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An open quantum material is a many-body material or synthetic-matter platform whose relevant states, spectra, or functions depend essentially on coupling to degrees of freedom outside the retained model. Those degrees of freedom may be phonons, photons, substrates, electrical leads, defects, fluctuating fields, measurement channels, or deliberately engineered reservoirs. “Open” is a modeling boundary, not a new chemical category: the same sample can be treated as closed for a femtosecond coherent process and open for transport, relaxation, or steady-state preparation.

We connect environmental coupling to measurable linewidths, conditional dynamics, state preparation and exceptional points. The same complex matrix can describe different experiments, so its physical interpretation matters as much as its eigenvalues. System–Bath Hamiltonians develops the microscopic setup; Driven-Dissipative Matter treats sustained pump–loss phases.

Required background. Driven-Dissipative Matter supplies material pump, loss and steady-response regimes. System–Bath Hamiltonians supplies the retained degrees of freedom, environment and coupling before reduction. Lindblad–GKSL Equation supplies the completely positive Markovian generator and its assumptions. Spectral Functions supplies spectral weights, pole and linewidth interpretation, and their distinction from measured probe intensity.

A useful microscopic starting point is

Htot=HM+HE+∑αAα⊗Bα.H_{\mathrm{tot}} = H_M + H_E + \sum_\alpha A_\alpha\otimes B_\alpha.

HMH_M contains the material degrees of freedom retained in the calculation, HEH_E contains the environment, and Aα⊗BαA_\alpha\otimes B_\alpha specifies what the environment can monitor or exchange. The split must be declared. Treating a cavity photon, optical phonon, or metallic lead as part of MM in one model and tracing it into EE in another changes both the state space and the observables.

Electrons may exchange energy and momentum with phonons, particles with leads, and radiation with a cavity or the electromagnetic vacuum. Slow spins and fluctuating charges can add memory. Static disorder instead describes uncertainty in a fixed sample; it is not itself a time-dependent reservoir that carries away energy.

Calling all these influences “decoherence” loses important distinctions. A bath can shift levels, broaden poles, thermalize occupations, dephase selected coherences, remove particles, mediate interactions, or create correlated noise. Phonons can destroy electronic phase coherence and also mediate pairing. A cavity can provide loss and also reorganize collective modes. The sign and usefulness of an environmental effect are questions about a specified observable and timescale.

The bath spectrum and state matter as well as the coupling strength. For stationary environmental fluctuations with their mean subtracted, the correlation matrix

Sαβ(ω)=∫−∞∞dt eiωt⟨Bα(t)Bβ(0)⟩ES_{\alpha\beta}(\omega) = \int_{-\infty}^{\infty} dt\, e^{i\omega t} \left\langle B_\alpha(t)B_\beta(0) \right\rangle_E

determines transition rates and noise in suitable weak-coupling reductions. A Markov approximation requires more than weak coupling: the relevant environmental correlations must decay rapidly compared with the retained evolution, and the system frequencies sampled by the coupling must be resolved consistently. Near a band edge, sharp phonon resonance, cavity pole, or critical environment, memory can be the leading physics.

No single “open Hamiltonian” contains every open-system observable. Different reductions preserve different information.

Observable Suitable description
Populations and coherences A density matrix and master equation include mixed states and jump channels.
Quasiparticle poles and lifetimes A retarded Green function includes spectral weight and self-energy.
Currents through contacts Scattering or nonequilibrium Green functions include occupations and contacts.
A monitored trajectory A conditional state includes the selected detector record.
Collective response and noise A Keldysh theory organizes both response and correlations.
Resonances in a subspace A projection method retains energy-dependent feedback from eliminated states.

Agreement between two descriptions is conditional. A Lindblad equation can imply a retarded response, but its jump operators contain information that an effective non-Hermitian Hamiltonian alone omits. A retarded self-energy gives linewidths but does not by itself fix occupations; the Keldysh or lesser component carries distribution information.

