Abstract

We study properties of the Petz recovery map in chaotic systems, such as the Hayden–Preskill setup for evaporating black holes and the Sachdev–Ye–Kitaev (SYK) model. Since these systems exhibit the phenomenon called scrambling, we expect that the expression of the recovery channel $\mathcal {R}$ gets simplified, given by just the adjoint $\mathcal {N}^{\dagger }$ of the original channel $\mathcal {N}$ which defines the time evolution of the states in the code subspace embedded into the physical Hilbert space. We check this phenomenon in two examples. The first one is the Hayden–Preskill setup described by Haar random unitaries. We compute the relative entropy $S(\mathcal {R}\left[\mathcal {N}[\rho ]\right] ||\rho)$ and show that it vanishes when the decoupling is archived. We further show that the simplified recovery map is equivalent to the protocol proposed by Yoshida and Kitaev. The second example is the SYK model where the 2D code subspace is defined by an insertion of a fermionic operator, and the system is evolved by the SYK Hamiltonian. We check the recovery phenomenon by relating some matrix elements of an output density matrix $\langle{T}|\mathcal {R}[\mathcal {N}[\rho ]]|{T^{\prime }}\rangle$ to Rényi-two modular flowed correlators, and show that they coincide with the elements for the input density matrix with small error after twice the scrambling time.

Details

Title
The Petz (lite) recovery map for the scrambling channel
Author
Nakayama, Yasuaki 1 ; Miyata, Akihiro 2   VIAFID ORCID Logo  ; Ugajin, Tomonori 3 

 Department of Physics, Kyoto University , Kitashirakawa, Kyoto 606-8502 , Japan 
 Kavli Institute for Theoretical Sciences, University of Chinese Academy of Sciences , Zhong-Guan-Cun East Road, Haidian District , Beijing 100190, China 
 Department of Physics, Rikkyo University , Nishi-Ikebukuro, Toshima, Tokyo 171-8501 , Japan 
Publication year
2023
Publication date
Dec 2023
Publisher
Oxford University Press
e-ISSN
20503911
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3171495147
Copyright
© The Author(s) 2023. Published by Oxford University Press on behalf of the Physical Society of Japan. This work is published under https://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.