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High-Frequency Expansions

A high-frequency expansion replaces rapid periodic driving by a slowly acting effective Hamiltonian together with a periodic micromotion transformation. It is useful when a Hamiltonian

H(t+T)=H(t),Ω=2πT,H(t+T)=H(t), \qquad \Omega=\frac{2\pi}{T},

contains a drive frequency whose quantum ℏΩ\hbar\Omega is large compared with the energy scales that couple relevant states. The leading approximation is often the period average. Higher orders retain virtual absorption and emission processes through commutators divided by powers of ℏΩ\hbar\Omega.

This page is the canonical home for the general inverse-frequency method, especially the van Vleck organization, its relation to Floquet-space block diagonalization, the separation of effective evolution from micromotion, and the prethermal interpretation in local many-body systems. Floquet Theorem in Quantum Mechanics owns the exact theorem. Magnus Expansion owns the general exponential series, while Floquet–Magnus Expansion owns the direct one-period Magnus construction at a chosen drive phase. Driven Many-Body Systems owns the broader absorption ledger and driven–dissipative distinction. Floquet Systems Preview owns the many-body regime map, Floquet ETH, engineering evidence, and emergent periodic phases. Floquet Quantum Matter supplies the materials-facing waveform, spectroscopy, topology, and lifetime evidence ledger.

The phrase high frequency is relational. A large numerical value of Ω\Omega is not enough: one must identify the matrix elements, bandwidths, detunings, local interaction scales, populated energy window, and observation time against which it is large.

Use the Fourier decomposition

H(t)=∑m∈ZHmeimΩt,H(t) = \sum_{m\in\mathbb Z} H_m e^{im\Omega t},

with

Hm=1T∫0Te−imΩtH(t) dt.H_m = \frac{1}{T} \int_0^T e^{-im\Omega t}H(t)\,dt.

Hermiticity of H(t)H(t) implies

H−m=Hm†.H_{-m}=H_m^\dagger.

The zero mode is the period average,

H0=1T∫0TH(t) dt.H_0 = \frac{1}{T} \int_0^T H(t)\,dt.

Fixing the sign in the Fourier exponential is essential. Reversing that convention reverses the order of several commutators. Formulas from different sources should therefore never be combined until their Fourier and micromotion conventions have been translated.

Floquet modes solve the quasienergy eigenvalue problem

(H(t)−iℏ∂t)∣uα(t)⟩=εα∣uα(t)⟩.\left( H(t)-i\hbar\partial_t \right) \lvert u_\alpha(t)\rangle = \varepsilon_\alpha \lvert u_\alpha(t)\rangle.

It is useful to regard the quasienergy operator

Q≡H(t)−iℏ∂t\mathcal Q \equiv H(t)-i\hbar\partial_t

as a time-independent operator on the extended space of TT-periodic functions. In the basis

∣α,m⟩ ⁣⟩=∣α⟩eimΩt,\lvert \alpha,m\rangle\!\rangle = \lvert\alpha\rangle e^{im\Omega t},

its blocks are

⟨ ⁣⟨α′,m′∣Q∣α,m⟩ ⁣⟩=⟨α′∣Hm′−m∣α⟩+δm′mδα′αmℏΩ.\begin{aligned} & \langle\!\langle \alpha',m' \rvert \mathcal Q \lvert \alpha,m \rangle\!\rangle \\ &\quad= \langle\alpha'| H_{m'-m} |\alpha\rangle \\ &\qquad+ \delta_{m'm}\delta_{\alpha'\alpha} m\hbar\Omega. \end{aligned}

The diagonal sectors are displaced by mℏΩm\hbar\Omega. A Fourier component HrH_r couples sectors whose photon labels differ by rr. The word photon is convenient bookkeeping here; the periodic drive need not be a quantized electromagnetic field.

Floquet-space sectors separated by drive quanta and their block diagonalization into copies of an effective Hamiltonian

At large ℏΩ\hbar\Omega, Fourier harmonics couple well-separated Floquet sectors. The shaded m=0m=0 sector is retained. A perturbative block diagonalization produces repeated copies Heff+mℏΩH_{\mathrm{eff}}+m\hbar\Omega, while the periodic kick operator K(t)K(t) restores the inter-sector admixture as micromotion.