For a translationally organized material, a retarded single-particle Green function can be written

GR(k,ω)=[(ℏω+i0+)I−H0(k)−ΣR(k,ω)]−1.G^R(\mathbf k,\omega) = \left[ \left( \hbar\omega+i0^+ \right)I - H_0(\mathbf k) - \Sigma^R(\mathbf k,\omega) \right]^{-1}.

With this energy-denominator convention, the spectral density is

A(k,ω)=−1πIm⁡Tr⁡GR(k,ω).\mathcal A(\mathbf k,\omega) = -\frac{1}{\pi} \operatorname{Im} \operatorname{Tr} G^R(\mathbf k,\omega).

For a complete set of NN canonical fermion orbitals, the full spectral sum is ∫ℏ dω A(k,ω)=N\int\hbar\,d\omega\,\mathcal A(\mathbf k,\omega)=N. A plot normalized per unit angular frequency would instead use ℏA\hbar\mathcal A. Restricting to a low-energy window can omit spectral weight.

The Hermitian part of ΣR\Sigma^R shifts and mixes quasiparticle levels. Its anti-Hermitian part produces decay and can mix decay channels. Both may depend strongly on frequency and momentum. The actual pole width follows from the pole equation; it is not generally just minus twice an eigenvalue of Im⁡ΣR\operatorname{Im}\Sigma^R evaluated at one real frequency. Replacing ΣR(ω)\Sigma^R(\omega) by a constant matrix requires a suitable spectral window.

A complex pole

zn=εn−i2Γnz_n = \varepsilon_n - \frac{i}{2}\Gamma_n

has an energy width Γn>0\Gamma_n>0 under the convention e−iznt/ℏe^{-iz_nt/\hbar}: amplitude decays as e−Γnt/(2ℏ)e^{-\Gamma_n t/(2\hbar)} and its squared magnitude as e−Γnt/ℏe^{-\Gamma_n t/\hbar}. The measured spectral peak need not sit exactly at Re⁡zn\operatorname{Re}z_n when backgrounds, overlapping resonances, matrix elements, or frequency-dependent self-energies distort the line shape.

Environmental coupling becomes a design tool when its spectrum, geometry, or monitored channel is deliberately chosen to stabilize a useful state or response. Examples include cooling selected modes, optically pumping a spin sector, making an entangled state dark, removing defects faster than they are created, or engineering a topological steady-state covariance matrix.

In a Markovian model,

ρ˙=−iℏ[H,ρ]+∑μD[Lμ]ρ.\dot\rho = -\frac{i}{\hbar} [H,\rho] + \sum_\mu \mathcal D[L_\mu]\rho.

The target ρ⋆\rho_\star must satisfy

Lρ⋆=0,\mathcal L\rho_\star=0,

but a stationary target may coexist with other dark states. Preparation requires attraction from the intended initial states, a usable relaxation time, and realizable couplings. Locality, transport and natural errors can limit preparation even when the target is unique (Diehl and collaborators, 2008; Verstraete, Wolf and Cirac, 2009).

A useful illustration is a two-state rate model. Let FF be the target population, κp\kappa_p the correction rate from the unwanted state, and γe\gamma_e the rate of leaving the target:

F˙=κp(1−F)−γeF,1−Fss=γeκp+γe.\dot F=\kappa_p(1-F)-\gamma_e F, \qquad 1-F_{\mathrm{ss}}=\frac{\gamma_e}{\kappa_p+\gamma_e}.

The estimate 1−Fss≃γe/κp1-F_{\mathrm{ss}}\simeq\gamma_e/\kappa_p follows only when errors are weak. A general many-body generator cannot be reduced to this formula by simply substituting its smallest decay rate: mode overlaps, nonnormality, dark sectors and correlated errors matter. A global target fidelity can also deteriorate with the number of error locations. Reservoir Engineering develops preparation strategies and their assumptions.

A non-Hermitian Hamiltonian is usually an effective generator, pole equation, or wave operator. Its physical meaning depends on how it was obtained.

