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Braneworld Gravity under gravitational decoupling
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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.
Forward citations
Cited by 2 Pith papers
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Isotropization and change of complexity by gravitational decoupling
A gravitational decoupling technique that continuously isotropizes anisotropic stellar solutions and generates new solutions with controlled complexity factor, demonstrated on two exact examples.
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Minimal Geometric Deformation in a Reissner-Nordstr\"om background
New exact Reissner-Nordström black hole solutions are built via minimal geometric deformation with a linear equation of state in the added source.
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