This is an energy-space version of scale separation. Eliminating remote Floquet sectors is closely analogous to a Schrieffer–Wolff Transformation. The large denominators are now multiples of ℏΩ\hbar\Omega, and the eliminated admixture reappears as micromotion rather than disappearing from the physical state.

A useful exact factorization is

U(t,t0)=e−iK(t)e−iHeff(t−t0)/ℏeiK(t0).U(t,t_0) = e^{-iK(t)} e^{-iH_{\mathrm{eff}}(t-t_0)/\hbar} e^{iK(t_0)}.

Here:

  • HeffH_{\mathrm{eff}} is time independent;
  • K(t)=K(t+T)K(t)=K(t+T) is a Hermitian kick or micromotion generator;
  • the exponentials e−iK(t)e^{-iK(t)} are periodic unitary transformations.

This decomposition is not unique. A constant unitary change of effective frame transforms HeffH_{\mathrm{eff}}, K(t)K(t), states, and observables together without changing laboratory predictions. A common van Vleck gauge chooses the micromotion generator to have zero period average order by order.

At a fixed sampling phase t0t_0, the one-period propagator is

U(t0+T,t0)=e−iK(t0)e−iHeffT/ℏeiK(t0).U(t_0+T,t_0) = e^{-iK(t_0)} e^{-iH_{\mathrm{eff}}T/\hbar} e^{iK(t_0)}.

Thus a stroboscopic Floquet Hamiltonian on a compatible logarithm branch is

HF(t0)=e−iK(t0)HeffeiK(t0).H_F(t_0) = e^{-iK(t_0)} H_{\mathrm{eff}} e^{iK(t_0)}.

The spectrum is independent of the sampling phase, but the operator representative and its eigenvectors are dressed by micromotion.

An effective-frame state at the initial phase is

∣ψeff(t0)⟩=eiK(t0)∣ψ(t0)⟩.\lvert\psi_{\mathrm{eff}}(t_0)\rangle = e^{iK(t_0)} \lvert\psi(t_0)\rangle.

For a laboratory observable OO, the corresponding time-periodic effective-frame observable is

Oeff(t)=eiK(t)Oe−iK(t).O_{\mathrm{eff}}(t) = e^{iK(t)} O e^{-iK(t)}.

Using HeffH_{\mathrm{eff}} while leaving the initial state and observable undressed generally loses terms at the same order as the Hamiltonian correction being retained. Stroboscopic questions at a specially chosen phase can simplify the dressing, but they do not abolish it.

Write

Heff=Heff(0)+Heff(1)+Heff(2)+⋯ ,H_{\mathrm{eff}} = H_{\mathrm{eff}}^{(0)} + H_{\mathrm{eff}}^{(1)} + H_{\mathrm{eff}}^{(2)} +\cdots,

where the superscript denotes the power of Ω−1\Omega^{-1} in the convention used here. The leading term is

Heff(0)=H0.H_{\mathrm{eff}}^{(0)}=H_0.

The first correction is

Heff(1)=∑m=1∞[Hm,H−m]mℏΩ.H_{\mathrm{eff}}^{(1)} = \sum_{m=1}^{\infty} \frac{ [H_m,H_{-m}] }{ m\hbar\Omega }.

Equivalently,

Heff(1)=∑m≠0HmH−mmℏΩ.H_{\mathrm{eff}}^{(1)} = \sum_{m\ne0} \frac{ H_mH_{-m} }{ m\hbar\Omega }.

The second form becomes the first after pairing mm with −m-m. It should not be replaced by an unrestricted commutator sum without a compensating factor of 1/21/2.

At order Ω−2\Omega^{-2}, the van Vleck result is

Heff(2)=∑m≠0[H−m,[H0,Hm]]2(mℏΩ)2+∑m≠0n≠0, n≠m[H−n,[Hn−m,Hm]]3mn(ℏΩ)2.\begin{aligned} H_{\mathrm{eff}}^{(2)} ={}& \sum_{m\ne0} \frac{ [H_{-m},[H_0,H_m]] }{ 2(m\hbar\Omega)^2 } \\ &+ \sum_{\substack{m\ne0\\n\ne0,\ n\ne m}} \frac{ [H_{-n},[H_{n-m},H_m]] }{ 3mn(\hbar\Omega)^2 }. \end{aligned}

Different papers shift the order labels by one, calling H0H_0 the first-order term. The powers of Ω−1\Omega^{-1}, not the superscript alone, identify the approximation.

