Strongly Coupled Radiation from Moving Mirrors and Holography in the Karch-Randall model
Oriol Pujolas

TL;DR
This paper investigates particle creation by accelerating mirrors modeled as gravitating domain walls in AdS space, comparing weak and strong coupling effects, and providing insights into holography and black hole evaporation.
Contribution
It offers an exact solution for particle production including backreaction at strong coupling in the Karch-Randall holographic model, linking boundary conditions to CFT radiation.
Findings
CFT radiation is not suppressed at strong coupling.
Boundary conditions in AdS_5 match CFT boundary conditions at leading order.
Relativistic cosmic strings in AdS are repulsive and produce tidal forces.
Abstract
Motivated by the puzzles in understanding how Black Holes evaporate into a strongly coupled Conformal Field Theory, we study particle creation by an accelerating mirror. We model the mirror as a gravitating Domain Wall and consider a CFT coupled to it through gravity, in asymptotically Anti de Sitter space. This problem (backreaction included) can be solved exactly at one loop. At strong coupling, this is dual to a Domain Wall localized on the brane in the Karch-Randall model, which can be fully solved as well. Hence, in this case one can see how the particle production is affected by A) strong coupling and B) its own backreaction. We find that A) the amount of CFT radiation at strong coupling is not suppressed relative to the weak coupling result; and B) once the boundary conditions in the AdS_5 bulk are appropriately mapped to the conditions for the CFT on the boundary of AdS_4, the…
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