Summary: Exact oscillator matrix elements connect cumulative state counts to polarized spatial response and energy-transfer distributions, while moving scalar and Dirac modes show why a frozen cavity overlap is only one part of coupling.

A spatial operator with a specified meaning

Let PN,dP_{N,d} project onto the normalized isotropic oscillator modes of total degree at most NN in dd ordinary spatial coordinates. Their common oscillator length is LL and their count is DN=(N+dd)D_N=\binom{N+d}{d}. The operator

A(k)=eik⋅x,η=∣k∣2L22,(1) A(k)=e^{ik\cdot x},\qquad \eta=\frac{|k|^2L^2}{2}, \tag{1}

is a Fourier component of a declared scalar density probe. It is unitary on the complete spatial Hilbert space. Its compressed matrix can lose weight to modes outside a selected band.

These are conditional spatial controls. Positive density is not automatically electric charge or a Dirac scalar. A band trace represents specified equal weights; a coherent field instead requires its actual complex coefficients. The calculation neither changes the particle depth assignments nor adds compactified coordinates.

Hockey-Stick gives an exact form factor

For one normalized oscillator mode,

⟨a∣eikx∣a⟩=e−η/2La(η),(2) \langle a|e^{ikx}|a\rangle =e^{-\eta/2}L_a(\eta), \tag{2}

where LaL_a is a Laguerre polynomial. Align the first coordinate with kk. The other d−1d-1 coordinates contribute their oscillator multiplicities. The generating function for the shell traces is

e−η/2(1−t)−dexp⁡(−ηt1−t).(3) e^{-\eta/2}(1-t)^{-d} \exp\left(-\frac{\eta t}{1-t}\right). \tag{3}

Multiplication by (1−t)−1(1-t)^{-1} performs the cumulative Hockey-Stick sum. Comparison with the generalized Laguerre generating function gives

FN,d(k)=Tr⁡(PN,dA(k))DN=e−η/2LN(d)(η)DN.(4) \begin{aligned} F_{N,d}(k)&=\frac{\operatorname{Tr}(P_{N,d}A(k))}{D_N}\\ &=e^{-\eta/2}\frac{L_N^{(d)}(\eta)}{D_N}. \end{aligned} \tag{4}

In particular FN,d(0)=1F_{N,d}(0)=1. Its small-kk expansion gives

⟨∣x∣2⟩N=dL2(Nd+1+12).(5) \langle |x|^2\rangle_N =dL^2\left(\frac{N}{d+1}+\frac12\right). \tag{5}

This explicitly separates a common well length from the spatial extent of different modes. Equation (4) is a normalized trace amplitude. Squaring it is not generally the probability of remaining in a band: amplitudes may cancel in a trace, while transitions to different final modes are distinct.

Complete transition weights

For ℓ=min⁡(a,b)\ell=\min(a,b) and h=max⁡(a,b)h=\max(a,b), the one-coordinate displacement matrix Aba=⟨b∣A(k)∣a⟩A_{ba}=\langle b|A(k)|a\rangle, with kk chosen positive along that coordinate, is

Aba=e−η/2ℓ!h!×(iη)h−ℓLℓ(h−ℓ)(η).(6) \begin{aligned} A_{ba}&=e^{-\eta/2}\sqrt{\frac{\ell!}{h!}}\\ &\quad\times(i\sqrt\eta)^{h-\ell}L_\ell^{(h-\ell)}(\eta). \end{aligned} \tag{6}

Let rr be the total degree in the spectator coordinates. Their shell multiplicity is gd−1(r)=(r+d−2d−2)g_{d-1}(r)=\binom{r+d-2}{d-2} for d≥2d\ge2. For d=1d=1, only r=0r=0 contributes, with weight one. The probability weight captured in a final cumulative band MM is

IN→M(η)=1DN∑r=0min⁡(N,M)gd−1(r)×∑a=0N−r∑b=0M−r∣Aba∣2.(7) \begin{aligned} I_{N\to M}(\eta) ={}&\frac1{D_N}\sum_{r=0}^{\min(N,M)}g_{d-1}(r)\\ &\times\sum_{a=0}^{N-r}\sum_{b=0}^{M-r} |A_{ba}|^2. \end{aligned} \tag{7}

This retains every allowed final mode. It obeys

DNIN→M=DMIM→N,lim⁡M→∞IN→M=1.(8) \begin{aligned} D_NI_{N\to M}&=D_MI_{M\to N},\\ \lim_{M\to\infty}I_{N\to M}&=1. \end{aligned} \tag{8}

The first identity follows from the symmetric squared entries in (6); the second follows from completeness and unitarity. It is a reciprocity identity for this operator, not a complete two-particle scattering law. Occupation blocking, an energy budget or a specified time-dependent probe would impose additional physical conditions.

