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Gravitational cracking and complexity in the framework of gravitational decoupling

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arxiv 2107.01140 v1 pith:PPI2HWZF submitted 2021-07-02 gr-qc

E. Contreras , E. Fuenmayor This is my paper · ORCID
classification gr-qc
keywords gravitationalcrackingdecouplingcomplexityeffectframeworkanalyseanisotropic
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In this work we analyse the stability of self gravitating spheres in the context of gravitational cracking. Besides exploring the role played by the anisotropy in the occurrence of cracking, we also study the effect of the complexity factor recently introduced by L. Herrera in Phys. Rev. D 97, 044010 (2018). The models under study correspond to anisotropic solutions obtained in the framework of the Gravitational Decoupling. The effect that the variation of the decoupling parameter and the compactness of the source have on the behaviour of the radial force is studied in detail.

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  1. Gravitational decoupling and regular hairy black holes: Geodesic stability, quasinormal modes, and thermodynamic properties

    gr-qc 2025-12 conditional novelty 4.0 of 10

    For the regular hairy black hole metric (29), larger β shrinks the ISCO and photon sphere, reduces QNM damping, and adds a canonical-ensemble stable phase.

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