The leading kick operator is

K(1)(t)=−i∑m≠0HmeimΩtmℏΩ.K^{(1)}(t) = -i \sum_{m\ne0} \frac{ H_m e^{im\Omega t} }{ m\hbar\Omega }.

It is Hermitian because H−m=Hm†H_{-m}=H_m^\dagger. Its norm is typically of order drive amplitude divided by ℏΩ\hbar\Omega, making micromotion small in the simplest off-resonant regime even when its repeated effect on observables remains important.

The period average discards every nonzero Fourier harmonic. The first correction remembers the order in which noncommuting pieces act. A virtual process can move from one Floquet sector to another through HmH_m and return through H−mH_{-m}. Reversing the order gives a different amplitude, and their difference is precisely a commutator.

If every HmH_m commutes with every other relevant component, time ordering is ineffective and the average can be exact. Rapid oscillation alone is not the mechanism; rapid oscillation together with off-resonant virtual mixing is.

Consider first a single Hermitian modulation,

H(t)=H0+AXcos⁡Ωt,X=X†.H(t)=H_0+A X\cos\Omega t, \qquad X=X^\dagger.

Its nonzero harmonics are

H1=H−1=A2X.H_1=H_{-1}=\frac{A}{2}X.

Therefore

[H1,H−1]=0,[H_1,H_{-1}]=0,

and the order-Ω−1\Omega^{-1} correction vanishes. The leading nonzero correction can occur at order Ω−2\Omega^{-2} through nested commutators involving H0H_0.

Now take a circularly rotating two-level drive,

H(t)=H0+A(σxcos⁡Ωt+σysin⁡Ωt).H(t) = H_0 + A\left( \sigma_x\cos\Omega t + \sigma_y\sin\Omega t \right).

Using σ±=(σx±iσy)/2\sigma_\pm=(\sigma_x\pm i\sigma_y)/2 gives

H1=Aσ−,H−1=Aσ+.H_1=A\sigma_-, \qquad H_{-1}=A\sigma_+.

Since

[σ−,σ+]=−σz,[\sigma_-,\sigma_+]=-\sigma_z,

the leading effective Hamiltonian is

Heff=H0−A2ℏΩσz+O(Ω−2).H_{\mathrm{eff}} = H_0 - \frac{A^2}{\hbar\Omega}\sigma_z + O(\Omega^{-2}).

The drive has zero average, yet its two quadratures do not commute. Their oriented cycle generates a static term whose sign reverses when the sense of rotation is reversed.

Several constructions are often grouped under the phrase high-frequency expansion. They agree on physical predictions through a consistent order but organize the effective frame differently.

ConstructionPrimary objectCharacteristic feature
MagnusU(t,t0)=eΞ(t,t0)U(t,t_0)=e^{\Xi(t,t_0)}General time-ordered exponential, not restricted to periodic driving
Floquet–Magnuslog⁡U(t0+T,t0)\log U(t_0+T,t_0)Direct stroboscopic generator tied to the phase t0t_0
van VleckHeffH_{\mathrm{eff}} and K(t)K(t)Drive-phase-independent effective Hamiltonian with micromotion separated
Brillouin–WignerProjected Floquet-space eigenproblemEliminates remote photon sectors through a wave operator or resolvent

Expanding the exact relation between HF(t0)H_F(t_0) and HeffH_{\mathrm{eff}} gives

HF(t0)=Heff+∑m≠0eimΩt0mℏΩ[H0,Hm]+O(Ω−2).\begin{aligned} H_F(t_0) ={}& H_{\mathrm{eff}} \\ &+ \sum_{m\ne0} \frac{e^{im\Omega t_0}} {m\hbar\Omega} [H_0,H_m] \\ &+ O(\Omega^{-2}). \end{aligned}

The second line records the micromotion dressing at the chosen phase. An exact shift of the drive origin changes HF(t0)H_F(t_0) by unitary conjugation and leaves its spectrum invariant. A finite Floquet–Magnus truncation can display apparent drive-phase dependence if the Hamiltonian and micromotion pieces are not kept consistently.

Brillouin–Wigner, van Vleck, and Schrieffer–Wolff-style block diagonalizations can produce different off-shell matrix elements or normalization conventions. Their truncated operators should not be spliced term by term. Compare quasienergies and dressed observables through the claimed order.

