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Vectorial and spinorial perturbations in Galileon Black Holes: Quasinormal modes, quasiresonant modes and stability

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arxiv 1810.01198 v2 pith:OGQRXD3D submitted 2018-10-02 gr-qc hep-th

E. Abdalla , B. Cuadros-Melgar , Jeferson de Oliveira , A. B. Pavan , C. E. Pellicer This is my paper · ORCID
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In this work we have considered a model that includes the interaction of gravity and matter fields with Galilean invariance (the so-called derivative coupling) as well as some corresponding black hole type solutions. Quasinormal perturbations of two kinds of matter fields have been computed by different methods. The effect of the derivative coupling in the quasinormal spectrum has been analyzed and evaluated.

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  1. Strong Cosmic Censorship in Horndeski Theory

    gr-qc 2019-08 conditional novelty 6.0 of 10

    For scalar fields with non-minimal derivative coupling on Reissner-Nordström-de Sitter black holes, strong cosmic censorship is violated only when the ratio β exceeds 3/2 instead of 1/2, and small near-extremal black ...

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