Resolve the response by energy as well as by band

Take oscillator energies ℏω(k+d/2)\hbar\omega(k+d/2). A transition from degree aa to bb in the active coordinate changes the energy by ℏωj\hbar\omega j, where j=b−aj=b-a can be positive, zero or negative. Resolve the sum (7) by this signed difference and let wN(j)w_N(j) denote the resulting complete weight, with the final cutoff removed.

Put u(t)=4ηsinh⁡2(t/2)u(t)=4\eta\sinh^2(t/2). The exact one-coordinate generating function is

Ga(t)=∑b∣Aba∣2et(b−a)=eη(et−1)La(−u(t)).(9) \begin{aligned} G_a(t)&=\sum_b|A_{ba}|^2e^{t(b-a)}\\ &=e^{\eta(e^t-1)}L_a(-u(t)). \end{aligned} \tag{9}

The same spectator and cumulative sums give the full moment-generating function

GN(t)=∑jwN(j)etj=eη(et−1)LN(d)(−u(t))DN.(10) \begin{aligned} \mathcal G_N(t)&=\sum_jw_N(j)e^{tj}\\ &=e^{\eta(e^t-1)} \frac{L_N^{(d)}(-u(t))}{D_N}. \end{aligned} \tag{10}

At t=0t=0, this is one. Its first two cumulants are

⟨j⟩=η,Var⁡(j)=η(1+2Nd+1).(11) \begin{aligned} \langle j\rangle&=\eta,\\ \operatorname{Var}(j)&=\eta\left(1+\frac{2N}{d+1}\right). \end{aligned} \tag{11}

There is an independent spatial check. Conjugating the oscillator Hamiltonian by A(k)A(k) adds ℏk⋅p/mkin\hbar k\cdot p/m_{\rm kin} and ℏ2∣k∣2/(2mkin)\hbar^2|k|^2/(2m_{\rm kin}). The band has zero mean momentum, and its directional momentum variance gives the second line of (11). Thus the generating function and the actual kinetic operator give the same two sum rules.

The inclusive weight remains one, but it need not lie in the frequencies available to a particular encounter. For example, every t<0t<0 gives the rigorous bound

Pr⁡(j≤J)≤e−tJGN(t).(12) \Pr(j\le J)\le e^{-tJ}\mathcal G_N(t). \tag{12}

This follows by applying the elementary exponential Markov inequality to etje^{tj}. The program evaluates the logarithm before optimizing tt, so an exponentially small bound is not confused with floating-point zero. Neither (11) nor (12) determines an IDWT encounter's available energy; that requires its actual field dynamics and conservation equations.

Complex polarization and a nested spatial probe

An isotropic trace removes orientation information. A normalized complex polarization v∈Cdv\in\mathbb C^d instead defines the degree-NN mode

∣N,v⟩=(v⋅a†)NN!∣0⟩.(13) |N,v\rangle=\frac{(v\cdot a^\dagger)^N}{\sqrt{N!}}|0\rangle. \tag{13}

Its actual spatial density form factor is

FN,v(k)=e−η/2LN ⁣(L2∣v†k∣22).(14) F_{N,v}(k)=e^{-\eta/2} L_N\!\left(\frac{L^2|v^\dagger k|^2}{2}\right). \tag{14}

Relative complex phases enter ∣v†k∣2|v^\dagger k|^2. Circular and linear polarizations give different directional responses. The diagnostic compares (14) with complete complex mode vectors and separately integrates a general complex superposition in physical coordinates.

Let EE be the real isometric inclusion of a lower spatial sector into a containing sector. For a declared product of two density profiles, a shared wavevector kk samples the higher profile at EkEk. Its Fourier pairing contains both factors

FNa,va(k) FNb,vb(−Ek).(15) F_{N_a,v_a}(k)\,F_{N_b,v_b}(-Ek). \tag{15}

A common physical rotation of vbv_b and EE leaves the result unchanged. Both polarizations are retained. A rotation of only one object is a different preparation. The normal marginal must be formed from the bilinear current before constructing this pairing. Equation (15) remains a specified profile overlap until both fields and their reciprocal motion are derived from an interaction action.

