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Czechoslovak Journal of Physics

Quasi-hermiticity and the Role of a Metric in Some Boson Hamiltonians

H. B. Geyer, Frederik G. Scholtz, Izak Snyman

Published Oct 1, 2004• 39 citations
Publisher
DOI
10.1023/b:cjop.0000044007.58266.a0

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It has been argued that it is incompatible to maintain unitary time evolution for time-dependent non-Hermitian Hamiltonians when the metric operator is explicitly time dependent. We demonstrate here that the time-dependent Dyson equation and the time-dependent quasi-Hermiticity relation can be solved consistently in such a scenario for a time-dependent Dyson map and time-dependent metric operator, respectively. These solutions are obtained at the cost of rendering the non-Hermitian Hamiltonian to be a nonobservable operator as it ceases to be quasi-Hermitian when the metric becomes time dependent.
We investigate the extension of the Kubo--Martin--Schwinger (KMS) thermal equilibrium condition to bounded non-Hermitian Hamiltonians with real spectra and biorthogonal eigensystems, providing a unified framework through three complementary constructions: a complete KMS theorem under quasi-Hermiticity, a biorthogonal KMS-type identity whose positivity characterises quasi-Hermiticity, and a quantum-detailed-balance condition for the associated open-system dynamics. Our main result is a thermodynamic characterisation of quasi-Hermiticity: for any diagonalisable H∈Md(C)H\in M_d(\mathbb C)H∈Md​(C) with real spectrum, the biorthogonal Gibbs functional ωbi(A)=Zbi−1∑ne−βEn⟨φn∣A∣ψn⟩ω_{\rm bi}(A)=Z_{\rm bi}^{-1}\sum_n e^{-βE_n}\langleφ_n|A|ψ_n\rangleωbi​(A)=Zbi−1​∑n​e−βEn​⟨φn​∣A∣ψn​⟩ satisfies ωbi(A†A)≥0ω_{\rm bi}(A^\dagger A)\ge0ωbi​(A†A)≥0 for all AAA if and only if HHH is quasi-Hermitian. The proof reconstructs the metric ηηη directly from the eigenprojectors of ωbiω_{\rm bi}ωbi​ via the Riesz representation theorem, yielding a metric-free criterion for quasi-Hermiticity. Under the quasi-Hermitian hypothesis, we prove that the ηηη-Gibbs state ωη(A)=Zη−1Tr[ηe−βHA]ω_η(A)=Z_η^{-1}{\rm Tr}[ηe^{-βH}A]ωη​(A)=Zη−1​Tr[ηe−βHA] satisfies the full analytic KMS condition using the Hadamard three-line theorem and Bari's theorem on Riesz bases. The transported state generally differs from the Gibbs state of the isospectral Hermitian partner whenever [η,h]≠0[η,h]\neq0[η,h]=0, so the KMS property cannot be obtained by similarity transformation alone. Finally, within the Haag--Hugenholtz--Winnink programme, we establish the Tomita--Takesaki modular structure of the ηηη-Gibbs state in finite dimensions, while the construction of a compatible C∗C^*C∗-norm and the proof of σσσ-weak continuity remain open.