1997
DOI: 10.1002/(sici)1099-0526(199709/10)3:1<36::aid-cplx11>3.0.co;2-x
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Complexity in quantum gravity
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Cited by 9 publications
(8 citation statements)
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“…One lesson we are learning is that the solitons and instantons are no less holographic [ 16 ] than black holes. Our observations indicate that saturation of the entropy bound and its area‐form go well beyond gravity and are defined by fundamental aspects of quantum field theory such as unitarity and asymptotic freedom.…”
Section: Discussionmentioning
confidence: 99%
“…One lesson we are learning is that the solitons and instantons are no less holographic [ 16 ] than black holes. Our observations indicate that saturation of the entropy bound and its area‐form go well beyond gravity and are defined by fundamental aspects of quantum field theory such as unitarity and asymptotic freedom.…”
Section: Discussionmentioning
confidence: 99%
“…This is a satisfying conclusion because the naive picture of two dimensional string theory appears to violate Bekenstein's entropy bound. There is no longer an obvious counterargument to the claim that string theory is a holographic theory [6].…”
Section: Discussionmentioning
confidence: 99%
“…The application of Bekenstein's bound to sufficiently small regions of the Universe can be found in [23][24][25][26][27][28][29]. Moreover, Fischler and Susskind have proposed a bound [24] which can formulate the holographic principle [30][31][32]. They have carefully exposed the difficulties that arise when such bounds are pushed beyond their range of validity [24,25,28].…”
mentioning
confidence: 99%