A laboratory-frame expansion can fail even when a better periodic frame is controlled. For a periodic unitary R(t)R(t), define

HR(t)=R†(t)H(t)R(t)−iℏR†(t)R˙(t).H_R(t) = R^\dagger(t)H(t)R(t) - i\hbar R^\dagger(t)\dot R(t).

One should choose R(t)R(t) exactly, recompute the Fourier components of HR(t)H_R(t), and only then identify a small inverse-frequency parameter.

This is especially important in two situations:

  • a large drive amplitude scales with ℏΩ\hbar\Omega and should be absorbed nonperturbatively;
  • the laboratory drive is near resonance with a large static splitting and a rotating frame exposes small detuning and slow couplings.

The first case appears in a shaken tight-binding chain. Consider

H(t)=−J∑j(cj+1†cj+cj†cj+1)+Kcos⁡Ωt∑jjnj.\begin{aligned} H(t) ={}& -J \sum_j \left( c_{j+1}^\dagger c_j + c_j^\dagger c_{j+1} \right) \\ &+ K\cos\Omega t \sum_j j n_j. \end{aligned}

With

κ=KℏΩ,\kappa=\frac{K}{\hbar\Omega},

the periodic transformation

R(t)=exp⁡[−iκsin⁡Ωt∑jjnj]R(t) = \exp\left[ -i\kappa\sin\Omega t \sum_j jn_j \right]

removes the oscillating potential exactly. It replaces the hopping by a phase eiκsin⁡Ωte^{i\kappa\sin\Omega t}. The leading average is therefore

Jeff=JJ0(κ),J_{\mathrm{eff}} = J\mathcal J_0(\kappa),

where J0\mathcal J_0 is a Bessel function. This approximation can be nonperturbative in κ\kappa while remaining perturbative in J/(ℏΩ)J/(\hbar\Omega). Calling it merely a weak-drive expansion would miss the useful regime.

Near a true resonance, the correct strategy is different: retain the resonant Floquet sectors together or transform to a frame where their small detuning is explicit. The Rotating-Wave Approximation then organizes near-resonant slow dynamics; an off-resonant high-frequency expansion can be applied only to the remaining fast terms.

No single norm ratio decides every high-frequency problem. A trustworthy calculation uses several complementary checks.

A practical first diagnostic is

ηK≡∑m≠0∥Hm∥∣m∣ℏΩ.\eta_K \equiv \sum_{m\ne0} \frac{\|H_m\|} {|m|\hbar\Omega}.

When ηK≪1\eta_K\ll1, the leading kick is small in the chosen frame. This condition is conservative and sufficient only in limited settings. It does not by itself rule out resonances or control long-time many-body heating.

If H0∣a⟩=Ea∣a⟩H_0\lvert a\rangle=E_a\lvert a\rangle, a harmonic HmH_m can connect ∣b,0⟩ ⁣⟩\lvert b,0\rangle\!\rangle to ∣a,m⟩ ⁣⟩\lvert a,m\rangle\!\rangle with detuning

Δab(m)=Ea−Eb+mℏΩ.\Delta_{ab}^{(m)} = E_a-E_b+m\hbar\Omega.

The relevant ratio is

∣⟨a∣Hm∣b⟩∣∣Δab(m)∣.\frac{ |\langle a|H_m|b\rangle| }{ |\Delta_{ab}^{(m)}| }.

If a coupled denominator is small, the corresponding sectors are quasi-degenerate and should not be eliminated. A high value of Ω\Omega relative to one local scale does not protect against a deliberately tuned multiphoton resonance.

For a bounded finite-dimensional Hamiltonian, the sufficient condition

∫t0t0+T∥H(t)∥ dt<πℏ\int_{t_0}^{t_0+T} \|H(t)\|\,dt \lt \pi\hbar

guarantees convergence of the one-period Magnus series in a standard operator norm. It is not necessary, and it can become useless when the global norm grows with system size. Convergence of a direct Magnus series, asymptotic usefulness of an optimally truncated local expansion, and absence of resonant heating are distinct claims.

Oscillators, particles in the continuum, and bosonic lattices have unbounded spectra or local occupations. No finite Ω\Omega exceeds every transition energy. Validity must then refer to:

  • a populated energy or occupation window;
  • decay of matrix elements to remote states;
  • a finite observation time;
  • a controlled truncation whose cutoff is varied;
  • the absence or explicit treatment of resonances inside that window.

