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 language | English |
|---|---|
| Article number | 95 |
| Journal | Journal of High Energy Physics |
| Volume | 2024 |
| Issue number | 9 |
| DOIs | |
| State | Published - 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.
| Funders | Funder 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 Research | DAE-BRNS 58/14/12/2021-BRNS, 6304 3, CRG/2021/004539 |
| Not added | EP/R014604/1 |
| National Science Foundation Arctic Social Science Program | NSF-PHY/211673 |
| Science and Engineering Research Board | JCB/2021/000030 |
| Max-Planck-Institut für Astronomie | MAXPLA/PHY/2018577, SERB/PHY/2020334 |
Keywords
- Conformal and W Symmetry
- Non-Equilibrium Field Theory
ASJC Scopus subject areas
- Nuclear and High Energy Physics