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The information paradox: a pedagogical introduction

Samir D Mathur

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The black hole information paradox is a very poorly understood problem. It is often believed that Hawking's argument is not precisely formulated, and a more careful accounting of naturally occurring quantum corrections will allow the radiation process to become unitary. We show that such is not the case, by proving that small corrections to the leading order Hawking computation cannot remove the entanglement between the radiation and the hole. We formulate Hawking's argument as a 'theorem': assuming 'traditional' physics at the horizon and usual assumptions of locality we will be forced into mixed states or remnants. We also argue that one cannot explain away the problem by invoking AdS/CFT duality. We conclude with recent results on the quantum physics of black holes which show that the interior of black holes have a 'fuzzball' structure. This nontrivial structure of microstates resolves the information paradox and gives a qualitative picture of how classical intuition can break down in black hole physics.


PACS

04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics

03.65.Ud Entanglement and quantum nonlocality (e.g. EPR paradox, Bell's inequalities, GHZ states, etc.)

97.60.Lf Black holes

11.25.Hf Conformal field theory, algebraic structures

04.60.-m Quantum gravity

MSC

83C57 Black holes

Subjects

Gravitation and cosmology

Particle physics and field theory

Quantum information and quantum mechanics

Astrophysics and astroparticles

Dates

Issue 22 (21 November 2009)

Received 1 September 2009

Published 23 October 2009



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