For an initially pure state and ideal counting of every jump channel in a Lindblad model, the unnormalized state conditioned on no detections evolves with

Heff=H−iℏ2∑μLμ†Lμ.H_{\mathrm{eff}} = H - \frac{i\hbar}{2} \sum_\mu L_\mu^\dagger L_\mu.

The jump operators include the square roots of their rates. The squared norm obeys

ddt⟨ψ~∣ψ~⟩=−∑μ⟨Lμ†Lμ⟩ψ~.\frac{d}{dt} \langle\tilde\psi\vert\tilde\psi\rangle = - \sum_\mu \left\langle L_\mu^\dagger L_\mu \right\rangle_{\tilde\psi}.

The remaining squared norm is the no-detection probability; its decrease gives the probability of a jump. Restoring jumps and averaging records recovers trace-preserving evolution. Undetected channels generally leave a mixed conditional state, while homodyne monitoring produces a different, diffusive trajectory. Quantum-Jump Simulation explains how the detection scheme selects the evolution.

Let PP retain a material subspace and Q=I−PQ=I-P contain eliminated states. Outgoing boundary conditions give an energy-dependent operator

Heff(E)=PHP+PHQ1E−QHQ+i0+QHP.H_{\mathrm{eff}}(E) ={} PHP + PHQ \frac{1}{ E-QHQ+i0^+ } QHP.

The second term is a self-energy. Above an open threshold it acquires an anti-Hermitian part on the real-energy boundary. Resonance poles require analytic continuation of this outgoing resolvent to the appropriate complex-energy sheet and solve

det⁡ ⁣[E−Heff(E)]=0,\det\!\left[ E-H_{\mathrm{eff}}(E) \right] = 0,

so diagonalizing a frozen matrix at one real EE can miss energy dependence, extra roots, and threshold structure. Feshbach Projection Formalism develops the state reconstruction and normalization that accompany this reduction.

Classical photonic, acoustic, mechanical, and circuit platforms often produce a non-Hermitian eigenproblem directly after imposing radiation, absorption, gain, or impedance boundary conditions. Electronic quasiparticle models can instead use

Hqp(k,ω)=H0(k)+ΣR(k,ω).H_{\mathrm{qp}}(\mathbf k,\omega) = H_0(\mathbf k) + \Sigma^R(\mathbf k,\omega).

The microscopic many-body Hamiltonian may remain Hermitian even though the quasiparticle pole operator is not. Complex bands then organize frequency and lifetime, but they are not a list of stationary energies of an isolated crystal.

For a diagonalizable non-Hermitian matrix,

Heff∣Rn⟩=zn∣Rn⟩,⟨Ln∣Heff=zn⟨Ln∣.\begin{aligned} H_{\mathrm{eff}} \lvert R_n\rangle &= z_n\lvert R_n\rangle, \\ \langle L_n\rvert H_{\mathrm{eff}} &= z_n\langle L_n\rvert. \end{aligned}

The left and right vectors can be normalized biorthogonally:

⟨Lm∣Rn⟩=δmn.\langle L_m\vert R_n\rangle = \delta_{mn}.

Right eigenvectors alone need not be orthogonal, and the matrix can be highly nonnormal. Small perturbations can then produce large eigenvector and transient-response changes even away from an exact degeneracy.

The biorthogonal quantity ⟨Ln∣O∣Rn⟩\langle L_n\vert O\vert R_n\rangle is mathematically natural, but it is not automatically a laboratory expectation value. Physical observables must be derived from the underlying density matrix, Green function, scattering state, or measurement protocol. This distinction prevents the effective eigenproblem from silently replacing the open-system experiment.

An exceptional point is a parameter value at which eigenvalues and their eigenvectors coalesce, making the effective operator defective. It differs from a Hermitian diabolic point, where degenerate eigenvectors can remain linearly independent and orthogonal.

