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Two-dimensional gravity and the Sachdev-Ye-Kitaev model

Omar Chammaa

Published Jan 1, 2020• 0 citations
Publisher

Abstract

We briefly introduce and review the Sachdev-Ye-Kitaev (SYK) model. This model exhibits quenched disorder, and many quantities, like the Euclidean path integral, are computed as an average over disorder or an average over many different unitary theories corresponding to different realizations of the disorder couplings. This places the interpretation of the Euclidean path integral as a thermal partition function under scrutiny, which we promptly investigate. We reach he seeming conclusion that the Euclidean path integral indeed does not support a Hilbert space interpretation, which is corroborated by other investigations in the literature. We then move one dimension higher, to two-dimensional Jackiw-Teitelboim (JT) gravity, investigating its salient features and most importantly, the problem of Hilbert space factorization. This puzzle implies that, due to constraints coming from gauge symmetry, a bulk gravitational theory cannot be dual to a theory with a tensor-product structure on disconnected boundary components. We then briefly introduce and review spin glasses, and review the investigations into the presence of a spin glass phase in the SYK model. Finally, we discuss some natural outgrowths of ideas presented in this thesis

DOI
10.82308/7729

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We briefly introduce and review the Sachdev-Ye-Kitaev (SYK) model. This model exhibits quenched disorder, and many quantities, like the Euclidean path integral, are computed as an average over disorder or an average over many different unitary theories corresponding to different realizations of the disorder couplings. This places the interpretation of the Euclidean path integral as a thermal partition function under scrutiny, which we promptly investigate. We reach he seeming conclusion that the Euclidean path integral indeed does not support a Hilbert space interpretation, which is corroborated by other investigations in the literature. We then move one dimension higher, to two-dimensional Jackiw-Teitelboim (JT) gravity, investigating its salient features and most importantly, the problem of Hilbert space factorization. This puzzle implies that, due to constraints coming from gauge symmetry, a bulk gravitational theory cannot be dual to a theory with a tensor-product structure on disconnected boundary components. We then briefly introduce and review spin glasses, and review the investigations into the presence of a spin glass phase in the SYK model. Finally, we discuss some natural outgrowths of ideas presented in this thesis
With the in-depth subjects chiasma among different research areas, many people are applying concepts and methods in theoretical high-energy physics to condensed matter systems. One of the most intensely studied tools is the Anti-de Sitter space/Conformal Field Theory (AdS/CFT) correspondence. It effectively permits a perturbative treatment of strongly coupled systems. Thus, it has been a focused topic in theoretical physics and high-energy physics. It represents a significant breakthrough in understanding quantum gravity. This paper focuses on the realisation of the duality in Jackiw-Teitelboim (JT) gravity and Sachdev-Ye-Kitaev (SYK) Model. To this end, the author derived the action, free energy, thermal entropy, and low-energy dynamics. The symmetry breaking pattern of the SYK model following previous works are also considered. These results were compared with the counterparts in Euclidean JT theory as a cut-out of the complete nearly AdS space in two dimensions. Based on the similarity in the mathematical form of these quantity and symmetry breaking process, the author concludes that the SYK model, as many believed, is a promising candidate for the holographic dual of the JT theory.
The Sachdev-Ye-Kitaev (SYK) model is a quantum mechanical many body system with random all-to-all interactions on fermionic N sites (N>>1). This model is shown to saturate the known maximal chaos bound of many body system and then based on this observation it is conjectured to be dual to a quantum black hole in the sense of the AdS/CFT correspondence. In this dissertation, we show that the large N physics of the SYK model is systematically described by a single bi-local field. In particular, we emphasize the appearance of the emergent conformal reparametrization symmetry at the critical IR fixed point and the corresponding divergent contribution of the symmetry modes in the propagator of the bi-local field. We discuss non-linear-level derivation of the zero modes effective action, which is given by the Schwarzian derivative for finite reparametrization symmetry. Besides the symmetry modes, which correspond to the dilaton-gravity sector in the dual AdS theory, the SYK model also predicts an infinite tower of matter fields in AdS_2. We demonstrate that this infinite spectrum can be nicely packaged into a single field in 3-dimensional space-time. Finally, we consider the question of identifying the dual space-time of the SYK model. Focusing on the signature of emergent space-time of the (Euclidean) model, we explain the need for non-local (Radon-type) transformations on external legs of n-point Green's functions. This results in a dual theory with Euclidean AdS signature with additional leg-factors. We speculate that these factors incorporate the coupling of additional bulk states similar to the discrete states of 2D string theory.