A calculation that converges only because an untested basis cutoff removed resonant states is not controlled.

For a finite numerical model, construct the exact one-period propagator UFU_F and compare it with

Uapp=e−iK(t0)e−iHeffT/ℏeiK(t0).U_{\mathrm{app}} = e^{-iK(t_0)} e^{-iH_{\mathrm{eff}}T/\hbar} e^{iK(t_0)}.

Useful diagnostics include operator or channel distance, quasienergy differences after branch matching, local-observable errors, and stability when the Fourier, Hilbert-space, timestep, and expansion-order cutoffs are varied. A small one-cycle error can still accumulate, so the comparison should extend to the intended number of periods.

For a local many-body Hamiltonian, the global norm generally grows with volume, so a bound based on ∥H∥/(ℏΩ)\|H\|/(\hbar\Omega) does not survive the thermodynamic limit. The relevant scale is instead a local energy gg, schematically the largest interaction energy incident on one site or degree of freedom.

When

ℏΩ≫g\hbar\Omega\gg g

and suitable locality and boundedness assumptions hold, one can truncate a local high-frequency construction near an optimal order

n∗∼c1ℏΩg.n_* \sim c_1\frac{\hbar\Omega}{g}.

The resulting local Hamiltonian H∗H_* is not exactly conserved, but its drift and the heating rate can be exponentially small. Schematically,

Γheat≲gℏexp⁡[−c2ℏΩg],\Gamma_{\mathrm{heat}} \lesssim \frac{g}{\hbar} \exp\left[ -c_2\frac{\hbar\Omega}{g} \right],

and local dynamics can be governed by H∗H_* up to a prethermal time

t∗∼ℏgexp⁡[c2ℏΩg].t_* \sim \frac{\hbar}{g} \exp\left[ c_2\frac{\hbar\Omega}{g} \right].

The constants and precise hypotheses are model dependent. These expressions state exponential scaling, not a universal numerical lifetime.

Prethermalization adds a second assumption: the dynamics under H∗H_* must itself relax within the relevant sector. If it does, local observables can approach a thermal or generalized prethermal state associated with H∗H_* long before appreciable drive heating occurs. The high-frequency construction alone does not prove ergodicity.

For generic isolated interacting systems with bounded local Hilbert spaces, resonant many-body processes can eventually invalidate the approximate conservation law and drive the system toward an infinite-temperature-like state within each exact symmetry sector. Integrability, strong constraints, localization mechanisms, finite size, or coupling to an environment can alter that endpoint. A prethermal effective Hamiltonian is powerful precisely because it controls a long finite window; it should not be advertised as an eternal conservation law.

High-frequency expansions fail in recognizable ways:

  1. Direct resonance: a coupled denominator Δab(m)\Delta_{ab}^{(m)} is comparable to its matrix element.
  2. Dense many-body resonances: collective excitations bridge multiples of ℏΩ\hbar\Omega even though each local term is weak.
  3. Wrong frame: a large removable drive dominates the Fourier norm and hides a controlled rotating-frame problem.
  4. Strong micromotion: observables are sampled within the period while the kick operator is neglected.
  5. Overtruncation: an asymptotic series is carried beyond its optimal order and the terms begin to grow.
  6. Long-time accumulation: a small local generator error is extrapolated past the demonstrated time window.
  7. Uncontrolled Hilbert cutoff: an unbounded problem appears stable only because high-energy resonances were discarded.
  8. Singular driving: ideal delta kicks or discontinuities produce slowly decaying harmonics and require separate domain and convergence care.

Heating is not synonymous with failure at the first period. A truncated H∗H_* can accurately describe exponentially many periods before the same small remainder causes appreciable energy absorption.

