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Scale-invariant rotating black holes in quadratic gravity

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arxiv 1506.07096 v2 pith:L2QSJO6V submitted 2015-06-23 gr-qc

Guido Cognola , Massimiliano Rinaldi , Luciano Vanzo This is my paper · ORCID
classification gr-qc
keywords blackgravityholesquadraticscale-invariantpurerotatingsolutions
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Black hole solutions in pure quadratic theories of gravity are interesting since they allow to formulate a set of scale-invariant thermodynamics laws. Recently, we have proven that static scale-invariant black holes have a well-defined entropy, which characterizes equivalent classes of solutions. In this paper, we generalize these results and explore the thermodynamics of rotating black holes in pure quadratic gravity.

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  1. Critical gravity from four dimensional scale invariant gravity

    hep-th 2019-08 accept novelty 6.0 of 10

    A purely quadratic, scale-invariant gravity action becomes critical when beta equals 6 alpha, turning its massive spin-two ghost into a massless graviton.

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