Spatial model

Consider two normalized densities on mm shared ordinary spatial coordinates of the nested physical manifold. A Gaussian is a specified local flat-space profile, with centre XX and positive-definite covariance matrix Σ\Sigma:

ρΣ,X(x)=exp⁡[−12(x−X)TΣ−1(x−X)](2π)m/2det⁡Σ,∫RmρΣ,X(x) dmx=1. \rho_{\Sigma,X}(x)= \frac{\exp[-\frac12(x-X)^T\Sigma^{-1}(x-X)]} {(2\pi)^{m/2}\sqrt{\det\Sigma}}, \qquad \int_{\mathbb R^m}\rho_{\Sigma,X}(x)\,d^mx=1.

Thus ⟨x⟩=X\langle x\rangle=X and ⟨(x−X)(x−X)T⟩=Σ\langle(x-X)(x-X)^T\rangle=\Sigma. Covariance eigenvalues have units of length squared. The Gaussian describes spatial extent; an actual orbit or a time-averaged exposure requires its own dynamical specification.

For a local density contact energy, define

U(R)=gI(R),I(R)=∫ρΣA,XA(x)ρΣB,XB(x) dmx,R=XA−XB. U(R)=g I(R),\qquad I(R)=\int\rho_{\Sigma_A,X_A}(x)\rho_{\Sigma_B,X_B}(x)\,d^mx, \qquad R=X_A-X_B.

The model supplies gg. If UU has energy units, gg has units of energy times spatial volume. Representation contractions and other nonlocal kernels can be included in a larger model; the calculation here evaluates this particular scalar contact.

Exact convolution

Let C=ΣA+ΣBC=\Sigma_A+\Sigma_B. Then

I(R)=exp⁡[−12RTC−1R](2π)m/2det⁡C. \boxed{ I(R)=\frac{\exp[-\frac12R^TC^{-1}R]} {(2\pi)^{m/2}\sqrt{\det C}}. }

For a direct derivation, use the Fourier convention ρ^(k)=∫e−ik⋅xρ(x) dmx\widehat\rho(k)=\int e^{-ik\cdot x}\rho(x)\,d^mx. Completing the Gaussian square gives ρ^Σ,X(k)=e−ik⋅X−12kTΣk\widehat\rho_{\Sigma,X}(k)=e^{-ik\cdot X-\frac12k^T\Sigma k}. The product integral is therefore

I(R)=1(2π)m∫Rme−ik⋅R−12kTCk dmk. I(R)=\frac{1}{(2\pi)^m} \int_{\mathbb R^m}e^{-ik\cdot R-\frac12k^TCk}\,d^mk.

Diagonalize the real symmetric positive matrix CC by an orthogonal rotation. Each one-dimensional integral contributes 2π/cjexp⁡[−Rj2/(2cj)]\sqrt{2\pi/c_j}\exp[-R_j^2/(2c_j)], where cj>0c_j>0 is an eigenvalue. Multiplication proves the formula. In particular, correlations and unequal widths are retained in CC.

The relative contact profile and the absolute overlap are

Ω(R)=I(R)I(0)=e−12RTC−1R,I(0)=1(2π)m/2det⁡C. \Omega(R)=\frac{I(R)}{I(0)} =e^{-\frac12R^TC^{-1}R}, \qquad I(0)=\frac{1}{(2\pi)^{m/2}\sqrt{\det C}}.

Ω\Omega is dimensionless; II has inverse-volume units. Replacing II by Ω\Omega in an energy absorbs the width-dependent I(0)I(0) into its coupling. That replacement needs an explicit normalization convention.

Forces and widths

With the covariances held fixed during a displacement, set W=C−1W=C^{-1}. The force on centre AA, the opposite force on BB, and the energy Hessian are

FA=−∇RU=gI(R)WR,FB=−FA, F_A=-\nabla_R U=gI(R)WR,\qquad F_B=-F_A,

∇R∇RU=gI(R)[WRRTW−W]. \nabla_R\nabla_R U =gI(R)\left[WRR^TW-W\right].

Positive gg gives repulsion in this contact model; negative gg gives attraction. If a profile deforms with RR, total derivatives additionally differentiate its covariance and normalization.

Profiles Relative overlap Ω(R)\Omega(R)
ΣA=σA21\Sigma_A=\sigma_A^2\mathbf1, ΣB=σB21\Sigma_B=\sigma_B^2\mathbf1 exp⁡[−∣R∣2/(2(σA2+σB2))]\exp[-|R|^2/(2(\sigma_A^2+\sigma_B^2))]
Equal ground-state densities of −Δ+λ∣x∣2-\Delta+\lambda|x|^2 exp⁡[−λ∣R∣2/2]\exp[-\sqrt{\lambda}|R|^2/2]

In the second row the wavefunction is proportional to e−λ∣x−X∣2/2e^{-\sqrt{\lambda}|x-X|^2/2}, so each density has σ2=1/(2λ)\sigma^2=1/(2\sqrt{\lambda}). The overlap's Gaussian standard deviation is L=λ−1/4L=\lambda^{-1/4} along each coordinate. An absolute physical length requires the scale and coefficients of the specified operator. The oscillator domain supplies its normalization and decay conditions.

Contact across nested depths

For a higher-depth density on coordinates z∈Rdz\in\mathbb R^d, choose an orthogonal shared-coordinate projection x=Bzx=Bz, with BBT=1mBB^T=\mathbf1_m. Completing BB to an orthogonal coordinate frame identifies the remaining ordinary spatial coordinates yy. A Gaussian with mean XBX_B and covariance ΣB\Sigma_B has full marginal

ρˉB(x)=∫ρB(x,y) dd−my=ρBΣBBT, BXB(x). \bar\rho_B(x)=\int\rho_B(x,y)\,d^{d-m}y =\rho_{B\Sigma_BB^T,\,BX_B}(x).

Indeed its characteristic function is the higher one evaluated at BTkB^Tk, which proves the covariance rule even when shared and remaining coordinates are correlated. Apply the contact formula with C=ΣA+BΣBBTC=\Sigma_A+B\Sigma_BB^T and R=XA−BXBR=X_A-BX_B.

The cylindrical contact premise uses a lower-depth density independent of yy. Fubini then gives ∫ρA(x)ρB(x,y) dx dy=∫ρA(x)ρˉB(x) dx\int\rho_A(x)\rho_B(x,y)\,dx\,dy=\int\rho_A(x)\bar\rho_B(x)\,dx. This uses a cylindrical field normalized on its supported submanifold. A box-normalized probability extension instead carries its explicit inverse fibre-volume factor.

Every coordinate in this construction belongs to the same nested physical manifold. The projection describes the smaller sector's shared directions; the containing particle's dimensions remain equivalent in physical kind.

spatial_profile_checks.py checks direct density quadrature, anisotropic rotations, force and Hessian derivatives, and correlated Gaussian marginals.