ID: hep-th/0501132

The Information Problem in Black Hole Evaporation: Old and Recent Results

January 18, 2005

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Pure states don't wear black

May 24, 1997

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Robert C. Myers
General Relativity and Quant...
High Energy Physics - Theory

Recently, string theory has provided some remarkable new insights into the microphysics of black holes. I argue that a simple and important lesson is also provided with regards to the information loss paradox, namely, pure quantum states do not form black holes! Thus it seems black hole formation, as well as evaporation, must be understood within the framework of quantum decoherence.

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Why Black Hole Information Loss is Paradoxical

October 10, 2017

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David Wallace
General Relativity and Quant...
High Energy Physics - Theory

I distinguish between two versions of the black hole information-loss paradox. The first arises from apparent failure of unitarity on the spacetime of a completely evaporating black hole, which appears to be non-globally-hyperbolic; this is the most commonly discussed version of the paradox in the foundational and semipopular literature, and the case for calling it `paradoxical' is less than compelling. But the second arises from a clash between a fully-statistical-mechanical...

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Black Hole Information

May 10, 1993

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Don N. University of Alberta Page
High Energy Physics - Theory
General Relativity and Quant...

Hawking's 1974 calculation of thermal emission from a classical black hole led to his 1976 proposal that information may be lost from our universe as a pure quantum state collapses gravitationally into a black hole, which then evaporates completely into a mixed state of thermal radiation. Another possibility is that the information is not lost, but is stored in a remnant of the evaporating black hole. A third idea is that the information comes out in nonthermal correlations w...

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Ali Akil, Oscar Dahlsten, Leonardo Modesto
High Energy Physics - Theory
General Relativity and Quant...
Quantum Physics

Hawking's black hole evaporation process suggests that we may need to choose between quantum unitarity and other basic physical principles such as no-signalling, entanglement monogamy, and the equivalence principle. We here provide a quantum model for Hawking pair black hole evaporation within which these principles are all respected. The model does not involve exotic new physics, but rather uses quantum theory and general relativity. The black hole and radiation are in a joi...

Do Black Holes Destroy Information?

September 16, 1992

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John Preskill
High Energy Physics - Theory
General Relativity and Quant...

I review the information loss paradox that was first formulated by Hawking, and discuss possible ways of resolving it. All proposed solutions have serious drawbacks. I conclude that the information loss paradox may well presage a revolution in fundamental physics. (To appear in the proceedings of the International Symposium on Black Holes, Membranes, Wormholes, and Superstrings.)

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Black Holes, Information, and Hilbert Space for Quantum Gravity

October 23, 2012

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Yasunori Nomura, Jaime Varela, Sean J. Weinberg
High Energy Physics - Theory
General Relativity and Quant...

A coarse-grained description for the formation and evaporation of a black hole is given within the framework of a unitary theory of quantum gravity preserving locality, without dropping the information that manifests as macroscopic properties of the state at late times. The resulting picture depends strongly on the reference frame one chooses to describe the process. In one description based on a reference frame in which the reference point stays outside the black hole horizo...

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Control of black hole evaporation?

April 26, 2006

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Doyeol Ahn
High Energy Physics - Theory
General Relativity and Quant...
Quantum Physics

Contradiction between Hawking's semi-classical arguments and string theory on the evaporation of black hole has been one of the most intriguing problems in fundamental physics. A final-state boundary condition inside the black hole was proposed by Horowitz and Maldacena to resolve this contradiction. We point out that original Hawking effect can be also regarded as a separate boundary condition at the event horizon for this scenario. Here, we found that the change of Hawking ...

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Black Hole evaporation: A Perspective from Loop Quantum Gravity

January 23, 2020

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Abhay Ashtekar
Cosmology and Nongalactic As...

A personal perspective on the black hole evaporation process is presented using as guidelines inputs from: (i) loop quantum gravity, (ii) simplified models where concrete results have been obtained, and, (iii) semi-classical quantum general relativity. On the one hand, the final picture is conservative in that there are concrete results that support each stage of the argument, and there are no large departures from general relativity or semi-classical gravity in tame regions ...

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The Black Hole Information Paradox and the Collapse of the Wave Function

June 8, 2014

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E. Okon, D. Sudarsky
General Relativity and Quant...
Quantum Physics

The black hole information paradox arises from an apparent conflict between the Hawking black hole radiation and the fact that time evolution in quantum mechanics is unitary. The trouble is that while the former suggests that information of a system falling into a black hole disappears, the latter implies that information must be conserved. In this work we discuss the current divergence in views regarding the paradox, we evaluate the role that objective collapse theories coul...

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Information paradox and black hole final state for fermions

July 24, 2006

91% Match
Doyeol Ahn
High Energy Physics - Theory
General Relativity and Quant...
Quantum Physics

The black hole information paradox is the result of contradiction between Hawking's semi-classical argument, which dictates that the quantum coherence should be lost during the black hole evaporation and the fundamental principles of quantum mechanics, the evolution of pure states to pure states. For over three decades, this contradiction has been one of the major obstacles to the ultimate unification of quantum mechanics and general relativity. Recently, a final-state bounda...

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