Black Hole Criticality in the Brans-Dicke Model

Abstract

We study the collapse of a free scalar field in the Brans-Dicke model of gravity. At the critical point of black hole formation, the model admits two distinctive solutions dependent on the value of the coupling parameter. We find one solution to be discretely self-similar and the other to exhibit continuous self-similarity.

4 pages, REVTeX 3.0, 5 figures included

References in corpus (1)

• S-Duality at the Black Hole Threshold in Gravitational Collapse

Cited by in corpus (29)

• Critical phenomena in gravitational collapse
• Self-Similarity in General Relativity \endtitle
• Critical phenomena in gravitational collapse (Physics Reports)
• Understanding critical collapse of a scalar field
• Breakup of Air Bubbles in Water: Memory and Breakdown of Cylindrical Symmetry
• Phases of massive scalar field collapse
• Black holes in the Brans-Dicke-Maxwell theory
• Critical phenomena in gravitational collapse - Living Reviews
• Rotating Black Branes in Brans-Dicke-Born-Infeld Theory
• Criticality and Bifurcation in the Gravitational Collapse of a Self-Coupled Scalar Field
• Charge scaling and universality in critical collapse
• Critical phenomena in dynamical scalarization of charged black hole
• Adaptive Mesh Refinement for Coupled Elliptic-Hyperbolic Systems
• Dynamical transitions in scalarization and descalarization through black hole accretion
• Gravitational Collapse of Perfect Fluid
• Critical Phenomena in the Einstein-Massless-Dirac System
• Existence of naked singularities in Brans-Dicke theory of gravitation. An analytical and numerical study
• Gravitational collapse of massless scalar field in $f(R)$ gravity
• Instability of an "Approximate Black Hole"
• A New Transition between Discrete and Continuous Self-Similarity in Critical Gravitational Collapse
• Multiply Unstable Black Hole Critical Solutions
• Dynamic generation or removal of a scalar hair
• Dynamics of critical collapse
• Cosmon Lumps and Horizonless Black Holes
• Spherical Self-Similar Solutions in Einstein-Multi-Scalar Gravity
• Unveiling horizons in quantum critical collapse
• Critical Dynamics in Holographic First-Order Phase Transition
• Black Hole Critical Phenomena Without Black Holes
• Self-similar collapse of a scalar field in dilaton gravity and critical behaviour