Spin-induced scalarization of Kerr-Newman black holes in Einstein-Maxwell-scalar theory
arXiv:2206.11587 · doi:10.1103/PhysRevD.106.044045
Abstract
In this paper, we consider the tachyonic instability of Kerr-Newman (KN) black holes in the Einstein-Maxwell-scalar (EMS) theory with nonminimal negative scalar coupling to Maxwell term, and then obtain a bound for spin parameter of KN black hole in the limit of coupling constant by using analytical method. In addition, we perform a -dimensional time evolution of linearized scalar field perturbation on the KN black hole background by implementing the hyperboloidal foliation method numerically in the EMS theory. It recovers the \textit{spontaneous scalarization} phenomenon for KN black hole in some certain regions of the parameter spaces. We further plot corresponding threshold curves which describe a boundary between bald KN black holes and scalarized spinning black holes in the EMS theory.
arXiv comment23 pages, 6 figures
References in corpus (30)
- Spontaneous scalarization of black holes and compact stars from a Gauss-Bonnet coupling
- New Gauss-Bonnet black holes with curvature induced scalarization in the extended scalar-tensor theories
- Evasion of No-Hair Theorems and Novel Black-Hole Solutions in Gauss-Bonnet Theories
- Spontaneous scalarisation of charged black holes
- Spontaneously scalarised Kerr black holes
- Spin-induced scalarized black holes
- Spin-induced black hole spontaneous scalarization
- Spin-induced black hole scalarization in Einstein-scalar-Gauss-Bonnet theory
- Spontaneous scalarisation of charged black holes: coupling dependence and dynamical features
- Hyperboloidal foliations and scri-fixing
- Spinning and excited black holes in Einstein-scalar-Gauss-Bonnet theory
- Instability of Reissner-Nordström black hole in Einstein-Maxwell-scalar theory
- Linear mode stability of Kerr-Newman and its quasinormal modes
- A new gravitational wave generation algorithm for particle perturbations of the Kerr spacetime
- Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality
- Null infinity waveforms from extreme-mass-ratio inspirals in Kerr spacetime
- Black hole scalarization induced by the spin -- 2+1 time evolution
- Onset of spontaneous scalarization in spinning Gauss-Bonnet black holes
- Hyperboloidal layers for hyperbolic equations on unbounded domains
- Numerical solution of the 2+1 Teukolsky equation on a hyperboloidal and horizon penetrating foliation of Kerr and application to late-time decays
- Numerical integration of the Teukolsky Equation in the time domain
- Numerical investigation of the late-time Kerr tails
- Scalar perturbations on the background of Kerr black holes in the quadratic dynamical Chern-Simons gravity
- Onset of rotating scalarized black holes in Einstein-Chern-Simons-Scalar theory
- Spin-induced scalarization of Kerr black holes with a massive scalar field
- Object picture of scalar field perturbation on Kerr black hole in scalar-Einstein-Gauss-Bonnet theory
- Numerical investigation of plasma-driven superradiant instabilities
- Massive scalar field perturbation on Kerr black holes in dynamical Chern-Simons gravity
- Scalar Fields in Black Hole Spacetimes
- Rotating scalarized black holes in scalar couplings to two topological terms