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      Multi-partite analysis of average-subsystem entropies

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          Abstract

          So-called average subsystem entropies are defined by first taking partial traces over some pure state to define density matrices, then calculating the subsystem entropies, and finally averaging over the pure states to define the average subsystem entropies. These quantities are standard tools in quantum information theory, most typically applied in bipartite systems. We shall first present some extensions to the usual bipartite analysis, (including a calculation of the average tangle, and a bound on the average concurrence), follow this with some useful results for tripartite systems, and finally extend the discussion to arbitrary multi-partite systems. A particularly nice feature of tri-partite and multi-partite analyses is that this framework allows one to introduce an "environment" for small subsystems to couple to.

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          Most cited references35

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          Experimental Black-Hole Evaporation?

          W. Unruh (1981)
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            Average Entropy of a Subsystem

            (2010)
            If a quantum system of Hilbert space dimension \(mn\) is in a random pure state, the average entropy of a subsystem of dimension \(m\leq n\) is conjectured to be \(S_{m,n}=\sum_{k=n+1}^{mn}\frac{1}{k}-\frac{m-1}{2n}\) and is shown to be \(\simeq \ln m - \frac{m}{2n}\) for \(1\ll m\leq n\). Thus there is less than one-half unit of information, on average, in the smaller subsystem of a total system in a random pure state.
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              The information paradox: A pedagogical introduction

              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 the 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.
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                Author and article information

                Journal
                31 July 2017
                Article
                1707.09755
                2c836a58-605e-4f3b-8261-71fe4749edd8

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                quant-ph gr-qc hep-th

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