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• W3034076915 abstract "We study scalar fields in a black hole background and show that, when the scalar is suitably coupled to curvature, rapid rotation can induce a tachyonic instability. This instability, which is the hallmark of spontaneous scalarization in the linearized regime, is expected to be quenched by nonlinearities and endow the black hole with scalar hair. Hence, our results demonstrate the existence of a broad class of theories that share the same stationary black hole solutions with general relativity at low spins, but which exhibit black hole hair at sufficiently high spins ($a/Mensuremath{gtrsim}0.5$). This result has clear implications for tests of general relativity and the nature of black holes with gravitational and electromagnetic observations." @default.
• W3034076915 created "2020-06-12" @default.
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• W3034076915 date "2020-12-01" @default.
• W3034076915 modified "2023-10-16" @default.
• W3034076915 title "Spin-Induced Black Hole Spontaneous Scalarization" @default.
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• W3034076915 doi "https://doi.org/10.1103/physrevlett.125.231101" @default.
• W3034076915 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/33337226" @default.
• W3034076915 hasPublicationYear "2020" @default.
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