Exactly solvable floquet dynamics for conformal field theories in dimensions greater than two

Diptarka Das, Sumit R. Das, Arnab Kundu, Krishnendu Sengupta

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7 Scopus citations

Abstract

We find classes of driven conformal field theories (CFT) in d + 1 dimensions with d > 1, whose quench and floquet dynamics can be computed exactly. The setup is suitable for studying periodic drives, consisting of square pulse protocols for which Hamiltonian evolution takes place with different deformations of the original CFT Hamiltonian in successive time intervals. These deformations are realized by specific combinations of conformal generators with a deformation parameter β; the β < 1 (β > 1) Hamiltonians can be unitarily related to the standard (Lüscher-Mack) CFT Hamiltonians. The resulting time evolution can be then calculated by performing appropriate conformal transformations. For d ≤ 3 we show that the transformations can be easily obtained in a quaternion formalism. Evolution with such a single Hamiltonian yields qualitatively different time dependences of observables depending on the value of β, with exponential decays characteristic of heating for β > 1, oscillations for β < 1 and power law decays for β = 1. This manifests itself in the behavior of the fidelity, unequal-time correlator, and the energy density at the end of a single cycle of a square pulse protocol with different hamiltonians in successive time intervals. When the Hamiltonians in a cycle involve generators of a single SU(1, 1) subalgebra we calculate the Floquet Hamiltonian. We show that one can get dynamical phase transitions for any β by varying the time period of a cycle, where the system can go from a non-heating phase which is oscillatory as a function of the time period to a heating phase with an exponentially damped behavior. Our methods can be generalized to other discrete and continuous protocols. We also point out that our results are expected to hold for a broader class of QFTs that possesses an SL(2, C) symmetry with fields that transform as quasi-primaries under this. As an example, we briefly comment on celestial CFTs in this context.

Original languageEnglish
Article number95
JournalJournal of High Energy Physics
Volume2024
Issue number9
DOIs
StatePublished - Sep 2024

Bibliographical note

Publisher Copyright:
© The Author(s) 2024.

Funding

We would like to thank Bobby Ezhuthachan, Akavoor Manu, Masahiro Nozaki and Koushik Ray for discussions. The work of S.R.D. is supported by a National Science Foundation grant NSF-PHY/211673 and Jack and Linda Gill Chair Professorship. S.R.D. would like to thank Yukawa Institute of Theoretical Physics and Isaac Newton Institute for Mathematical Physics for hospitality during the completion of this work. KS thanks DST for support through SERB project JCB/2021/000030. AK is partially supported by CEFIPRA 6304 3, DAE-BRNS 58/14/12/2021-BRNS and CRG/2021/004539 of Govt. of India. D.D. acknowledges support by the Max Planck Partner Group grant MAXPLA/PHY/2018577 and from MATRICS grant SERB/PHY/2020334.

FundersFunder number
Department of Science and Technology, Ministry of Science and Technology, India
Yukawa Institute for Theoretical Physics
Bobby Ezhuthachan
Indo-French Centre for the Promotion of Advanced ResearchDAE-BRNS 58/14/12/2021-BRNS, 6304 3, CRG/2021/004539
Not addedEP/R014604/1
National Science Foundation Arctic Social Science ProgramNSF-PHY/211673
Science and Engineering Research BoardJCB/2021/000030
Max-Planck-Institut für AstronomieMAXPLA/PHY/2018577, SERB/PHY/2020334

    Keywords

    • Conformal and W Symmetry
    • Non-Equilibrium Field Theory

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

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