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Pure Dephasing Model

A pure dephasing model is an open-system model in which the environment destroys relative phases between preferred alternatives without changing their populations. It is exactly solvable when the system operator coupled to the environment commutes with the system Hamiltonian.

The model is valuable because it separates three ideas that are often blended together:

  • loss of coherence in a chosen basis;
  • absence of energy relaxation in that basis;
  • non-Markovian memory in the coherence factor.

The Markovian generator version is Pure Dephasing Master Equation. The finite-time channel version is Dephasing Channel. This page is the exactly solvable model behind both when the microscopic assumptions are simple enough.

Let the system Hamiltonian and coupling operator share an eigenbasis:

HS∣m⟩=Em∣m⟩,A∣m⟩=am∣m⟩.H_S\lvert m\rangle = E_m\lvert m\rangle, \qquad A\lvert m\rangle = a_m\lvert m\rangle.

The pure dephasing Hamiltonian is

H=HS+HB+A⊗B,H = H_S + H_B + A\otimes B,

with

[A,HS]=0.[A,H_S]=0.

Because the interaction is diagonal in the energy basis, it cannot by itself move the system from ∣m⟩\lvert m\rangle to ∣n⟩\lvert n\rangle. It can, however, make different basis states imprint different phases and different bath states.

Equivalently, the full Hamiltonian can be written as a conditional bath Hamiltonian:

H=∑m∣m⟩⟨m∣⊗(EmIB+HB+amB).H = \sum_m \lvert m\rangle\langle m\rvert \otimes \left( E_m I_B+H_B+a_m B \right).

Each system alternative makes the bath evolve under a different Hamiltonian.

Assume an initially factorized state,

ρ(0)=ρS(0)⊗ρB.\rho(0) = \rho_S(0)\otimes\rho_B.

For a system basis state ∣m⟩\lvert m\rangle, define the conditional bath unitary

Um(t)=exp⁡[−iℏ(HB+amB)t].U_m(t) = \exp \left[ -\frac{i}{\hbar} \left( H_B+a_m B \right)t \right].

Then the reduced density-matrix elements evolve as

ρmn(t)=e−i(Em−En)t/ℏχmn(t)ρmn(0),\rho_{mn}(t) = e^{-i(E_m-E_n)t/\hbar} \chi_{mn}(t) \rho_{mn}(0),

where the coherence factor is

χmn(t)=Tr⁡B[Um(t)ρBUn†(t)].\chi_{mn}(t) = \operatorname{Tr}_B \left[ U_m(t)\rho_B U_n^\dagger(t) \right].

Diagonal elements have m=nm=n, so χmm(t)=1\chi_{mm}(t)=1 and

ρmm(t)=ρmm(0).\rho_{mm}(t)=\rho_{mm}(0).

Off-diagonal elements decay when the two conditional bath histories become distinguishable. The factor χmn(t)\chi_{mn}(t) is a Loschmidt-echo-like overlap of bath evolutions. Its magnitude measures retained coherence; its phase contributes a bath-induced energy shift.

For a qubit in the dephasing basis, a common Hamiltonian is

H=ϵ2σz+HB+σz2B.H = \frac{\epsilon}{2}\sigma_z + H_B + \frac{\sigma_z}{2}B.

The two conditional bath Hamiltonians are

H±=HB±12B.H_\pm = H_B \pm \frac12 B.

The populations in the σz\sigma_z basis are constant, while the coherence obeys

ρ+,−(t)=e−iϵt/ℏχ(t)ρ+,−(0),\rho_{+,-}(t) = e^{-i\epsilon t/\hbar} \chi(t)\rho_{+,-}(0),

with

χ(t)=Tr⁡B[e−iH+t/ℏρBeiH−t/ℏ].\chi(t) = \operatorname{Tr}_B \left[ e^{-iH_+t/\hbar} \rho_B e^{iH_-t/\hbar} \right].

If ∣χ(t)∣=e−Γϕt|\chi(t)|=e^{-\Gamma_\phi t} over the time window of interest, the model reduces to a Markovian exponential dephasing law. If ∣χ(t)∣|\chi(t)| is Gaussian, algebraic, oscillatory, or partially reviving, a one-rate Markovian description is not faithful.

A classical version replaces the bath operator by a stochastic frequency fluctuation:

H(t)=HS+A ξ(t).H(t) = H_S + A\,\xi(t).

For one noise realization, the evolution is unitary. After averaging over realizations,

ρmn(t)=e−i(Em−En)t/ℏ⟨e−iϕmn(t)⟩ρmn(0),\rho_{mn}(t) = e^{-i(E_m-E_n)t/\hbar} \left\langle e^{-i\phi_{mn}(t)} \right\rangle \rho_{mn}(0),

where

ϕmn(t)=am−anℏ∫0tds ξ(s).\phi_{mn}(t) = \frac{a_m-a_n}{\hbar} \int_0^t ds\,\xi(s).

