Role of complexity on the minimal deformation of black holes

DOI10.1088/1361-6382/AD6389zbMATH Open1546.83078MaRDI QIDQ6584887

M. Z. Bhatti, Kazuharu Bamba, Author name not available (Why is that?), Bander Almutairi, Author name not available (Why is that?)

Publication date: 8 August 2024

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

zbMATH Keywords

compact objectsgravitational decouplingKarmarkar conditioncomplexity factor

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Cites Work

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• Insufficiency of Karmarkar's condition
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• Generalised uncertainty principle Hawking fermions from minimally geometric deformed black holes
• The minimal geometric deformation approach extended
• Anisotropic stars in general relativity
• General relativistic boson stars
• Brane-world stars with a solid crust and vacuum exterior
• Gravitational instability of polytropic spheres containing region of trapped null geodesics: a possible explanation of central supermassive black holes in galactic halos
• NONUNIFORM BRANEWORLD STARS: AN EXACT SOLUTION
• Black strings from minimal geometric deformation in a variable tension brane-world
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• Stability Analysis of Isotropic Spheres in Einstein Gauss–Bonnet Gravity

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