Abstract

For time-independent excited states in conformal field theories, the entanglement entropy of small subsystems satisfies a ‘first law’-like relation, in which the change in entanglement is proportional to the energy within the entangling region. Such a law holds for time-dependent scenarios as long as the state is perturbatively close to the vacuum, but is not expected otherwise. In this paper we use holography to investigate the spread of entanglement entropy for unitary evolutions of special physical interest, the so-called global quenches. We model these using AdS-Vaidya geometries. We find that the first law of entanglement is replaced by a linear response relation, in which the energy density takes the role of the source and is integrated against a time-dependent kernel with compact support. For adiabatic quenches the standard first law is recovered, while for rapid quenches the linear response includes an extra term that encodes the process of thermalization. This extra term has properties that resemble a time-dependent ‘relative entropy’. We propose that this quantity serves as a useful order parameter to characterize far-from-equilibrium excited states. We illustrate our findings with concrete examples, including generic power-law and periodically driven quenches.

Highlights

  • Where ρA = trAc[ρ] is the reduced density matrix associated to A

  • We find that the first law of entanglement is replaced by a linear response relation, in which the energy density takes the role of the source and is integrated against a time-dependent kernel with compact support

  • We have studied analytic expressions for the evolution of entanglement entropy after a variety of time-dependent perturbations

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Summary

Perturbative expansion for small subsystems

We will begin by giving a quick overview of the results of [63] on the spread of entanglement of small subsystems in holographic CFTs. We assume that the size of the region A is small in comparison to any other scale of the system This will allow us to extract a universal contribution to the evolution of entanglement entropy following a global quench. In order to study the small subsystem limit we need to focus on the near boundary region of the bulk geometry. As a final example we can consider sourcing the quench with a bulk current Jμ In this case the normalizable corrections take the form δgμν = a zd Tμν + z2d−2 (c1 JμJν + c2 ημν JαJ α ) + · · · ,. The leading correction to the functional will already contain information about the time-dependence and thermalization

Entanglement entropy after global quenches
Linear response of entanglement entropy
Adiabatic limit and the first law of entanglement entropy
Particular cases
Instantaneous quench
Power-law quench
Periodically driven quench
Conclusions and outlook
B Holographic stress-energy tensor
C Ward identities
Full Text
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