01291nas a2200169 4500008004100000245005900041210005900100260001400159300000900173490000900182520082200191100001701013700001801030700001901048700001701067856003701084 2020 eng d00aBuilding Bulk Geometry from the Tensor Radon Transform0 aBuilding Bulk Geometry from the Tensor Radon Transform c12/4/2020 a1-500 v20203 a

Using the tensor Radon transform and related numerical methods, we study how bulk geometries can be explicitly reconstructed from boundary entanglement entropies in the specific case of AdS3/CFT2. We find that, given the boundary entanglement entropies of a 2d CFT, this framework provides a quantitative measure that detects whether the bulk dual is geometric in the perturbative (near AdS) limit. In the case where a well-defined bulk geometry exists, we explicitly reconstruct the unique bulk metric tensor once a gauge choice is made. We then examine the emergent bulk geometries for static and dynamical scenarios in holography and in many-body systems. Apart from the physics results, our work demonstrates that numerical methods are feasible and effective in the study of bulk reconstruction in AdS/CFT.

1 aCao, ChunJun1 aQ, Xiao-Liang1 aSwingle, Brian1 aTang, Eugene uhttps://arxiv.org/abs/2007.0000401902nas a2200157 4500008004100000245011500041210006900156260001500225520137700240100001801617700001301635700001701648700001901665700002301684856003701707 2019 eng d00aButterfly effect in interacting Aubry-Andre model: thermalization, slow scrambling, and many-body localization0 aButterfly effect in interacting AubryAndre model thermalization  c02/19/20193 a

The many-body localization transition in quasiperiodic systems has been extensively studied in recent ultracold atom experiments. At intermediate quasiperiodic potential strength, a surprising Griffiths-like regime with slow dynamics appears in the absence of random disorder and mobility edges. In this work, we study the interacting Aubry-Andre model, a prototype quasiperiodic system, as a function of incommensurate potential strength using a novel dynamical measure, information scrambling, in a large system of 200 lattice sites. Between the thermal phase and the many-body localized phase, we find an intermediate dynamical phase where the butterfly velocity is zero and information spreads in space as a power-law in time. This is in contrast to the ballistic spreading in the thermal phase and logarithmic spreading in the localized phase. We further investigate the entanglement structure of the many-body eigenstates in the intermediate phase and find strong fluctuations in eigenstate entanglement entropy within a given energy window, which is inconsistent with the eigenstate thermalization hypothesis. Machine-learning on the entanglement spectrum also reaches the same conclusion. Our large-scale simulations suggest that the intermediate phase with vanishing butterfly velocity could be responsible for the slow dynamics seen in recent experiments.

1 aXu, Shenglong1 aLi, Xiao1 aHsu, Yi-Ting1 aSwingle, Brian1 aSarma, Sankar, Das uhttps://arxiv.org/abs/1902.0719901804nas a2200157 4500008004100000245003600041210003600077520137400113100001701487700001801504700001901522700002401541700002501565700001901590856003701609 2018 eng d00aBlack Hole Microstate Cosmology0 aBlack Hole Microstate Cosmology3 a

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. 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. 

1 aCooper, Sean1 aRozali, Moshe1 aSwingle, Brian1 aVan Raamsdonk, Mark1 aWaddell, Christopher1 aWakeham, David uhttps://arxiv.org/abs/1810.10601