Consider two reciprocal modes with complex bare frequencies

Ωj=ωj−i2γj\Omega_j = \omega_j - \frac{i}{2}\gamma_j

and a real conservative coupling g≥0g\geq0, whose sign is fixed by a mode-phase choice. Here H2H_2 is written in angular-frequency units: i∂ta=H2ai\partial_t\mathbf a=H_2\mathbf a, so the corresponding energy matrix is ℏH2\hbar H_2. Reciprocal dissipative coupling can also be complex and is not included in this example:

H2=(Ω1ggΩ2).H_2 = \begin{pmatrix} \Omega_1 & g \\ g & \Omega_2 \end{pmatrix}.

The eigenvalues are

z±=Ω1+Ω22±g2+(Ω1−Ω22)2.z_\pm = \frac{\Omega_1+\Omega_2}{2} \pm \sqrt{ g^2 + \left( \frac{\Omega_1-\Omega_2}{2} \right)^2 }.

The two eigenvalues coincide when the discriminant vanishes,

g2+(Ω1−Ω22)2=0.g^2 + \left( \frac{\Omega_1-\Omega_2}{2} \right)^2 = 0.

This repeated eigenvalue is an exceptional point only if H2H_2 is not a scalar multiple of the identity. For this model, g≠0g\ne0 ensures that the zero-discriminant matrix is defective. The case g=0g=0 and Ω1=Ω2\Omega_1=\Omega_2 instead has two independent eigenvectors.

If ω1=ω2\omega_1=\omega_2 and the loss rates are unequal, the exceptional point occurs at

g=∣γ1−γ2∣4.g = \frac{ \lvert\gamma_1-\gamma_2\rvert }{4}.

The nonzero coupling then leaves a one-dimensional eigenspace. Near a generic second-order exceptional point, a perturbation ϵ\epsilon produces

z+−z−∝ϵ.z_+-z_- \propto \sqrt{\epsilon}.

Because the discriminant is complex, two real conditions generally have to be satisfied. A generic second-order exceptional point therefore has codimension two unless a symmetry or constraint reduces the tuning requirement.

The square root gives two sheets. Encircling the exceptional point once in a two-parameter plane exchanges z+z_+ and z−z_-. A second loop returns the eigenvalue branch; the eigenvector may acquire an additional geometric phase depending on the path and normalization.

The two square-root eigenvalue branches follow opposite semicircles when the complex discriminant goes once around zero.

Local square-root model w±=z±−zEP=±λw_\pm=z_\pm-z_{\mathrm{EP}}=\pm\sqrt{\lambda}. As the discriminant follows λ=reiθ\lambda=re^{i\theta} through 0≤θ≤2π0\leq\theta\leq2\pi, the two eigenvalues exchange their initial positions. The loop does not pass through the degeneracy λ=0\lambda=0. This is analytic continuation of eigenvalues, not a prediction that a slowly evolving physical state follows the same path.

Static analytic continuation and dynamical encircling must be separated. In a lossy system, arbitrarily slow evolution need not follow an instantaneous eigenstate: differential decay and Stokes transitions can select one mode and produce direction-dependent transfer. Experiments by Doppler and collaborators and by Xu and collaborators demonstrated asymmetric mode conversion in microwave and optomechanical settings. Their dynamical outcomes contain the exceptional-point topology together with nonadiabatic open-system evolution.

Exceptional points from material lifetimes

Section titled “Exceptional points from material lifetimes”

Interactions and disorder give orbital-dependent self-energies. When two quasiparticle sectors have different lifetimes, the anti-Hermitian part of the self-energy can turn an ordinary band crossing into exceptional points connected by a locus where the real parts of the poles coincide. Kozii and Fu developed this finite-lifetime quasiparticle mechanism; dynamical mean-field calculations by Nagai and collaborators found corresponding bulk-arc structures in heavy-fermion models.

The inference remains spectral and model dependent. An intensity ridge that resembles an arc is not sufficient. One should reconstruct complex poles or a controlled self-energy, verify the defective points at the arc ends, and exclude matrix-element zeros, surface states, finite resolution, and ordinary lifetime-broadened crossings.