If ξ(t)\xi(t) is zero-mean Gaussian noise with correlation

C(τ)=⟨ξ(τ)ξ(0)⟩,C(\tau) = \langle \xi(\tau)\xi(0)\rangle,

then

⟨e−iϕmn(t)⟩=exp⁡[−Γmn(t)],\left\langle e^{-i\phi_{mn}(t)} \right\rangle = \exp[-\Gamma_{mn}(t)],

with

Γmn(t)=(am−an)22ℏ2∫0tds∫0tds′ C(s−s′).\Gamma_{mn}(t) = \frac{(a_m-a_n)^2}{2\hbar^2} \int_0^t ds \int_0^t ds'\, C(s-s').

This formula is often the simplest bridge between noise measurements and dephasing envelopes.

For stationary classical Gaussian noise, write

C(τ)=∫−∞∞dω2π e−iωτSξξ(ω).C(\tau) = \int_{-\infty}^{\infty} \frac{d\omega}{2\pi}\, e^{-i\omega\tau} S_{\xi\xi}(\omega).

Then

Γmn(t)=(am−an)22ℏ2∫−∞∞dω2π Sξξ(ω)∣∫0tds e−iωs∣2.\Gamma_{mn}(t) = \frac{(a_m-a_n)^2}{2\hbar^2} \int_{-\infty}^{\infty} \frac{d\omega}{2\pi}\, S_{\xi\xi}(\omega) \left| \int_0^t ds\,e^{-i\omega s} \right|^2.

Since

∣∫0tds e−iωs∣2=4sin⁡2(ωt/2)ω2,\left| \int_0^t ds\,e^{-i\omega s} \right|^2 = \frac{4\sin^2(\omega t/2)}{\omega^2},

the coherence envelope samples noise through a filter centered near zero frequency. Control pulses replace the constant integrand by a sign-changing modulation function; that is the entry point to Dynamical Decoupling.

For white noise,

C(τ)=D δ(τ),C(\tau)=D\,\delta(\tau),

one finds exponential decay:

Γmn(t)=(am−an)2D2ℏ2t.\Gamma_{mn}(t) = \frac{(a_m-a_n)^2D}{2\hbar^2}t.

For quasi-static Gaussian noise with ξ\xi constant during each run but distributed with variance σ2\sigma^2,

Γmn(t)=(am−an)2σ22ℏ2t2.\Gamma_{mn}(t) = \frac{(a_m-a_n)^2\sigma^2}{2\hbar^2}t^2.

The first is a Markovian-looking irreversible envelope. The second is inhomogeneous broadening and can often be refocused by echo sequences.

The pure-dephasing limit of the spin-boson model sets the tunneling amplitude to zero. A common qubit-bath Hamiltonian is

H=ϵ2σz+∑kℏωkbk†bk+σz2∑kgk(bk+bk†).H = \frac{\epsilon}{2}\sigma_z + \sum_k \hbar\omega_k b_k^\dagger b_k + \frac{\sigma_z}{2} \sum_k g_k \left( b_k+b_k^\dagger \right).

This is exactly solvable because σz\sigma_z is conserved. In one common continuum convention, define

J(ω)=π∑kgk2δ(ω−ωk),ω>0.J(\omega) = \pi \sum_k g_k^2 \delta(\omega-\omega_k), \qquad \omega>0.

For a thermal Gaussian oscillator bath, the qubit coherence has the form

ρ+,−(t)=ρ+,−(0)e−iϵt/ℏe−Φ(t)eiΘ(t).\rho_{+,-}(t) = \rho_{+,-}(0) e^{-i\epsilon t/\hbar} e^{-\Phi(t)} e^{i\Theta(t)}.

The dephasing exponent is

Φ(t)=1π∫0∞dω J(ω)ω2[1−cos⁡(ωt)]coth⁡(βℏω2).\Phi(t) = \frac{1}{\pi} \int_0^\infty d\omega\, \frac{J(\omega)}{\omega^2} \left[ 1-\cos(\omega t) \right] \coth \left( \frac{\beta\hbar\omega}{2} \right).

The phase Θ(t)\Theta(t) depends on counterterm and bias-renormalization conventions, so the robust decoherence content is usually the magnitude e−Φ(t)e^{-\Phi(t)}. The same spectral density controls how low-frequency bath weight dephases the qubit.

Take an Ohmic zero-temperature spectrum in the convention

J(ω)=2πα ωe−ω/ωc.J(\omega) = 2\pi\alpha\,\omega e^{-\omega/\omega_c}.

