09 Jun 2026

VI: Exceptional-Basis Spectral Propagation and Synchronization

exceptional Hermite angular-momentum quench spectral propagation quantum synchronization cutoff convergence non-Gaussian dynamics

The short-time commutator expansion tells us how an observable first responds to the quench. It does not, by itself, produce a finite-time trajectory. Here we use the complete exceptional-Hermite product basis to propagate the same non-Gaussian state beyond short times, without imposing a Gaussian closure.

The result is a numerical approximation to the infinite-dimensional Schrödinger evolution, not a new finite-dimensional exact model. Its reliability therefore rests on observable-level cutoff tests.

The fixed-confinement quench

We use

\[\hbar=2M=1,\]

and retain the sign of the half-cyclotron frequency

\[\omega_c=\frac{qB}{2Mc}.\]

After the coordinate potential has been diagonalized, the post-quench Hamiltonian is

\[H_{\mathrm{RE},B} =H_{\mathrm{sep}}^{\mathrm{RE}}-\omega_c L_z, \qquad L_z=q_+p_- -q_-p_+.\]

The preparation Hamiltonian $H_{\mathrm{sep}}^{\mathrm{RE}}$ already contains the coordinate scales $\Omega_\pm$, including the target diamagnetic dressing. At $t=0$, only the angular generator $-\omega_cL_z$ is activated. This is a fixed-confinement angular-momentum quench. It is not a literal switch of the complete magnetic field, which would also alter the diamagnetic coordinate term.

The signed $\omega_c$ matters. Reversing it reverses every first-order angular-response coefficient, although even-in-time quantities such as the leading survival loss depend on $\omega_c^2$.

Expansion in the exceptional basis

Fix the even exceptional-Hermite codimensions

\[\boldsymbol m=(m_+,m_-).\]

The separable one-mode eigenstates form a complete product basis, so the evolving state can be written as

\[|\Psi(t)\rangle =\sum_{r,s=0}^{\infty}c_{rs}(t) |m_+,r\rangle\otimes|m_-,s\rangle.\]

Projecting the Schrödinger equation gives

\[i\dot c_{rs} =E^{\mathrm{sep}}_{\boldsymbol m,(r,s)}c_{rs} -\omega_c\sum_{u,v=0}^{\infty} \mathsf L_{rs,uv}c_{uv},\]

where the angular-momentum matrix elements factor into one-dimensional integrals:

\[\begin{aligned} \mathsf L_{rs,uv} ={}&\langle r|q_+|u\rangle \langle s|p_-|v\rangle\\ &-\langle r|p_+|u\rangle \langle s|q_-|v\rangle. \end{aligned}\]

The mode labels $m_+$ and $m_-$ are suppressed inside these one-mode matrix elements. For momentum elements, the derivative acts on the exceptional polynomial ratio as well as on its Gaussian envelope. Reweighting a Gaussian probability density is therefore insufficient for the momentum sector.

Both $q_\alpha$ and $p_\alpha$ reverse one-mode parity. Each term in $L_z$ consequently flips both mode parities and preserves their product. The propagation separates into fixed total-parity sectors, a useful structural check on the matrix assembly.

What the finite cutoff means

For computation we retain

\[0\le r,s\le N\]

and Hermitize the projected Hamiltonian before diagonalizing it. If

\[H_N=V_ND_NV_N^\dagger,\]

then the coefficient vector within the retained space is propagated as

\[\boldsymbol c_N(t) =V_Ne^{-iD_Nt}V_N^\dagger\boldsymbol c_N(0).\]

This spectral exponential is unitary within the truncated space, so its norm is conserved to floating-point accuracy. That fact does not establish convergence to the infinite-basis dynamics: a truncated Hermitian matrix can conserve its norm while omitting physically important high-level amplitudes.

We therefore monitor two more demanding diagnostics:

  1. the maximum change in each observable curve when $N$ is increased; and
  2. the population on the cutoff boundary,
\[P_{\partial}(t) =\sum_s|c_{Ns}(t)|^2 +\sum_r|c_{rN}(t)|^2 -|c_{NN}(t)|^2.\]

There is no claim that any finite $N$ closes the rational dynamics exactly. The cutoff must be reconsidered for stronger quenches, more highly excited inputs, or longer time windows.

Synchronization as a relative-fluctuation contrast

For the mass convention above, define dimensionless quadratures

\[Q_j=\sqrt{\frac{\omega_0}{2}}\,x_j, \qquad P_j=\sqrt{\frac{2}{\omega_0}}\,p_j.\]

The complete-synchronization contrast is

\[S_c(t)=\langle\mathcal D_c(t)\rangle^{-1},\]

with

\[\mathcal D_c =\frac12\left[ (\delta Q_x-\delta Q_y)^2 +(\delta P_x-\delta P_y)^2 \right].\]

This is an equal-time relative-fluctuation measure. A large value, an extremum, or an oscillatory interval does not by itself prove phase locking or stationary synchronization.

In the benchmark below, $g=0$, so the rotated $+,-$ axes coincide with the laboratory axes up to a permutation. For $g\ne0$, one must keep track of which quadratures define the synchronization observable.