  1. State the period TT, frequency Ω\Omega, Fourier convention, and sampling phase.
  2. Identify exact static splittings, drive amplitudes, local interaction scales, and the populated energy window.
  3. Transform away any large solvable motion or expose a near-resonant block in a rotating frame.
  4. Compute the Fourier components in that frame and inspect their harmonic decay.
  5. Search for small denominators Ea−Eb+mℏΩE_a-E_b+m\hbar\Omega in every symmetry-allowed channel.
  6. Choose one expansion convention and keep its effective Hamiltonian, kick, states, and observables consistent.
  7. Truncate at a declared order and estimate the first omitted term; do not assume higher order is automatically better.
  8. Benchmark the one-cycle propagator and the intended multi-cycle observables whenever a finite calculation is possible.
  9. For many-body claims, state the local energy scale, locality assumptions, system-size dependence, and prethermal time window.
  • Calling Ω\Omega large without naming the comparison scale.
  • Treating the period average as exact when noncommuting harmonics are present.
  • Reversing commutator order after changing the Fourier convention.
  • Summing over positive and negative harmonics twice.
  • Confusing HeffH_{\mathrm{eff}} with the phase-dependent stroboscopic HF(t0)H_F(t_0).
  • Keeping a corrected Hamiltonian while dropping state, observable, or micromotion dressing at the same order.
  • Expanding a large drive that could be removed exactly by a periodic frame.
  • Eliminating a resonant Floquet sector instead of retaining it in the model space.
  • Using the global many-body norm as though it were a size-independent local scale.
  • Interpreting exponential prethermal longevity as proof of no eventual heating.
  • Trusting agreement at one period without checking accumulated error at the intended time.

Show that

Heff(1)=∑m=1∞[Hm,H−m]mℏΩH_{\mathrm{eff}}^{(1)} = \sum_{m=1}^{\infty} \frac{[H_m,H_{-m}]}{m\hbar\Omega}

is Hermitian.

Solution

Because H−m=Hm†H_{-m}=H_m^\dagger,

[Hm,H−m]†=(HmHm†−Hm†Hm)†=HmHm†−Hm†Hm=[Hm,H−m].\begin{aligned} [H_m,H_{-m}]^\dagger &= \left( H_mH_m^\dagger - H_m^\dagger H_m \right)^\dagger \\ &= H_mH_m^\dagger - H_m^\dagger H_m \\ &= [H_m,H_{-m}]. \end{aligned}

Each commutator in the positive-mm sum is Hermitian. The real denominator mℏΩm\hbar\Omega preserves Hermiticity.

For

Hlin(t)=H0+Aσxcos⁡Ωt,H_{\mathrm{lin}}(t) = H_0+A\sigma_x\cos\Omega t,

and

Hcirc(t)=H0+A(σxcos⁡Ωt+σysin⁡Ωt),H_{\mathrm{circ}}(t) = H_0 + A\left( \sigma_x\cos\Omega t + \sigma_y\sin\Omega t \right),

find the order-Ω−1\Omega^{-1} effective correction in each case.

Solution

For the linear drive,

H1=H−1=A2σx,H_1=H_{-1}=\frac{A}{2}\sigma_x,

so

[H1,H−1]=0.[H_1,H_{-1}]=0.

There is no order-Ω−1\Omega^{-1} correction.

For the circular drive,

H1=Aσ−,H−1=Aσ+.H_1=A\sigma_-, \qquad H_{-1}=A\sigma_+.

Therefore

Heff(1)=A2ℏΩ[σ−,σ+]=−A2ℏΩσz.H_{\mathrm{eff}}^{(1)} = \frac{A^2}{\hbar\Omega} [\sigma_-,\sigma_+] = -\frac{A^2}{\hbar\Omega}\sigma_z.

The result distinguishes an unoriented line segment in control space from an oriented circular cycle.

Starting from

U(t,t0)=e−iK(t)e−iHeff(t−t0)/ℏeiK(t0),U(t,t_0) = e^{-iK(t)} e^{-iH_{\mathrm{eff}}(t-t_0)/\hbar} e^{iK(t_0)},

derive the relation between HF(t0)H_F(t_0) and HeffH_{\mathrm{eff}} on compatible logarithm branches.

Solution

Periodicity gives K(t0+T)=K(t0)K(t_0+T)=K(t_0), so

U(t0+T,t0)=e−iK(t0)e−iHeffT/ℏeiK(t0).U(t_0+T,t_0) = e^{-iK(t_0)} e^{-iH_{\mathrm{eff}}T/\hbar} e^{iK(t_0)}.

Conjugation can be moved inside an exponential. Therefore

U(t0+T,t0)=exp⁡[−iTℏHF(t0)],U(t_0+T,t_0) = \exp\left[ -\frac{iT}{\hbar} H_F(t_0) \right],

where, after choosing a compatible quasienergy branch,

HF(t0)=e−iK(t0)HeffeiK(t0).H_F(t_0) = e^{-iK(t_0)} H_{\mathrm{eff}} e^{iK(t_0)}.

