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---
## Why a propagation channel must be selected first

An accompanying field arises from the joint response of a moving core and the surrounding spatial structure. To obtain a matter wave that crosses apertures and accumulates propagation phase, that response needs an extended field mode. An internal vibration localized around a core does not automatically become a wave propagating through the surrounding region, even when it has a definite frequency. Chapter 5 therefore states a spectral condition before reducing a field equation to a slowly varying envelope equation.

A gapped branch retains a nonzero eigenfrequency $\omega_0$ as wavenumber tends to zero. Let $a$ label the selected channel, $\mathbf k$ its wavevector, $a_0$ a microscopic length scale and $B_{ij}$ a real symmetric positive-definite dimensionless propagation matrix. Its long-wavelength spectrum is written

<Equation name="qm-gapped-branch" compact />

$B$ describes directional gradient costs. Equation (5.1.22) in the final manuscript defines this selected second-order continuum branch without an appended remainder. Three levels remain distinct: the full FCC lattice spectrum (5.1.11), its long-wave expansion for $ka_0\ll1$, and the subsequent slow-envelope reduction of this adopted gapped channel. Higher-gradient lattice corrections belong to the first transition and must be restored if that range fails. The gapped branch is a constitutive spectral input whose realization is to be computed from the full core–field action; a localized bound oscillator alone does not supply it. The envelope derivation below does not assume that a particular FCC realization is already a complete microscopic particle model.

Assuming that branch exists, let $\Phi^{(+)}$ denote the selected positive-frequency channel and $S^{(+)}$ its source. Chapter 5 adopts the second-order effective equation

<Equation name="qm-underlying" compact />

Here $c$ is the characteristic propagation speed. $V$ has units of energy and enters through $2\omega_0V/\hbar$ as a weak scalar modulation of frequency squared, with $|V|\ll\hbar\omega_0$. This is an explicit effective constitutive input; general gauge coupling to electromagnetic scalar and vector potentials needs a separate construction. Both $\omega_0$ and field normalization are constant in the region considered. If $B$ varies slowly in space, the operator must retain divergence form $\partial_i(B_{ij}\partial_j)$ rather than moving $B$ outside the derivatives.

The second time derivative retains fast oscillations and propagation fronts. The next steps extract slow evolution within this specified channel; they do not assume the Schrödinger equation as the fundamental spatial dynamics.

## Separating the fast carrier from the slow envelope

The field oscillates rapidly near its eigenfrequency while amplitude and phase may vary slowly. Extracting the rapid part lets the equation describe packet evolution on longer experimental timescales. Following the manuscript, this page uses a rest carrier with spatial carrier wavevector $\mathbf k_0=0$:

<Equation name="qm-carrier" compact />

$\Psi(\mathbf r,t)$ is the complex envelope, $S_0$ the source envelope with the same carrier, and the physical real field is the real part. If $\Psi=Q_1+iQ_2$,

$$
\Phi_{\rm real}=Q_1\cos\omega_0t+Q_2\sin\omega_0t.
$$

$Q_1,Q_2$ are two real quadratures. Complex notation records both without changing the real nature of the field or defining a detection probability. A spatially phased carrier or co-moving coordinates would introduce the corresponding first spatial or convective terms; those are outside the present rest-carrier simplification.

First compute the time derivative in full, before approximating. The product rule gives manuscript equation (5.1.32):

$$
\partial_t^2\!\left(\Psi e^{-i\omega_0t}\right)
=e^{-i\omega_0t}
\left(\partial_t^2\Psi-2i\omega_0\partial_t\Psi-\omega_0^2\Psi\right).
$$

On substitution into the second-order channel equation, the carrier's $-\omega_0^2\Psi$ cancels the original $+\omega_0^2\Psi$ exactly. Removing the common carrier factor leaves

<Equation name="qm-exact-envelope" compact />

The term $\partial_t^2\Psi$ is still present: this is an exact rewriting within the given channel. It remains available when the envelope changes rapidly. Removing that second derivative is the actual approximation made next.

## How slow variation and mass matching enter

Let $\Omega$ be the envelope's angular frequency relative to the carrier, not the total field frequency. For an envelope spectrally concentrated at $|\Omega|\ll\omega_0$, the second slow-time derivative is small relative to the first-derivative carrier cross term. Low wavenumber, a continuum long-wavelength range and weak background modulation are also required:

<Equation name="qm-matching-scales" compact />

These conditions do different work. Slow frequency permits discarding $\partial_t^2\Psi$ at leading order; low wavenumber keeps the frequency close to the bottom of the gapped branch; $ka_0\ll1$ controls microscopic higher-gradient terms; weak $V$ prevents background modulation from disrupting the carrier scale. They should be checked spectrally or in suitable norms, not by dividing by $|\Psi|$ at envelope nodes. Initial and boundary preparation must also avoid substantial excitation of the omitted fast branch; otherwise the second-order equation is needed for initial or boundary layers.