Non-Hermitian lattice spectra can depend strongly on boundary conditions. Under the non-Hermitian skin effect, an extensive number of right eigenmodes accumulate near a boundary, so periodic Bloch bands may fail to predict an open sample. A point-gap winding in one dimension can be defined by

ν(E0)=12πi∫BZdk ∂klog⁡det⁡ ⁣[H(k)−E0].\nu(E_0) = \frac{1}{2\pi i} \int_{\mathrm{BZ}} dk\, \partial_k \log\det\!\left[ H(k)-E_0 \right].

This invariant is meaningful only when the reference point E0E_0 lies outside the periodic complex spectrum. Open-boundary predictions may require a generalized, non-Bloch Brillouin zone (Kunst and collaborators, 2018; Bergholtz, Budich and Kunst, 2021). Boundary localization in a pumped or lossy experiment must also be distinguished from ordinary attenuation, source placement, defects, and finite propagation length.

An avoided crossing in frequency, a crossing in linewidth, or a change in intensity can suggest a two-mode non-Hermitian model. Stronger evidence tracks both real and imaginary pole components and tests eigenvector behavior.

Scattering poles and zeros are distinct. Coherent perfect absorption concerns a zero of a scattering eigenvalue; lasing concerns a pole reaching the real axis. Either can interact with exceptional structures, but neither is identical to an exceptional point.

Intensity-only spectra discard phase and can merge nearby modes. Complex scattering amplitudes, homodyne quadratures or time-domain ringdown provide more information. Fit the instrument response and backgrounds as well as the modes, and compare against a nondegenerate two-pole model over multiple fitting windows. Near a defective point, eigenvectors are ill conditioned and parameter uncertainties can be strongly correlated.

The square-root splitting Δz∝ϵ\Delta z\propto\sqrt{\epsilon} gives large eigenvalue responsivity to a small perturbation. Metrological precision also depends on linewidth, noise, integration time, estimator bias, technical drift, and the resources needed to hold the device near the exceptional point.

Chen and collaborators (2017) demonstrated enhanced splitting near an exceptional point. In the linear two-mode sensing models analyzed by Lau and Clerk (2018), noise and reciprocity constrain the attainable measurement rate; proximity to an exceptional point alone does not guarantee an advantage. Compare uncertainty in the inferred perturbation at fixed input resources, bandwidth, integration time and detection efficiency (see also Langbein, 2018).

For

GR(E)=1E−ε+iΓ/2,G^R(E) = \frac{1}{ E-\varepsilon+i\Gamma/2 },

derive the spectral function A(E)=−(1/π)Im⁡GR(E)A(E)=-(1/\pi)\operatorname{Im}G^R(E) and show that its integral over EE is one.

Solution

Multiplying by the complex conjugate denominator gives

GR(E)=E−ε−iΓ/2(E−ε)2+(Γ/2)2.G^R(E) = \frac{ E-\varepsilon-i\Gamma/2 }{ \left( E-\varepsilon \right)^2 + \left( \Gamma/2 \right)^2 }.

Therefore

A(E)=1πΓ/2(E−ε)2+(Γ/2)2.A(E) = \frac{1}{\pi} \frac{ \Gamma/2 }{ \left( E-\varepsilon \right)^2 + \left( \Gamma/2 \right)^2 }.

Using ∫−∞∞dx a/(x2+a2)=π\int_{-\infty}^{\infty}dx\,a/(x^2+a^2)=\pi gives ∫dE A(E)=1\int dE\,A(E)=1. A frequency-dependent self-energy redistributes weight between the pole and other spectral contributions. The full canonical spectral sum remains fixed, whereas a restricted energy window need not contain unit weight.

A two-level emitter has L=γ∣g⟩⟨e∣L=\sqrt{\gamma}\lvert g\rangle\langle e\rvert and H=0H=0. Starting in ∣e⟩\lvert e\rangle, find the unnormalized no-jump state and its squared norm.

