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Recent work by Shenker, Stanford, and Kitaev has related the black hole horizon geometry to chaotic behavior.
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2010
Cited alongside, same era.
2013
Cited alongside, same era.
2013
Cited alongside, same era.
S. H. Shenker and D. Stanford, “Stringy effects in scrambling,” arXiv:1412.6087 [hep-th]
Cited in the paper.
Cited in the paper.
J. Maldacena, S. H. Shenker and D. Stanford, “A bound on chaos,” arXiv:1503.01409 [hep-th]
Cited in the paper.
N. Itzhaki, “Some remarks on ’t Hooft’s S matrix for black holes,” hep-th/9603067; N. Itzhaki, “Is the black hole complementarity principle really necessary?,” hep-th/9607028
Cited in the paper.
Cited in the paper.
2014
Later among the works it cites.
R. Akhoury, “Unitary S Matrices With Long-Range Correlations and the Quantum Black Hole,” JHEP 1408
2014
Later among the works it cites.
A. Kitaev, “Hidden correlations in the Hawking radiation and thermal noise,” Breakthrough Prize Fundamental Physics Symposium 11/10/2014, KITP seminar 2/12/2015; “A simple model of quantum holography (part 1),” KITP seminar 4/7/2015
2015
Closest in time.