this work is to study in some detail the Randall-Sundrum gravity under the gravitational decoupling through the minimal geometric deformation approach (MGD-decoupling). We show a family of new black hole solutions as well as new exact interior solutions for self-gravitating stellar systems and we discuss the corresponding matching conditions.

arXiv comment17 pages, 14 figures

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Cited by in corpus (17)

• Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A${}^{\ast }$
• Hairy black holes by gravitational decoupling
• Gravitational decoupling for axially symmetric systems and rotating black holes
• Stellar models with like--Tolman IV complexity factor
• Ultracompact stars with polynomial complexity by gravitational decoupling
• Gravitational cracking and complexity in the framework of gravitational decoupling
• Anisotropic 2+1 dimensional black holes by gravitational decoupling
• Echoes of the gravitational decoupling: scalar perturbations and quasinormal modes of hairy black holes
• Durgapal IV model in light of the minimal geometric deformation approach
• Geodesic motion around hairy black holes
• Gravitational decoupling, hairy black holes and conformal anomalies
• Quasi Normal Modes of hairy black holes at higher--order WKB approach
• Integration of the Lane-Emden equation for relativistic anisotropic polytropes through Gravitational Decoupling: a novel approach
• A note of the first law of thermodynamics by gravitational decoupling
• Complexity factor of spherically anisotropic polytropes from gravitational decoupling
• A way of decoupling the gravitational bulk field equations of regular braneworld black holes to suppress the bulk singularities
• Braneworld-Klein-Gordon system in the framework of gravitational decoupling