Comparison of the standard and dressed-picture master equations for the quantum Rabi model in the ultrastrong coupling regime
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Quantum Physics arXiv:2604.08852 (quant-ph) [Submitted on 10 Apr 2026] Title:Comparison of the standard and dressed-picture master equations for the quantum Rabi model in the ultrastrong coupling regime Authors:Alexandre P. Costa, Hebert S. Rego de Oliveira, Alexandre Dodonov View a PDF of the paper titled Comparison of the standard and dressed-picture master equations for the quantum Rabi model in the ultrastrong coupling regime, by Alexandre P. Costa and 2 other authors View PDF HTML (experimental) Abstract:The goal of this chapter is to investigate the effects of relaxation and dephasing on the quantum Rabi model in the ultrastrong coupling regime, and to provide explicit formulas to implement and numerically solve the resulting nonunitary dynamics from first principles. The quantum Rabi model constitutes the most fundamental description of light-matter interaction, describing a single two-level system coupled to a single mode of a quantized cavity field. The ultrastrong coupling regime is typically defined by $g \gtrsim 0.1\omega$, where $\omega$ denotes the cavity-mode frequency. In this regime, the standard master equation of quantum optics -- commonly referred to as the Gorini-Kossakowski-Sudarshan-Lindblad (GKSL) master equation -- becomes inaccurate. The reason is that strong light-matter interaction hybridizes the bare atom and field states, so that dissipation cannot be consistently described in the uncoupled basis. A consistent treatment must therefore incorporate this hybridization directly into the dissipative terms. One such approach is the dressed-picture Markovian master equation derived by Beaudoin, Gambetta, and Blais, in which the qubit-field interaction is explicitly included in the construction of the system-bath coupling operators. In this chapter, we numerically solve both the GKSL master equation and the dressed master equation (DME) for various initial field states, including coherent, odd Schrödinger cat, squeezed vacuum, squeezed coherent, and thermal states. We also examine photon generation from the vacuum induced by external time-dependent modulation of the qubit parameters, as well as multiphoton Rabi oscillations for an initially excited qubit. Two reservoir spectral densities are considered: white and Ohmic noise. The differences between the two approaches are illustrated through numerical results for several physical observables. Comments: Subjects: Quantum Physics (quant-ph) Cite as: arXiv:2604.08852 [quant-ph] (or arXiv:2604.08852v1 [quant-ph] for this version) https://doi.org/10.48550/arXiv.2604.08852 Focus to learn more arXiv-issued DOI via DataCite (pending registration) Submission history From: A. V. Dodonov [view email] [v1] Fri, 10 Apr 2026 01:22:07 UTC (2,741 KB) Full-text links: Access Paper: View a PDF of the paper titled Comparison of the standard and dressed-picture master equations for the quantum Rabi model in the ultrastrong coupling regime, by Alexandre P. Costa and 2 other authorsView PDFHTML (experimental)TeX Source view license Current browse context: quant-ph new | recent | 2026-04 References & Citations INSPIRE HEP NASA ADSGoogle Scholar Semantic Scholar export BibTeX citation Loading... BibTeX formatted citation × loading... Data provided by: Bookmark Bibliographic Tools Bibliographic and Citation Tools Bibliographic Explorer Toggle Bibliographic Explorer (What is the Explorer?) Connected Papers Toggle Connected Papers (What is Connected Papers?) Litmaps Toggle Litmaps (What is Litmaps?) scite.ai Toggle scite Smart Citations (What are Smart Citations?) Code, Data, Media Code, Data and Media Associated with this Article alphaXiv Toggle alphaXiv (What is alphaXiv?) Links to Code Toggle CatalyzeX Code Finder for Papers (What is CatalyzeX?) DagsHub Toggle DagsHub (What is DagsHub?) GotitPub Toggle Gotit.pub (What is GotitPub?) Huggingface Toggle Hugging Face (What is Huggingface?) ScienceCast Toggle ScienceCast (What is ScienceCast?) Demos Demos Replicate Toggle Replicate (What is Replicate?) Spaces Toggle Hugging Face Spaces (What is Spaces?) Spaces Toggle TXYZ.AI (What is TXYZ.AI?) Related Papers Recommenders and Search Tools Link to Influence Flower Influence Flower (What are Influence Flowers?) Core recommender toggle CORE Recommender (What is CORE?) Author Venue Institution Topic About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs. Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)