On the gravitational collapse in anti-de Sitter space-time
arXiv:gr-qc/0306002 · doi:10.1016/j.physletb.2003.06.015
Abstract
We study the semiclassical evolution of a self-gravitating thick shell in Anti-de Sitter space-time. We treat the matter on the shell as made of quantized bosons and evaluate the back-reaction of the loss of gravitational energy which is radiated away as a non-adiabatic effect. A peculiar feature of anti-de Sitter is that such an emission also occurs for large shell radius, contrary to the asymptotically flat case.
Changed to Elsevier style, 9 pages, 1 figure. Minor typos corrected. Accepted for publication in Phys. Lett. B
References in corpus (11)
- Gauge Theory Correlators from Non-Critical String Theory
- Vacua, Propagators, and Holographic Probes in AdS/CFT
- Spherically Collapsing Matter in AdS, Holography, and Shellons
- Black Hole Formation in AdS and Thermalization on the Boundary
- Gravitational collapse and its boundary description in AdS
- Charged False Vacuum Bubbles and the AdS/CFT Correspondence
- An Operational Approach To Black Hole Entropy
- Gravitational Collapse of a Shell of Quantized Matter
- Gravitational Collapse of a Radiating Shell
- Effective Action and Thermodynamics of Radiating Shells in General Relativity
- Thermodynamics for radiating shells in anti-de Sitter space-time
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- Cosmological anti-deSitter space-times and time-dependent AdS/CFT correspondence
- Classical dynamics and stability of collapsing thick shells of matter
- Vacuum for a massless quantum scalar field outside a collapsing shell in anti-de Sitter space-time