Then

Φ(t)=2α∫0∞dω e−ω/ωc1−cos⁡(ωt)ω.\Phi(t) = 2\alpha \int_0^\infty d\omega\, e^{-\omega/\omega_c} \frac{1-\cos(\omega t)}{\omega}.

Using

∫0∞dω e−aω1−cos⁡(bω)ω=12ln⁡(1+b2a2),\int_0^\infty d\omega\, e^{-a\omega} \frac{1-\cos(b\omega)}{\omega} = \frac12 \ln \left( 1+\frac{b^2}{a^2} \right),

with a=1/ωca=1/\omega_c and b=tb=t, one obtains

Φ(t)=αln⁡(1+ωc2t2).\Phi(t) = \alpha \ln \left( 1+\omega_c^2t^2 \right).

Thus the zero-temperature Ohmic pure-dephasing envelope is algebraic:

e−Φ(t)=(1+ωc2t2)−α.e^{-\Phi(t)} = \left( 1+\omega_c^2t^2 \right)^{-\alpha}.

This is not a Markovian exponential. At finite temperature, the long-time envelope becomes exponential in many Ohmic models, with a rate set by temperature and coupling convention.

A pure-dephasing model reduces to a Lindblad pure-dephasing master equation when the coherence factor is approximately exponential over the times being modeled:

χmn(t)≈e−iδωmnte−γmnt.\chi_{mn}(t) \approx e^{-i\delta\omega_{mn}t} e^{-\gamma_{mn}t}.

Then

ρmn(t)≈e−i(Em−En)t/ℏe−iδωmnte−γmntρmn(0).\rho_{mn}(t) \approx e^{-i(E_m-E_n)t/\hbar} e^{-i\delta\omega_{mn}t} e^{-\gamma_{mn}t} \rho_{mn}(0).

For a Hermitian Lindblad operator LL with eigenvalues ℓm\ell_m, the Markovian generator

ρ˙=γD[L]ρ\dot\rho = \gamma\mathcal D[L]\rho

gives

γmn=γ2(ℓm−ℓn)2.\gamma_{mn} = \frac{\gamma}{2} (\ell_m-\ell_n)^2.

This is a useful effective model, but it should not be assumed when the measured coherence has Gaussian decay, power-law decay, revivals, or strong dependence on pulse sequence.

Pure dephasing is environmental distinguishability without population transfer. If two system alternatives make the environment evolve to nearly identical states, their coherence remains. If they make the environment evolve to nearly orthogonal states, their coherence is lost in the reduced state.

This interpretation does not require a human observer or a classical apparatus. It follows from tracing over degrees of freedom that carry which-alternative information.

The basis is part of the model. Pure dephasing in the σz\sigma_z basis may be relaxation in the energy basis if the Hamiltonian contains a transverse term. This is why the full Spin-Boson Model distinguishes localized and energy bases.

  • Calling every loss of Ramsey contrast irreversible dephasing.
  • Forgetting that pure dephasing is basis-dependent.
  • Replacing a nonexponential coherence envelope by a constant rate without checking the time window.
  • Treating quasi-static disorder as a Markovian bath.
  • Ignoring the imaginary phase of χmn(t)\chi_{mn}(t) when it shifts transition frequencies.
  • Applying the Δ=0\Delta=0 spin-boson solution when the Hamiltonian has a transverse term that causes relaxation.
  • Comparing formulas for Φ(t)\Phi(t) without checking the convention for J(ω)J(\omega).
  • Assuming classical noise and quantum bath models are physically identical just because they give the same coherence envelope.
  • H.-P. Breuer and F. Petruccione, The Theory of Open Quantum Systems, Oxford University Press (2002).
  • U. Weiss, Quantum Dissipative Systems, 4th ed., World Scientific (2012).
  • A. J. Leggett, S. Chakravarty, A. T. Dorsey, M. P. A. Fisher, A. Garg, and W. Zwerger, “Dynamics of the dissipative two-state system,” Reviews of Modern Physics 59, 1–85 (1987).
  • M. Schlosshauer, Decoherence and the Quantum-to-Classical Transition, Springer (2007).
  • G. Ithier et al., “Decoherence in a superconducting quantum bit circuit,” Physical Review B 72, 134519 (2005).
  • E. Paladino, Y. M. Galperin, G. Falci, and B. L. Altshuler, “1/f noise: Implications for solid-state quantum information,” Reviews of Modern Physics 86, 361–418 (2014).
  • L. Cywiński, R. M. Lutchyn, C. P. Nave, and S. Das Sarma, “How to enhance dephasing time in superconducting qubits,” Physical Review B 77, 174509 (2008).

