Lukewarm black holes in quadratic gravity

Abstract

Perturbative solutions to the fourth-order gravity describing spherically-symmetric, static and electrically charged black hole in an asymptotically de Sitter universe is constructed and discussed. Special emphasis is put on the lukewarm configurations, in which the temperature of the event horizon equals the temperature of the cosmological horizon.

References in corpus (9)

• Regular black holes in quadratic gravity
• The Newtonian limit of metric gravity theories with quadratic Lagrangians
• Vacuum polarization for lukewarm black holes
• Higher dimensional black holes with a generalized gravitational action
• Extended Green-Liouville asymptotics and vacuum polarization for lukewarm black holes
• Next-to-leading term of the renormalized stress-energy tensor of the quantized massive scalar field in Schwarzschild spacetime. The back reaction
• Some general properties of the renormalized stress-energy tensor for static quantum states on (n+1)-dimensional spherically symmetric black holes
• Vacuum polarization of the quantized massive scalar field in Reissner-Nordström spacetime
• $Ad{S}_2\times S^2$ geometries and the extreme quantum-corrected black holes

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• Inside the degenerate horizons of regular black holes
• The tetralogy of Birkhoff theorems
• Born-Infeld-de Sitter gravity: Cold, ultracold and Nariai black holes
• Semiclassical lukewarm black holes
• de Sitter field equations from quadratic curvature gravity: A group theoretical approach