Published October 2022 | Version public
Journal Article

Periodically, Quasi-periodically, and Randomly Driven Conformal Field Theories (II): Furstenberg's Theorem and Exceptions to Heating Phases

  • 1. ROR icon Harvard University
  • 2. ROR icon University of Colorado Boulder
  • 3. ROR icon California Institute of Technology

Abstract

In this sequel (to [Phys. Rev. Res. 3, 023044(2021)], arXiv:2006.10072), we study randomly driven (1 + 1) dimensional conformal field theories (CFTs), a family of quantum many-body systems with soluble non-equilibrium quantum dynamics. The sequence of driving Hamiltonians is drawn from an independent and identically distributed random ensemble. At each driving step, the deformed Hamiltonian only involves the energy-momentum density spatially modulated at a single wavelength and therefore induces a M\"obius transformation on the complex coordinates. The non-equilibrium dynamics is then determined by the corresponding sequence of M\"obius transformations, from which the Lyapunov exponent λ_L is defined. We use Furstenberg's theorem to classify the dynamical phases and show that except for a few exceptional points that do not satisfy Furstenberg's criteria, the random drivings always lead to a heating phase with the total energy growing exponentially in the number of driving steps n and the subsystem entanglement entropy growing linearly in n with a slope proportional to central charge c and the Lyapunov exponent λ_L. On the contrary, the subsystem entanglement entropy at an exceptional point could grow as √n while the total energy remains to grow exponentially. In addition, we show that the distributions of the operator evolution and the energy density peaks are also useful characterizations to distinguish the heating phase from the exceptional points: the heating phase has both distributions to be continuous, while the exceptional points could support finite convex combinations of Dirac measures depending on their specific type. In the end, we compare the field theory results with the lattice model calculations for both the entanglement and energy evolution and find remarkably good agreement.

Additional Information

We thank for helpful discussions with Dan Borgnia, Daniel Jafferis, Bo Han, Eslam Khalaf, Ching Hua Lee, Ivar Martin, Shinsei Ryu, Hassan Shapourian, Tsukasa Tada, Michael Widom, Jie-Qiang Wu, and Yahui Zhang. XW, RF and AV are supported by a Simons Investigator award (AV) and by the Simons Collaboration on Ultra-Quantum Matter, which is a grant from the Simons Foundation (651440, AV). AV and RF are supported by the DARPA DRINQS program (award D18AC00033). YG is supported by the the Simons Foundation through the "It from Qubit" program.

Additional details

Identifiers

Eprint ID
117716
Resolver ID
CaltechAUTHORS:20221104-610921700.12

Related works

Funding

Air Force Office of Scientific Research (AFOSR)
D18AC00033
Simons Foundation
651440

Dates

Created
2022-11-17
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Updated
2022-11-17
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