Exact local slope for the codimension-two input

For the $m=2$, $\ell=0$ exceptional-Hermite factor, let

\[\mathcal M =\sqrt{\frac{\pi}{2}}e^{1/2} \operatorname{erfc}\!\left(\frac{1}{\sqrt2}\right).\]

Its physical variances are

\[V_{q,\alpha} =\frac{2(\mathcal M-1/2)}{\Omega_\alpha}, \qquad V_{p,\alpha} =\frac{\Omega_\alpha}{2} \left(\frac32+\frac{\mathcal M}{3}\right).\]

At $\omega_0=1$, define the dimensionless variance sum

\[A_\alpha^{(2)} =\frac{\mathcal M-1/2}{\Omega_\alpha} +\Omega_\alpha\left(\frac32+\frac{\mathcal M}{3}\right).\]

This is $V_{Q,\alpha}+V_{P,\alpha}$, not $V_{q,\alpha}+V_{p,\alpha}$.

For the real product eigenstate, both local variance rates vanish at the instant of the quench:

\[\left.\frac{dV_{Q,\alpha}}{dt}\right|_{0}=0, \qquad \left.\frac{dV_{P,\alpha}}{dt}\right|_{0}=0.\]

The cross-covariance rates remain

\[\left.\frac{d}{dt}\langle q_+q_-\rangle\right|_0 =\omega_c(V_{q,-}-V_{q,+}),\] \[\left.\frac{d}{dt}\langle p_+p_-\rangle\right|_0 =\omega_c(V_{p,-}-V_{p,+}),\]

while both mixed position-momentum cross rates vanish. Combining these facts gives the exact first-order expansion

\[\boxed{ S_c^{(2,2)}(t) =\frac{2}{A_+^{(2)}+A_-^{(2)}} -\frac{4\omega_c\bigl(A_+^{(2)}-A_-^{(2)}\bigr)} {\bigl(A_+^{(2)}+A_-^{(2)}\bigr)^2}\,t +O(t^2) }.\]

This statement is local to $t=0$. It is exact for the stated real, definite-parity product preparation, but the displayed Taylor truncation is only a first-order short-time approximation.

If $A_+^{(2)}=A_-^{(2)}$, the linear slope vanishes. That cancellation does not freeze the state: the survival probability can still have nonzero quadratic curvature. It also does not establish stationary synchronization.

A cutoff-tested finite-time benchmark

The representative quench uses

\[g=0, \qquad m_+=m_-=2, \qquad \ell_+=\ell_-=0,\]

and

\[\Omega_+=\frac54, \qquad \Omega_-=\frac{17}{20}, \qquad \omega_c=\frac34, \qquad \omega_0=1.\]

The bare-confinement stability margins are positive:

\[\Omega_+^2-\omega_c^2=1, \qquad \Omega_-^2-\omega_c^2=\frac4{25}.\]

One-mode $q$ and $p$ matrices were evaluated with 360-point Gauss-Hermite quadrature. We propagated $0\le t\le12$ at square cutoffs $N=30,34,38,42$. At $N=42$, the maximum one-mode overlap error was $1.71\times10^{-12}$, and the maximum propagated norm error was $5.77\times10^{-15}$.

The more informative observable-level comparison is:

$N$ $\max \Delta\mathcal S $ $\max \Delta S_c $ $\max \Delta I $ $\max P_\partial$
30 $1.69\times10^{-5}$ $9.60\times10^{-4}$ $3.49\times10^{-4}$ $1.01\times10^{-6}$            
34 $1.25\times10^{-5}$ $7.25\times10^{-4}$ $2.39\times10^{-4}$ $5.15\times10^{-7}$            
38 $9.83\times10^{-6}$ $3.70\times10^{-4}$ $1.58\times10^{-4}$ $1.59\times10^{-7}$            
42 reference reference reference $1.04\times10^{-7}$            

Every $\Delta$ is the largest absolute difference from the $N=42$ curve over the stated time window. Thus $N=42$ is the numerical reference, not a mathematically certified infinite-cutoff answer.

Short-time and finite-time checks

The analytic synchronization values are

\[S_c(0)=0.5106376395009\ldots,\] \[\dot S_c(0)=-0.1229730434570\ldots.\]

At the first numerical step, $t=10^{-3}$, the propagated values give

\[S_c(0)=0.5106376395002\ldots, \qquad \dot S_c(0)\big|_{\mathrm{one\,step}} =-0.1229306242038\ldots.\]

The slope difference is consistent with the remainder of a one-sided finite difference. The analytic coefficient, together with the stability margins and the codimension-two moment formulas, was independently evaluated in Maxima 5.49.0.

At the $N=42$ reference cutoff:

These are bounded-window dynamics. They do not establish equilibration, an asymptotic synchronized state, or uniform long-time convergence.

What this calculation establishes

The exceptional basis turns the formal coefficient equations into a reproducible finite-time method for one stable quench. It also separates four logically different claims:

No Gaussian closure is used. The rational force continues to generate an open moment hierarchy, while the basis calculation evolves the state amplitudes directly.

Series navigation

  1. Magnetic oscillator stability and rotated-coordinate reduction
  2. Exceptional-Hermite preparation
  3. Fixed-confinement angular quench
  4. Exact covariance response
  5. Survival curvature
  6. Spectral propagation and synchronization
  7. Non-Gaussian mutual information
© Rajesh Kumar, SKMU · Physics Lecture Notes · rajeshphy.github.io

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