Changing t0t_0 changes the eigenvectors by micromotion conjugation but leaves the quasienergy spectrum invariant.

Let H0∣g⟩=0H_0\lvert g\rangle=0 and H0∣e⟩=Δ∣e⟩H_0\lvert e\rangle=\Delta\lvert e\rangle. Suppose H1H_1 couples ∣g⟩\lvert g\rangle and ∣e⟩\lvert e\rangle. Which Floquet-space denominator controls elimination of ∣e,−1⟩ ⁣⟩\lvert e,-1\rangle\!\rangle from the sector containing ∣g,0⟩ ⁣⟩\lvert g,0\rangle\!\rangle?

Solution

The unperturbed quasienergy of ∣g,0⟩ ⁣⟩\lvert g,0\rangle\!\rangle is zero. The quasienergy of ∣e,−1⟩ ⁣⟩\lvert e,-1\rangle\!\rangle is

Δ−ℏΩ.\Delta-\hbar\Omega.

The controlling ratio is therefore

∣⟨e∣H−1∣g⟩∣∣Δ−ℏΩ∣,\frac{ |\langle e|H_{-1}|g\rangle| }{ |\Delta-\hbar\Omega| },

up to the equivalent harmonic labeling implied by the Fourier convention. When Δ≈ℏΩ\Delta\approx\hbar\Omega, this ratio is not small. The two sectors should be retained together or treated in a resonant rotating frame rather than eliminating one of them.

5. Time-origin invariance of van Vleck order one

Section titled “5. Time-origin invariance of van Vleck order one”

Shift the drive by tst_s:

H′(t)=H(t−ts).H'(t)=H(t-t_s).

Show that the order-Ω−1\Omega^{-1} van Vleck Hamiltonian is unchanged.

Solution

The shifted Fourier components are

Hm′=e−imΩtsHm.H'_m=e^{-im\Omega t_s}H_m.

Their commutator is

[Hm′,H−m′]=[e−imΩtsHm,eimΩtsH−m]=[Hm,H−m].\begin{aligned} [H'_m,H'_{-m}] &= [e^{-im\Omega t_s}H_m, e^{im\Omega t_s}H_{-m}] \\ &= [H_m,H_{-m}]. \end{aligned}

Every term in

∑m>0[Hm′,H−m′]mℏΩ\sum_{m>0} \frac{[H'_m,H'_{-m}]}{m\hbar\Omega}

therefore equals the corresponding unshifted term. The drive-origin dependence is carried by the kick operator and the stroboscopic representative, not by this van Vleck effective Hamiltonian.

Use the identity

eiκsin⁡θ=∑m∈ZJm(κ)eimθe^{i\kappa\sin\theta} = \sum_{m\in\mathbb Z} \mathcal J_m(\kappa)e^{im\theta}

to find the leading effective hopping of the shaken chain discussed above. At which values of κ\kappa does the leading hopping vanish?

Solution

After the exact periodic frame transformation, the forward hopping is multiplied by

eiκsin⁡Ωt.e^{i\kappa\sin\Omega t}.

Its zero Fourier component is J0(κ)\mathcal J_0(\kappa). Therefore

Jeff=JJ0(κ).J_{\mathrm{eff}} = J\mathcal J_0(\kappa).

The leading hopping vanishes at the zeros of J0\mathcal J_0. This is a leading high-frequency statement in J/(ℏΩ)J/(\hbar\Omega), not an exact claim that every higher-order process vanishes.

7. Interpret an exponential prethermal time

Section titled “7. Interpret an exponential prethermal time”

Suppose a local driven lattice system has

t∗∼ℏgecℏΩ/g.t_* \sim \frac{\hbar}{g} e^{c\hbar\Omega/g}.

Does this imply that the system never heats? What additional condition is needed to call the intermediate state thermal with respect to H∗H_*?

Solution

No. The estimate says that heating is parametrically slow and that H∗H_* governs local dynamics over a long finite window. At times comparable to or beyond t∗t_*, the exponentially small remainder can produce appreciable energy absorption.

Calling the intermediate state thermal with respect to H∗H_* additionally requires relaxation or ergodicity under H∗H_* within the relevant exact symmetry sector. The high-frequency construction gives approximate conservation and controlled dynamics; it does not by itself prove thermalization.