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Physical review. D/Physical review. D.

Maximal entangling rates from holography

Åsmund Folkestad, Aditya Dhumuntarao

Published Oct 30, 2023• 0 citations
Publisher

Abstract

We prove novel far-from-equilibrum bounds on conformal field theories, upper bounding the growth rate of entanglement entropy in spatially uniform states. When equal-time correlators and Wilson loops are computed by geodesics and world sheets, we also bound the growth rate of these. Example applications include lower bounds on thermalization times or the time it takes to achieve deconfinement. Our bounds are proven for holographic conformal field theories at strong coupling and large--$N$, but we provide evidence that they are valid independent of these assumptions. In two dimensions, our results prove a conjectured bound on entanglement growth by Liu and Suh for a large class of states. We also derive bounds on spatial derivatives of correlation measures. From a gravitational perspective, our results constitute new lower bounds on the mass of asymptotically AdS spacetimes with planar symmetry, strengthening the positive mass theorem for these spacetimes. We also derive novel relations in $\mathrm{AdS}/\mathrm{CFT}$ relating various geometric features directly to entanglement entropy derivatives. For example, we show that conformal field theory entanglement growth corresponds to bulk matter falling deeper into the bulk.

DOI
10.1103/physrevd.108.086032

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We prove novel far-from-equilibrum bounds on conformal field theories, upper bounding the growth rate of entanglement entropy in spatially uniform states. When equal-time correlators and Wilson loops are computed by geodesics and world sheets, we also bound the growth rate of these. Example applications include lower bounds on thermalization times or the time it takes to achieve deconfinement. Our bounds are proven for holographic conformal field theories at strong coupling and large--NNN, but we provide evidence that they are valid independent of these assumptions. In two dimensions, our results prove a conjectured bound on entanglement growth by Liu and Suh for a large class of states. We also derive bounds on spatial derivatives of correlation measures. From a gravitational perspective, our results constitute new lower bounds on the mass of asymptotically AdS spacetimes with planar symmetry, strengthening the positive mass theorem for these spacetimes. We also derive novel relations in AdS/CFT\mathrm{AdS}/\mathrm{CFT}AdS/CFT relating various geometric features directly to entanglement entropy derivatives. For example, we show that conformal field theory entanglement growth corresponds to bulk matter falling deeper into the bulk.
We prove novel speed limits on the growth of entanglement, equal-time correlators, and spacelike Wilson loops in spatially uniform time-evolving states in strongly coupled CFTs with holographic duals. These bounds can also be viewed as quantum weak energy conditions. Several of the speed limits are valid for regions of arbitrary size and with multiple connected components, and our findings imply new bounds on the effective entanglement velocity of small subregions. In 2d CFT, our results prove a conjecture by Liu and Suh for a large class of states. We also bound spatial derivatives of entanglement and correlators. Key to our findings is a momentum-entanglement correspondence, showing that entanglement growth is computed by the momentum crossing the HRT surface. In our setup, we prove a number of general features of boundary-anchored extremal surfaces, such as a sharp bound on the smallest radius that a surface can probe, and that the tips of extremal surfaces cannot lie in trapped regions. Our methods rely on novel global GR techniques, including a delicate interplay between Lorentzian and Riemannian Hawking masses. While our proofs assume the dominant energy condition in the bulk, we provide numerical evidence that our bounds are true under less restrictive assumptions.
Abstract We studied the upper bounds of the holographic entanglement entropy growth rate for thermofield double (TFD) states. By comparing the cases of vacuum AdS and charged AdS black holes, we conjecture: for all static planar or spherically symmetric asymptotically Schwarzschild-AdS black holes of same mass density or entropy density, the vacuum AdS black hole gives the maximum entanglement entropy growth rate. We gave proofs by assuming dominant energy condition. We also considered the AdS black hole spacetime with real scalar fields case, where the scalar fields violate the dominant energy condition and the bulk geometry is not asymptotically Schwarzschild-AdS. Numerical results show that this case vacuum black hole still has maximal growth rate if we fixed entropy. However, in the case of fixed energy, vacuum case has maximal growth rate of entanglement entropy only under standard quantization scheme.
We derive in detail several universal features in the time evolution of entanglement entropy and other nonlocal observables in quenched holographic systems. The quenches are such that a spatially uniform density of energy is injected at an instant in time, exciting a strongly coupled conformal field theory which eventually equilibrates. Such quench processes are described on the gravity side by the gravitational collapse of a thin shell that results in a black hole. Various nonlocal observables have a unified description in terms of the area of extremal surfaces of different dimensions. In the large distance limit, the evolution of an extremal surface, and thus the corresponding boundary observable, is controlled by the geometry around and inside the event horizon of the black hole, allowing us to identify regimes of pre-local-equilibration quadratic growth, post-local-equilibration linear growth, a memory loss regime, and a saturation regime with behavior resembling those in phase transitions. We also discuss possible bounds on the maximal rate of entanglement growth in relativistic systems.
A global quench is an interesting setting where we can study thermalization of subsystems in a pure state. We investigate entanglement entropy (EE) growth in global quenches in holographic field theories and relate some of its aspects to quantities characterizing chaos. More specifically we obtain four key results: 1. We prove holographic bounds on the entanglement velocity v E and the butterfly effect speed v B that arises in the study of chaos. 2. We obtain the EE as a function of time for large spherical entangling surfaces analytically. We show that the EE is insensitive to the details of the initial state or quench protocol. 3. In a thermofield double state we determine analytically the two-sided mutual information between two large concentric spheres separated in time. 4. We derive a bound on the rate of growth of EE for arbitrary shapes, and develop an expansion for EE at early times. In a companion paper [1], these results are put in the broader context of EE growth in chaotic systems: we relate EE growth to the chaotic spreading of operators, derive bounds on EE at a given time, and compare the holographic results to spin chain numerics and toy models. In this paper, we perform holographic calculations that provide the basis of arguments presented in that paper.
A global quench is an interesting setting where we can study thermalization of subsystems in a pure state. We investigate entanglement entropy (EE) growth in global quenches in holographic field theories and relate some of its aspects to quantities characterizing chaos. More specifically we obtain four key results: 1. We prove holographic bounds on the entanglement velocity vE and the butterfly effect speed vB that arises in the study of chaos. 2. We obtain the EE as a function of time for large spherical entangling surfaces analytically. We show that the EE is insensitive to the details of the initial state or quench protocol. 3. In a thermofield double state we determine analytically the two-sided mutual information between two large concentric spheres separated in time. 4. We derive a bound on the rate of growth of EE for arbitrary shapes, and develop an expansion for EE at early times. In a companion paper, these results are put in the broader context of EE growth in chaotic systems: we relate EE growth to the chaotic spreading of operators, derive bounds on EE at a given time, and compare the holographic results to spin chain numerics and toy models. In this paper, we perform holographic calculations that provide the basis of arguments presented in that paper.
Time-dependent entanglement entropy (EE) is computed for a single interval in two-dimensional conformal theories from a quenched initial state in the presence of spatial boundaries. The EE is found to be periodic in time with periodicity equal to the system size LLL. For large enough LLL, the EE shows a rise to a thermal value (characterized by a temperature 1/β1/β1/β determined by the initial state), followed by periodic returns to the original value. This works irrespective of whether the conformal field theory (CFT) is rational or irrational. For conformal field theories with a holographic dual, the large ccc limit plays an essential role in ensuring that the EE computed from the CFT is universal (independent of the details of the CFT and of boundary conditions) and is exactly matched by the holographic EE. The dual geometry is computed and it interpolates between a BTZ black hole at large LLL and global AdS at large βββ.