Black hole microstate cosmology

Journal Article · Sat Jul 13 00:00:00 EDT 2019 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/jhep07(2019)065· OSTI ID:1613202

Cooper, Sean ^[1]; Rozali, Moshe ^[2]; Swingle, Brian ^[3]; Van Raamsdonk, Mark ^[2]; Waddell, Christopher ^[2]; Wakeham, David ^[2]

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1. Univ. of British Columbia, Vancouver, BC (Canada); DOE/OSTI
2. Univ. of British Columbia, Vancouver, BC (Canada)
3. Univ. of Maryland, College Park, MD (United States)

In this note, we explore the possibility that certain high-energy holographic CFT states correspond to black hole microstates with a geometrical behind-the-horizon region, modelled by a portion of a second asymptotic region terminating at an end-of-the-world (ETW) brane. We study the time-dependent physics of this behind-the-horizon region, whose ETW boundary geometry takes the form of a closed FRW spacetime. We show that in many cases, this behind-the-horizon physics can be probed directly by looking at the time dependence of entanglement entropy for sufficiently large spatial CFT subsystems. We study in particular states defined via Euclidean evolution from conformal boundary states and give specific predictions for the behavior of the entanglement entropy in this case. We perform analogous calculations for the SYK model and find qualitative agreement with our expectations. We also calculate holographic complexity for the d = 2 ETW geometries, finding that complexity-action and complexity-volume proposals give the same linear growth at late times, but differ at early times. A fascinating possibility is that for certain states, we might have gravity localized to the ETW brane as in the Randall-Sundrum II scenario for cosmology. In this case, the effective description of physics beyond the horizon could be a big bang/big crunch cosmology of the same dimensionality as the CFT. In this case, the d-dimensional CFT describing the black hole microstate would give a precise, microscopic description of the d-dimensional cosmological physics.

• Research Organization: Univ. of California, Oakland, CA (United States)
• Sponsoring Organization: Natural Sciences and Engineering Research Council of Canada (NSERC); Simons Foundation; USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
• Grant/Contract Number: SC0019380
• OSTI ID: 1613202
• Journal Information: Journal of High Energy Physics (Online), Journal Name: Journal of High Energy Physics (Online) Journal Issue: 7 Vol. 2019; ISSN 1029-8479
• Publisher: Springer Berlin
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
AdS-CFT Correspondence
Black Holes in String Theory
Conformal Field Theory
Holography and condensed matter physics (AdS/CMT)
Physics