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Main Authors: Zhang, Chenyi, Yu, Minghong, Yan, Yiying, Chen, Lipeng, Lü, Zhiguo, Zhao, Yang
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2304.02675
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author Zhang, Chenyi
Yu, Minghong
Yan, Yiying
Chen, Lipeng
Lü, Zhiguo
Zhao, Yang
author_facet Zhang, Chenyi
Yu, Minghong
Yan, Yiying
Chen, Lipeng
Lü, Zhiguo
Zhao, Yang
contents We study the emission spectra of dissipative Rabi and Jaynes-Cummings models in the non-Markovian and ultrastrong coupling regimes. We have derived a polaron-transformed Nakajima-Zwanzig master equation (PTNZE) to calculate the emission spectra, which eliminates the well known limitations of the Markovian approximation and the standard second-order perturbation. Using the time-dependent variational approach as benchmark, the PTNZE is found to yield accurate emission spectra in certain ultrastrong coupling regimes where the standard second-order Nakajima-Zwanzig master equation breaks down. It is shown that the emission spectra of the dissipative Rabi and Jaynes-Cummings models are in general asymmetric under various initial conditions. Direct comparisons of spectra for the two models illustrate the essential role of the qubit-cavity counter-rotating term and the spectra features under different qubit-cavity coupling strengths and system initial conditions.
format Preprint
id arxiv_https___arxiv_org_abs_2304_02675
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Emission spectral non-Markovianity in qubit-cavity systems in the ultrastrong coupling regime
Zhang, Chenyi
Yu, Minghong
Yan, Yiying
Chen, Lipeng
Lü, Zhiguo
Zhao, Yang
Quantum Physics
We study the emission spectra of dissipative Rabi and Jaynes-Cummings models in the non-Markovian and ultrastrong coupling regimes. We have derived a polaron-transformed Nakajima-Zwanzig master equation (PTNZE) to calculate the emission spectra, which eliminates the well known limitations of the Markovian approximation and the standard second-order perturbation. Using the time-dependent variational approach as benchmark, the PTNZE is found to yield accurate emission spectra in certain ultrastrong coupling regimes where the standard second-order Nakajima-Zwanzig master equation breaks down. It is shown that the emission spectra of the dissipative Rabi and Jaynes-Cummings models are in general asymmetric under various initial conditions. Direct comparisons of spectra for the two models illustrate the essential role of the qubit-cavity counter-rotating term and the spectra features under different qubit-cavity coupling strengths and system initial conditions.
title Emission spectral non-Markovianity in qubit-cavity systems in the ultrastrong coupling regime
topic Quantum Physics
url https://arxiv.org/abs/2304.02675