Kubo-Martin-Schwinger conditions for non-Hermitian systems
Abstract
We investigate the extension of the Kubo--Martin--Schwinger (KMS) thermal equilibrium condition to non-Hermitian Hamiltonians with real spectra and biorthogonal eigensystems, providing a systematic analysis through three complementary routes. Our central result is a thermodynamic characterisation of quasi-Hermiticity: for H ∈ Md(C) diagonalisable with real spectrum, the biorthogonal Gibbs functional ωbi(A) = Zbi-1 Σn e-βEnϕn|A|ψn satisfies ωbi(A†A) ≥ 0 for all A if and only if H is quasi-Hermitian. The proof constructs the metric η directly from the eigenprojectors of ωbi via the Riesz representation theorem, with no prior choice of η, providing a metric-free certificate of quasi-Hermiticity outside the Mostafazadeh--Scholtz framework. Under the full quasi-Hermitian hypothesis, we prove that the η-Gibbs state ωη(A) = Zη-1\, Tr[ηe-βHA] satisfies all three analytic KMS conditions, using the Hadamard three-line theorem and Bari's theorem on Riesz bases. The result is non-trivial: the transported state ω(X) = Tr[e-βhXη]/Zη differs from the Gibbs state of the isospectral Hermitian partner h = η1/2Hη-1/2 whenever [η,h]≠ 0, so the KMS property cannot be deduced from the Hermitian theory by similarity. The gap between this result and the full Haag--Hugenholtz--Winnink C*-algebraic framework is identified. Failure modes at exceptional points and for complex spectra are analysed, and the relation to the Fagnola--Umanità quantum detailed balance condition for open systems is discussed.
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