2011
DOI: 10.1142/s0217751x11053924
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Semiclassical Black Holes With Large N Rescaling and Information Loss Problem

Abstract: We consider semi-classical black holes and related re-scalings with N massless fields. For a given semi-classical solution of an N = 1 universe, we can find other solution of a large N universe by the re-scaling. After the re-scaling, any curvature quantity takes a sufficiently small value without changing its causal structure. Via the re-scaling, we argue that black hole complementarity for semi-classical black holes cannot provide a fundamental resolution of the information loss problem, and the violation of… Show more

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Cited by 47 publications
(40 citation statements)
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“…However, the lifetime can be considerably shortened if one considers sufficiently large N number of massless particles -it is of the order M 3 /N . One way to explore the consequence of large number of scalar field is the so-called "large N rescaling" [12] of evaporating black holes, which we will now explain.…”
Section: Jhep12(2014)021mentioning
confidence: 99%
“…However, the lifetime can be considerably shortened if one considers sufficiently large N number of massless particles -it is of the order M 3 /N . One way to explore the consequence of large number of scalar field is the so-called "large N rescaling" [12] of evaporating black holes, which we will now explain.…”
Section: Jhep12(2014)021mentioning
confidence: 99%
“…In addition, we discuss previous arguments that violate black hole complementarity, so-called the large N rescaling [14]. This will make the purpose of this paper clear.…”
Section: Preliminariesmentioning
confidence: 97%
“…then X ′ is also a solution of large N semi-classical equations [14]. Note that it is not welldefined for two dimensional case, which will be discussed in later.…”
Section: Large N Rescaling In Dimensions D >mentioning
confidence: 98%
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