0000000000088417

AUTHOR

Gérard Clément

showing 3 related works from this author

An alternative scenario for critical scalar field collapse in $AdS_3$

2016

In the context of gravitational collapse and black hole formation, we reconsider the problem to describe analytically the critical collapse of a massless and minimally coupled scalar field in $2+1$ gravity.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Particle physicsBlack HolesCritical phenomenaAstrophysics::High Energy Astrophysical PhenomenaCollapse (topology)FOS: Physical sciencesContext (language use)Critical collapseGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesGravitational collapse010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsMassless particle2+1 gravityHigh Energy Physics - Theory (hep-th)Anti-de Sitter spaceScalar field
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Comment on `Critical scalar field collapse in AdS$_3$: an analytical approach'

2014

We comment on the derivation of an analytical solution presented in arXiv:1309.1629, show that it belongs to a family of separable solutions previously constructed in arXiv:gr-qc/0109002, and question its relevance to critical collapse.

High Energy Physics - TheoryPhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsCollapse (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologySeparable spaceTheoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010306 general physicsScalar field
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A scenario for critical scalar field collapse in $AdS_3$

2014

We present a family of exact solutions, depending on two parameters $\alpha$ and $b$ (related to the scalar field strength), to the three-dimensional Einstein-scalar field equations with negative cosmological constant $\Lambda$. For $b=0$ these solutions reduce to the static BTZ family of vacuum solutions, with mass $M = -\alpha$. For $b\neq0$, the solutions become dynamical and develop a strong spacelike central singularity. The $\alpha0$ agrees qualitatively with that observed in numerical simulations of subcritical collapse. We analyze the linear perturbations of the threshold solution, $\alpha=0$, in the $\Lambda=0$ approximation, and find that it has only one unstable growing mode, whi…

PhysicsHigh Energy Physics - Theory[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Physics and Astronomy (miscellaneous)SpacetimeFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyEffective mass (solid-state physics)SingularityHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Field equationGlobal structureScalar fieldMathematical physics
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