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Schwarzschild-type black holes in Starobinsky-Bel-Robinson gravity

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arxiv 2209.01574 v3 pith:3A73N46J submitted 2022-09-04 gr-qc hep-th

Ruben Campos Delgado , Sergei V. Ketov This is my paper
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keywords blackschwarzschild-typegravityholestarobinsky-bel-robinsoncomputeconstantcoupling
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We study physical properties of a Schwarzschild-type black hole in the framework of the recently proposed Starobinsky-Bel-Robinson (SBR) modified theory of gravity, working perturbatively in the new coupling constant. In particular, we compute the temperature, entropy, pressure and lifetime of a Schwarzschild-type black hole.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On the stability of de Sitter inflationary solution in the Starobinsky-Bel-Robinson gravity

    gr-qc 2025-07 conditional novelty 2.0 of 10

    The exact de Sitter solution of Starobinsky-Bel-Robinson gravity is fixed by the quartic Bel-Robinson coupling alone and is an unstable saddle point for the physically allowed positive sign of the R^2 coefficient.

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