Starting from

H=∑m∣m⟩⟨m∣⊗(EmIB+HB+amB),H = \sum_m \lvert m\rangle\langle m\rvert \otimes \left( E_m I_B+H_B+a_m B \right),

derive the coherence factor χmn(t)\chi_{mn}(t).

Solution

The full unitary is block diagonal:

U(t)=∑me−iEmt/ℏ∣m⟩⟨m∣⊗Um(t),U(t) = \sum_m e^{-iE_mt/\hbar} \lvert m\rangle\langle m\rvert \otimes U_m(t),

with

Um(t)=exp⁡[−iℏ(HB+amB)t].U_m(t) = \exp \left[ -\frac{i}{\hbar} \left( H_B+a_mB \right)t \right].

For an initially factorized state, the mnmn reduced matrix element is

ρmn(t)=e−i(Em−En)t/ℏρmn(0)Tr⁡B[Um(t)ρBUn†(t)].\rho_{mn}(t) = e^{-i(E_m-E_n)t/\hbar} \rho_{mn}(0) \operatorname{Tr}_B \left[ U_m(t)\rho_B U_n^\dagger(t) \right].

Thus

χmn(t)=Tr⁡B[Um(t)ρBUn†(t)].\chi_{mn}(t) = \operatorname{Tr}_B \left[ U_m(t)\rho_B U_n^\dagger(t) \right].

Use the exact solution to show that ρmm(t)=ρmm(0)\rho_{mm}(t)=\rho_{mm}(0).

Solution

Set m=nm=n in the exact solution. The Hamiltonian phase is unity, and

χmm(t)=Tr⁡B[Um(t)ρBUm†(t)].\chi_{mm}(t) = \operatorname{Tr}_B \left[ U_m(t)\rho_B U_m^\dagger(t) \right].

By cyclicity of the trace and unitarity,

χmm(t)=Tr⁡B(ρB)=1.\chi_{mm}(t) = \operatorname{Tr}_B(\rho_B) = 1.

Therefore ρmm(t)=ρmm(0)\rho_{mm}(t)=\rho_{mm}(0).

For classical Gaussian phase noise, compare C(τ)=Dδ(τ)C(\tau)=D\delta(\tau) with a quasi-static random variable of variance σ2\sigma^2.

Solution

The Gaussian dephasing exponent is

Γmn(t)=(am−an)22ℏ2∫0tds∫0tds′ C(s−s′).\Gamma_{mn}(t) = \frac{(a_m-a_n)^2}{2\hbar^2} \int_0^t ds \int_0^t ds'\, C(s-s').

For white noise,

∫0tds∫0tds′ Dδ(s−s′)=Dt,\int_0^t ds \int_0^t ds'\, D\delta(s-s') = Dt,

so the envelope is exponential. For quasi-static noise, C(s−s′)=σ2C(s-s')=\sigma^2 over one run, so

∫0tds∫0tds′ σ2=σ2t2,\int_0^t ds \int_0^t ds'\, \sigma^2 = \sigma^2t^2,

and the envelope is Gaussian in time. The quasi-static case is reversible in principle by echo techniques, while ideal white-noise decay is not.

Show that for

J(ω)=2πα ωe−ω/ωc,J(\omega) = 2\pi\alpha\,\omega e^{-\omega/\omega_c},

the zero-temperature exponent is Φ(t)=αln⁡(1+ωc2t2)\Phi(t)=\alpha\ln(1+\omega_c^2t^2) in the convention used on this page.

Solution

At zero temperature, coth⁡(βℏω/2)→1\coth(\beta\hbar\omega/2)\to1. Substitute the Ohmic J(ω)J(\omega) into

Φ(t)=1π∫0∞dω J(ω)ω2[1−cos⁡(ωt)].\Phi(t) = \frac{1}{\pi} \int_0^\infty d\omega\, \frac{J(\omega)}{\omega^2} \left[ 1-\cos(\omega t) \right].

This gives

Φ(t)=2α∫0∞dω e−ω/ωc1−cos⁡(ωt)ω.\Phi(t) = 2\alpha \int_0^\infty d\omega\, e^{-\omega/\omega_c} \frac{1-\cos(\omega t)}{\omega}.

Using

∫0∞dω e−aω1−cos⁡(bω)ω=12ln⁡(1+b2a2),\int_0^\infty d\omega\, e^{-a\omega} \frac{1-\cos(b\omega)}{\omega} = \frac12 \ln \left( 1+\frac{b^2}{a^2} \right),

with a=1/ωca=1/\omega_c and b=tb=t yields

Φ(t)=αln⁡(1+ωc2t2).\Phi(t) = \alpha \ln \left( 1+\omega_c^2t^2 \right).