Black hole hair formation in shift-symmetric generalised scalar-tensor gravity

DOI10.1088/1361-6382/aa5ce7zbMath1368.83057arXiv1610.09168OpenAlexW2543725960MaRDI QIDQ5348155

Robert Benkel, Helvi Witek, Thomas P. Sotiriou

Publication date: 14 August 2017

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1610.09168

zbMATH Keywords

collapseblack holesnumericsalternative theories of gravityblack hole hairGauss-Bonnet invariantgeneralised scalar-tensor gravity

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (14)

Existence and instability of hairy black holes in shift-symmetric Horndeski theories ⋮ Extreme gravity tests with gravitational waves from compact binary coalescences. I: Inspiral-merger ⋮ Stability of hairy black holes in shift-symmetric scalar-tensor theories via the effective field theory approach ⋮ On instabilities of stationary scalar field configurations supported by reflecting compact stars ⋮ Dynamics of test particles around hairy black holes in Horndeski's theory ⋮ Dynamic generation or removal of a scalar hair ⋮ Autonomous dynamical system of Einstein-Gauss-Bonnet cosmologies ⋮ Gravitational collapse in Einstein dilaton-Gauss–Bonnet gravity ⋮ Higher dimensional black hole scalarization ⋮ Quasinormal modes of scalar field coupled to Einstein's tensor in the non-commutative geometry inspired black hole ⋮ Spinning black holes in shift-symmetric Horndeski theory ⋮ Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations ⋮ A no-hair theorem for stars in Horndeski theories ⋮ Post-Newtonian gravitational and scalar waves in scalar-Gauss–Bonnet gravity

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