Solution

Since

L†L=γ∣e⟩⟨e∣,L^\dagger L = \gamma \lvert e\rangle\langle e\rvert,

the conditional generator is

Heff=−iℏγ2∣e⟩⟨e∣.H_{\mathrm{eff}} = -\frac{i\hbar\gamma}{2} \lvert e\rangle\langle e\rvert.

Thus

∣ψ~(t)⟩=e−γt/2∣e⟩,⟨ψ~(t)∣ψ~(t)⟩=e−γt.\lvert\tilde\psi(t)\rangle = e^{-\gamma t/2} \lvert e\rangle, \qquad \langle\tilde\psi(t)\vert\tilde\psi(t)\rangle = e^{-\gamma t}.

The squared norm is the probability that no photon has been detected up to time tt under the ideal monitoring assumed here. The unconditional state also contains the ground-state population created by jump records.

For equal bare frequencies ω1=ω2=ω0\omega_1=\omega_2=\omega_0, derive the exceptional-point condition with the convention g≥0g\geq0 and unequal loss rates. Explain why the equal-loss, zero-coupling limit is not exceptional.

Solution

The complex-frequency difference is

Ω1−Ω2=−i2(γ1−γ2).\Omega_1-\Omega_2 = -\frac{i}{2} \left( \gamma_1-\gamma_2 \right).

The discriminant becomes

g2−(γ1−γ2)216.g^2 - \frac{ \left( \gamma_1-\gamma_2 \right)^2 }{16}.

It vanishes at

g=∣γ1−γ2∣4.g = \frac{ \lvert\gamma_1-\gamma_2\rvert }{4}.

Because the losses differ, this coupling is nonzero and H2−zIH_2-zI has rank one at the repeated eigenvalue zz. Its eigenspace is therefore one-dimensional: the point is exceptional. If the losses are equal, the zero-discriminant condition instead gives g=0g=0 and H2=(ω0−iγ/2)IH_2=(\omega_0-i\gamma/2)I, which has a two-dimensional eigenspace. Equality of eigenvalues alone is not sufficient.

Let z±(λ)=±λz_\pm(\lambda)=\pm\sqrt{\lambda} and take λ=reiθ\lambda=re^{i\theta}. What happens as θ\theta advances from 00 to 2π2\pi, and then to 4π4\pi?

Solution

Choose

z±=±r eiθ/2.z_\pm = \pm \sqrt r\, e^{i\theta/2}.

After one loop,

ei(θ+2π)/2=−eiθ/2,e^{i(\theta+2\pi)/2} = -e^{i\theta/2},

so z+z_+ continues onto z−z_- and vice versa. After a second loop the eigenvalue returns to its original branch. The associated eigenvector can acquire an additional geometric phase; that phase must be calculated with a declared normalization and path.

In the two-state rate model, suppose κp(L)=D/L2\kappa_p(L)=D/L^2 and the total error rate γe\gamma_e is size independent. Find the error-free preparation time and the stationary infidelity with errors. Why should the large-LL relaxation time not be confused with successful preparation?

Solution

With γe=0\gamma_e=0, 1−F(t)=[1−F(0)]e−Dt/L21-F(t)=[1-F(0)]e^{-Dt/L^2}, so a fixed accuracy requires a time proportional to L2/DL^2/D. With errors,

1−Fss=γeL2D+γeL2,τrelax=1D/L2+γe.1-F_{\mathrm{ss}}=\frac{\gamma_e L^2}{D+\gamma_e L^2}, \qquad \tau_{\mathrm{relax}}=\frac{1}{D/L^2+\gamma_e}.

Weak errors give 1−Fss≃γeL2/D1-F_{\mathrm{ss}}\simeq\gamma_e L^2/D. At large LL, the relaxation time approaches 1/γe1/\gamma_e, but the stationary fidelity approaches zero: the system reaches a bad state quickly. This two-state example does not establish the preparation scaling of a particular many-body protocol.

For current questions about interacting systems and sensing performance, see Non-Hermitian and PT-symmetric frontiers and Dissipation Engineering.