2010
DOI: 10.48550/arxiv.1006.4090
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Holographic Evolution of Entanglement Entropy

Javier Abajo-Arrastia,
Joao Aparicio,
Esperanza Lopez
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Cited by 112 publications
(246 citation statements)
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“…Finally, let us compare our results for two-point functions of a massless scalar field with light-like separation to previous discussions of space-like separation, for instance those of [36,37,21]. There it was pointed out that for large masses, or alternatively for large conformal dimension, the correlator is dominated by the contribution of the space-like geodesic joining the two points.…”
Section: Discussionsupporting
confidence: 58%
See 1 more Smart Citation
“…Finally, let us compare our results for two-point functions of a massless scalar field with light-like separation to previous discussions of space-like separation, for instance those of [36,37,21]. There it was pointed out that for large masses, or alternatively for large conformal dimension, the correlator is dominated by the contribution of the space-like geodesic joining the two points.…”
Section: Discussionsupporting
confidence: 58%
“…At a late stage, the numerical results match with the analytical solutions based on an asymptotic expansion [19,20]. An interesting link between the thin shell and perturbative approaches described above has recently been established in [21,22,23]. The evolutions of entanglement entropy in d = 2 and d = 3 have been studied in a Vaidya metric describing a collapsing shell in the formation of a black hole.…”
Section: Introductionsupporting
confidence: 55%
“…We would also like to mention that quite recently, remarkable numerical calculations of time evolutions of entanglement entropy have been done holographically in [23,24]. When we essentially finished calculations for this paper, we found the paper [23], which has a partial but important overlap with ours about the argument which shows unitary evolutions of CFTs dual to the black hole formations by using the holographic entanglement entropy. A similar issue has also been discussed independently in the appendix of the paper [24].…”
Section: Introductionmentioning
confidence: 82%
“…1. This is realized in the charged time-dependent Vaidya black brane [32][33][34][35] with the solution…”
Section: Holographic Modelmentioning
confidence: 99%
“…The model is based on a time-dependent charged black brane spacetime in Einstein-Maxwell theory coupled to time-dependent external sources illustrated in Fig. 1 [32][33][34][35]. The infall of matter causes the mass of the black brane to increase rapidly, corresponding to a change of the temperature and the entropy density in the dual field theory.…”
Section: Introductionmentioning
confidence: 99%