An Introduction to Black Holes, Information And The String Theory Revolution: The Holographic Universe

By L. Susskind, J. Lindesay. 2004

418 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/582d3005baef167bbac991f5e7b6abcd3eddfaa6

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. Y. Sekino
2. D. Harlow
3. John McGreevy
4. G. Mack
5. S. Hartnoll
6. L. Susskind
7. D. Stanford
8. Adam R. Brown

In Nuclear and High Energy Physics

1. R. Myers
2. D. Harlow
3. D. Stanford
4. L. Susskind
5. Adam R. Brown
6. S. Hartnoll
7. J. Maldacena
8. T. Takayanagi

Citations in the corpus

• Jerusalem Lectures on Black Holes and Quantum Information (2014, background): “ussed here, some of which are dispersed throughout the literature and some of which are widely known but as far as I know do not appear in print anywhere. The source with the most overlap is probably [3], from which I learned many of the things in the earlier sections of these notes. For some other ”
• Lectures on holographic methods for condensed matter physics (2009, background): “An elegant and robust argument showing that horizons correspond to thermally mixed states can be found, for instance, in chapter 3 of [48].”
• Second law of quantum complexity (2017, background): “[22]) that the total energy of a black hole in Rindler units is proportional to its entropy K we may identify Ea = E ∼ K.”
• Operator Dictionaries and Wave Functions in AdS/CFT and dS/CFT (2011, background): “eems to involve information that cuts across horizons and is inaccesible to any particular observer. In black hole physics such thinking led to many problems, and it seems like it may also do so here [22]. In [7] it was argued { 21 { that precise eld theory duals are only possible when they describe”
• Holographic Duality with a View Toward Many-Body Physics (2009, background): “The loophole in this case is blindingly obvious in retrospect: the graviton needn’t live in the same spacetime as the QFT. 2) Hint number two comes from the Holographic Principle (a good reference is [11]). This is a far-reaching consequence of black hole thermodynamics. The basic fact is that a bla”
• D-independent representation of Conformal Field Theories in D dimensions via transformation to auxiliary Dual Resonance Models. Scalar amplitudes (2009, background): “The leading pole determines the satellites n = 1, 2, 3, ...”
• Fast Scram blers (2008, methodology): “The latter is estimated as follows: In unit Rindler time, approximately one photon will escape from the potential barrier outside the black hole and is emitted as Hawking radiation [10].”