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Volumn 112, Issue 1, 2014, Pages

Entanglement tsunami: Universal scaling in holographic thermalization

Author keywords

[No Author keywords available]

Indexed keywords

CONTINUOUS PHASE TRANSITIONS; CRITICAL BEHAVIOR; ENTANGLEMENT ENTROPY; GRAVITATIONAL COLLAPSE; HOLOGRAPHIC SYSTEM; RELATIVISTIC SYSTEMS; SATURATION REGIME; UNIVERSAL SCALING;

EID: 84892378290     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.112.011601     Document Type: Article
Times cited : (456)

References (26)
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    • With a RN black hole, at fixed Q and sufficiently large R, the linear regime does not appear to extend all the way to saturation.
    • With a RN black hole, at fixed Q and sufficiently large R, the linear regime does not appear to extend all the way to saturation.
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    • The discontinuous saturation for a strip and for a sphere in d = 3 for a RN black hole with a sufficiently large Q was first observed in [4]; see also Ref. [5].
    • The discontinuous saturation for a strip and for a sphere in d = 3 for a RN black hole with a sufficiently large Q was first observed in [4]; see also Ref. [5].
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    • The expression below may not apply in d = 3, where we do not yet have a clean result.
    • The expression below may not apply in d = 3, where we do not yet have a clean result.


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