Black Hole Scalarization in Gauss-Bonnet Extended Starobinsky Gravity
arXiv:2004.14395 · doi:10.1103/PhysRevD.103.084043
Abstract
We propose a class of higher-derivative gravities that can be viewed as the Gauss-Bonnet extension of the Starobinsky model. The theory admits the Minkowski spacetime vacuum whose linear spectrum consists of the graviton and a massive scalar mode. In addition to the usual Schwarzschild black hole, we use numerical analysis to establish that in some suitable mass range, new black holes carrying the massive scalar hair can emerge. The new black hole serves as a "wall" separating the naked spacetime singularity and wormholes in the parameter space of the scalar hair. Our numerical results also indicate that although the new hairy black hole and the Schwarzschild have different spacetime geometry, their entropy and temperature are same for the same mass.
Latex, 11 pages, reference added
References in corpus (13)
- Massive Gravity in Three Dimensions
- Spontaneously scalarised Kerr black holes
- Black Holes in Higher-Derivative Gravity
- Critical Gravity in Four Dimensions
- A new cubic theory of gravity in five dimensions: Black hole, Birkhoff's theorem and C-function
- Einsteinian cubic gravity
- Self-interactions and Spontaneous Black Hole Scalarization
- Critical Points of D-Dimensional Extended Gravities
- Note on New Massive Gravity in
- Static Solutions for 4th order gravity
- Gauss-Bonnet black holes with a massive scalar field
- Modes of Log Gravity
- Ghosts of Critical Gravity
Cited by in corpus (12)
- Horizon curvature and spacetime structure influences on black hole scalarization
- Dynamical scalarization in Einstein-Maxwell-dilaton theory
- Exact black holes in string-inspired Euler-Heisenberg theory
- Purely metric Horndeski theories and spontaneous curvaturization of black holes
- Dynamics of scalar hair with self-interactions around a Schwarzchild black hole
- Cosmology with Higher-Derivative Gravities
- Gravity with higher-curvature terms and second-order field equations: meets Gauss-Bonnet
- Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability
- Neutron stars more compact than black holes as a probe of strong-field gravity
- Dark Information in Black Hole with Fluid
- Topological Black Holes with curvature induced scalarization in the extended scalar-tensor theories
- Scalarization of Chern-Simons Kerr Black Hole Solutions and Wormholes