Multiple shocks
By S. Shenker, D. Stanford. 2013
490 citations recorded by the source corpus.
A bstractUsing gauge/gravity duality, we explore a class of states of two CFTs with a large degree of entanglement, but with very weak local two-sided correlation. These states are constructed by perturbing the thermofield double state with thermal-scale operators that are local at different times. Acting on the dual black hole geometry, these perturbations create an intersecting network of shock waves, supporting a very long wormhole. Chaotic CFT dynamics and the associated fast scrambling time play an essential role in determining the qualitative features of the resulting geometries.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/c40f86efe9eb5bc79638a562142dfab0f5395523
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Citations in the corpus
- Localized shocks (2014, background): “In [24], two of us checked a refinement of this relationship for a family of states, corresponding to the spherical shock wave geometries constructed in [25].”
- A bound on chaos (2015, methodology): “In the holographic calculations [16, 17, 5, 18, 19] that use Einstein gravity in the bulk, the result (7) holds independent of d and independent of the choice of V and W .”
- Addendum to computational complexity and black hole horizons (2014, background): “An analysis of the two-shockwave geometry [5] gives the same formula for the length of the geodesic connecting the boundary points.”
- Translationally Invariant Non-Fermi-Liquid Metals with Critical Fermi Surfaces: Solvable Models (2018, background): “They have been shown to diagnose quantum chaos in black hole physics [47,53,133,135], and they are supposed to be the fastest scramblers in nature [136].”
- Holographic Complexity Equals Bulk Action? (2015, background): “[9], we can add more than one shock wave [31] in more than one location [7], and the dual calculations continue to match.”
- Efficient decoding for the Hayden-Preskill protocol (2017, unknown): “The type of higher-order OTOCs associated with our deterministic decoding algorithm are similar to those previously considered by Shenker and Stanford [17] in the context of multiple shockwave geometries.”
- TASI Lectures on the Emergence of Bulk Physics in AdS/CFT (2017, methodology): “The right diagram is a spacetime Penrose diagram for an “elongated wormhole”, of the type that can be constructed using infalling matter as in [78].”
- Holographic complexity in Vaidya spacetimes. Part II (2018, background): “The nontrivial cancellations in the complexity of the precursor are connected to the switchback effect [15, 19, 47].”
- Second law of quantum complexity (2017, background): “It can also be explicitly seen in black hole dynamics using the classical shock wave calculus of [29].”
- Switchbacks and the Bridge to Nowhere (2014, methodology): “The old ways are: using Einstein field equations to calculate the response of the ERB geometry to the action of a precursor [9]; and using random quantum circuits to evolve the precursor.”
- An investigation of AdS2 backreaction and holography (2016, background): “Within a holographic context, the link between shockwave interactions in the bulk, and chaotic behavior of the boundary theory has been substantially studied in the recent years [21][22][23][24][25][26].”
- Quantum epidemiology: operator growth, thermal effects, and SYK (2018, methodology): “OTOC) [17–20]:”
- Computational complexity and black hole horizons (2014, background): “Support for this research came through NSF grant Phy-1316699 and the Stanford Institute for Theoretical Physics.”
- Chaos in quantum channels (2015, background): “[22, 23, 7, 47]), one needs to consider superpositions of such tensor networks which do not have a geometric description and thus would not be expected to have a semiclassical bulk interpretation.”
- The factorization problem in Jackiw-Teitelboim gravity (2018, background): “In particular the strong redshift effects near black hole horizons make physics from the point of view of the outside observer unusually sensitive to gravitational effects there [10–14].”