The Sachdev--Ye--Kitaev (SYK) model has a wormholelike solution after averaging over the fermionic couplings in the nearly AdS2{\mathrm{AdS}}_{2}AdS2​ space. Even when the couplings are fixed the contribution of these wormholes continues to exist and new saddle points appear which are interpreted as ``half-wormholes.'' In this paper, we will study the fate of these wormholes in a model without quenched disorder, namely, a tensor model with $O(N{)}^{q\ensuremath{-}1}$ gauge symmetry whose correlation function and thermodynamics in the large NNN limit are the same as that of the SYK model. We will restate the factorization problem linked with the wormhole threaded Wilson operator, in terms of global charges or nontrivial cobordism classes associated with disconnected wormholes. Therefore for the partition function to factorize especially at short distances, there must exist certain topological defects which break the global symmetry associated with wormholes and make the theory devoid of global symmetries. We will interpret these wormholes with added topological defects as our ``half-wormholes.'' We will also comment on the late time behavior of the spectral form factor, particularly its leading and subleading order contributions coming from higher genus wormholes in the gravitational sector. Finally we will show how the other nontrivial saddles from half-wormhole dominate and give rise to unusual thermodynamics in the bulk sector due to nonperturbative effects.
In this paper, I study the entanglement entropy in Hartle-Hawking states of JT gravity set up by a Euclidean path integral with an operator inserted somewhere along the Euclidean boundary. I show that the entanglement entropy between the dual SYK models can be written to leading order in 1/GN1/G_N1/GN​ in a way that resembles a formula for entanglement entropy in a compact lattice gauge theory, but where the link that we appear to compute the entanglement across depends on where we put the operator along the Euclidean boundary. I then describe a toy model where we can write down an explicit family of density matrices whose von Neumann entropies exhibit such a phase transition as we tune an interpolating parameter. This behavior relies on a certain superselection sector structure and I comment on the possibility that the gravitational result comes from a similar emergent superselection sector structure in SYK/JT holography. The main implication is that each copy of the SYK model should then contain Hilbert space sectors labeled by multiple SL(2,R)SL(2,R)SL(2,R) representations whose entanglement gives rise to space.
We study a two-site Sachdev-Ye-Kitaev (SYK) model with complex couplings, and identify a low temperature transition to a gapped phase characterized by a constant in temperature free energy. This transition is observed without introducing a coupling between the two sites, and only appears after ensemble average over the complex couplings. We propose a gravity interpretation of these results by constructing an explicit solution of Jackiw-Teitelboim gravity with matter: a two-dimensional Euclidean wormhole whose geometry is the double trumpet. This solution is sustained by imaginary sources for a marginal operator, without the need of a coupling between the two boundaries. As the temperature is decreased, there is a transition from a disconnected phase with two black holes to the connected wormhole phase, in qualitative agreement with the SYK observation. The expectation value of the marginal operator is an order parameter for this transition. This illustrates in a concrete setup how a Euclidean wormhole can arise from an average over field theory couplings.
Entanglement is one of the most important concepts in quantum physics. We review recent progress in understanding the quantum entanglement in many-body systems using large- N solvable models: the Sachdev—Ye—Kitaev (SYK) model and its generalizations. We present the study of entanglement entropy in the original SYK model using three different approaches: the exact diagonalization, the eigenstate thermalization hypothesis, and the path-integral representation. For coupled SYK models, the entanglement entropy shows linear growth and saturation at the thermal value. The saturation is related to replica wormholes in gravity. Finally, we consider the steady-state entanglement entropy of quantum many-body systems under repeated measurements. The traditional symmetry breaking in the enlarged replica space leads to the measurement-induced entanglement phase transition.