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Accelerating Plasma Mirrors to Investigate the Black Hole Information Loss Paradox

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TLDR
It is pointed out that relativistic plasma mirrors can be accelerated drastically and stopped abruptly by impinging intense x-ray pulses on solid plasma targets with a density gradient, analogous to the late time evolution of black hole Hawking evaporation.
Abstract
The question of whether Hawking evaporation violates unitarity, and therefore results in the loss of information, has remained unresolved since Hawking's seminal discovery. To date, the investigations have remained mostly theoretical since it is almost impossible to settle this paradox through direct astrophysical black hole observations. Here, we point out that relativistic plasma mirrors can be accelerated drastically and stopped abruptly by impinging intense x-ray pulses on solid plasma targets with a density gradient. This is analogous to the late time evolution of black hole Hawking evaporation. A conception of such an experiment is proposed and a self-consistent set of physical parameters is presented. Critical issues, such as how the black hole unitarity may be preserved, can be addressed through the entanglement between the analog Hawking radiation photons and their partner modes.

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Nobel Lecture: Extreme light physics and application

TL;DR: The 2018 Nobel Prize for Physics was shared by Gerard Mourou, Arthur Askin, and Donna Strickland as discussed by the authors, who gave an address given in conjunction with the award.
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Moving mirror model for quasithermal radiation fields

TL;DR: In this article, the authors analyze the flow of energy and entropy emitted by a class of moving mirror trajectories which provide models for important aspects of the radiation fields produced by black hole evaporation.
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On Horizonless Temperature with an Accelerating Mirror

TL;DR: In this article, a new solution of a unitary moving mirror was found to produce finite energy and emit thermal radiation despite the absence of an acceleration horizon, which corresponds to a black hole formed from the collapse of a null shell.
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Effects of Horizons on Entanglement Harvesting

TL;DR: In this paper, the effects of horizons on the entanglement harvested between two Unruh-DeWitt detectors via the use of moving mirrors with and without strict horizons were studied.
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Eternal and evanescent black holes and accelerating mirror analogs

TL;DR: The analogy between black hole radiation and accelerating mirror radiation (the dynamical Casimir effect) is particularly strong for mirror trajectories giving rise to a constant thermal flux of particles as mentioned in this paper.
References
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Quantum Fields in Curved Space

N. D. Birrell, +1 more
TL;DR: A comprehensive review of the subject of gravitational effects in quantum field theory can be found in this paper, where special emphasis is given to the Hawking black hole evaporation effect, and to particle creation processes in the early universe.
Journal ArticleDOI

Black Hole Remnants and the Information Loss Paradox

TL;DR: In this paper, the authors provide a review of various types of black hole remnants, and provide some new thoughts regarding the challenges that black hole survivors face in the context of the information loss paradox and its latest incarnation, namely the firewall controversy.
Journal ArticleDOI

Naked Black Hole Firewalls

TL;DR: If the firewall is located near where the horizon would have been, based on the spacetime evolution up to that time, later quantum fluctuations of the Hawking emission rate can cause the "teleological" event horizon to have migrated to the inside of the firewall location, rendering the firewall naked.

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Posted Content

Quantum Purity at a Small Price: Easing a Black Hole Paradox

TL;DR: In this paper, the effect of collapse space-time geometry on quantum fields in a semi-classical approximation by imposing suitable boundary conditions at the origin of coordinates, which effectively becomes a moving mirror.
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