Quantum Markovian master equation in the high-temperature limit
Ricardo C. Zamar, J. Agust\'in Taboada

TL;DR
This paper derives a high-temperature quantum Markovian master equation (HTME) that generalizes existing models, incorporates non-thermal initial states, and clarifies the conditions for its validity in open quantum systems.
Contribution
The authors provide a rigorous derivation of the HTME, extending previous models to include non-thermal states and analyzing spectral density symmetrization, thereby refining the theoretical framework for quantum dissipation.
Findings
Derivation of a generalized HTME including non-thermal initial states
Identification of a symmetrization condition for spectral densities at high temperatures
Demonstration of limitations of ARH-IME in strongly correlated spin systems
Abstract
We present a critical derivation of the high-temperature quantum Markovian master equation (HTME), examining its foundational assumptions, their quantum-mechanical implications, and its range of validity. Starting from the Born-Markov master equation, and combining the spin Hamiltonian eigenoperator formalism with a linear expansion in statistical coefficients, as the only assumption, we obtain a quantum dissipator that generalizes the Abragam-Redfield-Hubbard inhomogeneous master equation (ARH-IME). Our derivation naturally incorporates an additional term for non-thermal, high-order initial states, while reducing to ARH-IME for spin states evolving near thermal equilibrium (weak-order). Through an alternative operator-based derivation of the HTME, we confirm these results and reveal a symmetrization condition for the spectral densities in the linear thermal regime. We rigorously…
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