Separately from these small parameters, $\hbar\omega_0=m_0c^2$ matches the core eigenenergy to the channel frequency. It identifies the gradient coefficient $\hbar c^2/(2\omega_0)$ as $\hbar^2/(2m_0)$. Differentiation does not supply this relation: it is the physical input connecting rest frequency and material mass.

Discard the second slow-time derivative in the exact remainder equation, multiply by $-\hbar/(2\omega_0)$ and rearrange to obtain

<Equation name="qm-schrodinger" compact />

The minus sign in $S_{\rm Sch}$ comes from this algebraic transformation. Isotropy $B=I$ and no explicit source give the familiar scalar Schrödinger form; general $B$ retains direction dependence in the gradient operator. The equation describes a low-frequency envelope of a gapped spatial field. It does not establish, in reverse, the upstream spectrum, stable core or mass matching.

The rest period $\tau=2\pi/\omega_0$ also distinguishes $h$ from $\hbar$. With matched energy $E_0=m_0c^2$, one has $E_0\tau=h$ and $E_0/\omega_0=\hbar$. A nonlinear periodic configuration must supply its own orbit action before testing this single-excitation matching. The [matter-wave page](/en/theory/quantum/matter-wave) explains how that matching connects total mechanical momentum and phase.

## Comparing the retained terms with truncation error

An approximation should identify what it leaves out. For a uniform, source-free, isotropic channel with $V=0$, the complete positive-frequency dispersion is $\omega=\sqrt{\omega_0^2+c^2k^2}$. The envelope frequency is $\Omega=\omega-\omega_0$, after subtracting the carrier. Setting $z=ck/\omega_0$ gives the Taylor check already present in the equation registry:

<Equation name="qm-dispersion-error" compact />

The slow-envelope equation retains $z^2/2$; the next correction in the complete dispersion is $-z^4/8$. Increasing wavenumber therefore exposes the error from omitting the second slow-time derivative. The interactive comparison below shows frequencies in these two specified models, not a new high-energy prediction of complete ASD dynamics.

<EnvelopeLimitExplorer />

This check applies to the stated uniform channel. General potentials, rapid preparation, boundary layers, mode coupling and microscopic higher-gradient spectra need separate error control; a uniform-dispersion plot cannot replace it. The effective Schrödinger kernel has nonzero tails at long distance. Following a sudden boundary change, the earliest signal must still be calculated with the original second-order field equation.

## What the squared envelope represents first

Field energy gives a direct reason to retain envelope amplitude. Let $Z_\Phi$ be the kinetic normalization of the selected real channel. In the quadratic energy approximation without external potential, the manuscript takes

$$
\mathcal E_\Phi=\frac{Z_\Phi}{2}
\left[(\partial_t\Phi)^2+c^2B_{ij}\partial_i\Phi\,\partial_j\Phi+\omega_0^2\Phi^2\right].
$$

Substitute the carrier representation of the real field and average over a fast period, treating the envelope as slowly varying across it:

<Equation name="qm-energy-weight" compact />

Carrier kinetic energy and the eigenfrequency potential term together give the leading contribution $Z_\Phi\omega_0^2|\Psi|^2/2$. The squared modulus therefore first has the meaning of field-energy or action weight, rather than being assigned particle-detection probability during substitution.

If corrections of kinetic-energy order are retained, expansion of the time term produces $-2\omega_0\operatorname{Im}(\Psi^*\partial_t\Psi)$. It must be retained alongside the spatial gradient term; adding only gradient energy would omit a term of the same order. Energy accounting across the two timescales requires consistent ordering.

The gapped spectrum, carrier separation, slow-variation conditions and energy matching now form a checkable effective-equation derivation. [Interference and diffraction](/en/theory/quantum/interference-diffraction) calculate how a packet makes a field pattern, while [detection and statistics](/en/theory/quantum/detection-statistics) address how that field transfers energy to a detector and produces discrete events. They use the same envelope but require different derivations.

## Sources and applicability checks

This page restores the continuous steps of Chapter 5, equations (5.1.22) and (5.1.30)–(5.1.36). The uniform-dispersion Taylor check retains the existing ASD-WEB-QM-016. [OP-QM-003](/en/open-problems/quantum/effective-limit) specifies the remaining spectral, error-control and initial/boundary-value tasks.

<CanonicalSource />