A moving final cavity has a different spectral projector

The moving-cavity calculation gives an exact identity for quadratic kinetics:

Hv=H0−v⋅p,Uv=eimkinv⋅x/ℏ,Pv=UvP0Uv†.(16) \begin{aligned} H_v&=H_0-v\cdot p,\\ U_v&=e^{im_{\rm kin}v\cdot x/\hbar},\\ P_v&=U_vP_0U_v^\dagger. \end{aligned} \tag{16}

For k=mkin(vf−vi)/ℏk=m_{\rm kin}(v_f-v_i)/\hbar, the spatial phase A(k)A(k) maps the initial moving band isometrically onto the corresponding final moving band. In consistently related bases,

⟨Uvfub∣A(k)∣Uviua⟩=δab.(17) \langle U_{v_f}u_b|A(k)|U_{v_i}u_a\rangle =\delta_{ab}. \tag{17}

Projection back into an unchanged cavity is a different operation. In the fifteen-state quasiperiodically perturbed oscillator used for the inertia control, a boost of 1.41.4 in its nonrelativistic units leaves fixed-band weights 0.652533350.65253335 and 0.653947850.65394785 for the two well phases. The corresponding moving-band weights are one to within 3×10−143\times10^{-14}.

The prescribed well and its velocity are part of this calculation. The identity does not derive a physical collision that accelerates the well, or remove the need to include its source and energy. It shows why a frozen profile overlap alone cannot decide whether a moving particle pattern can persist after receiving momentum.

Full first-order Dirac current overlaps

For the exact Dirac control

H=σxp+bσyx+m0σz,(18) H=\sigma_xp+b\sigma_yx+m_0\sigma_z, \tag{18}

use the complete normalized moving spinors derived in the inertia note. With ℏ=c=1\hbar=c=1, the current matrix element is

JΓ(k,v)=∫dx ϕn,v†(x)×Γϕn,0(x)eikx.(19) \begin{aligned} J_\Gamma(k,v)={}&\int dx\,\phi_{n,v}^\dagger(x)\\ &\qquad\times\Gamma\phi_{n,0}(x)e^{ikx}. \end{aligned} \tag{19}

The vertices I,σx,σy,σzI,\sigma_x,\sigma_y,\sigma_z give the density, spatial, pseudoscalar and scalar channels of this two-component comparison. Both spinor components, the boost phase and the changed width remain inside the integral.

At b=0.8b=0.8, m0=0m_0=0, n=1n=1, v=0.8v=0.8, choose the phase-matched wavevector k=E′γv=1.30639453k=E'\gamma v=1.30639453. This matches the spinor phase; it is not automatically the total conserved momentum transfer of a collision. The calculated density amplitudes give

Density comparison Squared amplitude
Both spatial profiles held at zero velocity 0.07494905
Final profile is the complete moving mode 0.75019526

For the moving mode, the spatial-current amplitude is 0.433069070.43306907, the scalar amplitude is 0.013973610.01397361, and the pseudoscalar amplitude is 0.00698680i0.00698680i. They are distinct channels. Independent coordinate quadrature at orders 80 and 160 verifies the complete complex integrals. This comparison contains an external well; it is not a closed reciprocal IDWT encounter or a prediction of a physical interaction rate.

The large inverse-scale ratio is a conditional suppression test

The existing mass-scale benchmarks suggest L5/L6≃3.6×107L_5/L_6\simeq3.6\times10^7 if the geometric conversion factors in the common-size relation are equal. For the illustrative probe ∣k∣L6=10−3|k|L_6=10^{-3}, (4) gives Fe=0.9999988929F_e=0.9999988929 and Fμ=0.9999973214F_\mu=0.9999973214 at the unchanged degree assignments. The same probe has η=6.48×108\eta=6.48\times10^8 in the depth-five oscillator comparison.

At depth-five degrees 9,14,219,14,21, the logarithms of the absolute fixed-band trace amplitudes are approximately −3.24×108-3.24\times10^8. The finite-band capture weights are also exponentially small. Equation (12) gives a similarly small bound if the allowed increase in oscillator energy is only ten quanta. All these statements retain the prescribed stationary well and specified energy window.

This establishes strong suppression for those operator channels. It does not yet explain rare neutrino interactions: the oscillator frequency in the energy window, the physical current, allowed final states, moving confinement and both objects' response must be supplied by the same-field action. In particular, neither a trace amplitude nor a positive density marginal establishes electric neutrality. The broader spatial contact calculation also keeps the physical measure and its units explicit.

Reproduction

cavity_form_factors.py implements the exact matrix elements and generating functions. cavity_form_factor_checks.py checks direct finite matrices, independent complex coordinate integration, reciprocal band weights, energy moment sum rules, the complete transfer generating function, rotated polarized profiles, moving bands and Dirac currents. The numerical controls retain the fixed particle indices; their success establishes the stated mathematics under the stated operators.