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Shadow Theory

Bulk-to-Brane Projection, Dynamical Nonclosure, and Observable Residues in Randall–Sundrum Gravity

Comparative examples and limits of interpretation

Jeremy RodgersSection 14 of 18Original PDF ↗Publication DOI ↗

Comparative examples and limits of interpretation

An exactly soluble projection: two coupled oscillators

The following systems are scientific comparisons that clarify the meaning and limits of the RS2 result. An ordinary Hamiltonian model verifies, without gravitational complications, every step from fiber nonprojectability through memory to an exact Tier-1 surrogate, and simultaneously exhibits the logical boundary that Section 11 proves in general. The projected equation obtained below is the elementary exactly soluble instance of the Mori–Zwanzig projection-operator structure [13]: a memory kernel, an initial-slip term, and a retained susceptibility. Let Hf=px22m+12mω02x2+py22M+12MΩ2(y−cxMΩ2)2−f(t) x,(106) H_f=\frac{p_x^2}{2m}+\tfrac12 m\omega_0^2x^2 +\frac{p_y^2}{2M} +\tfrac12 M\Omega^2\Bigl(y-\frac{cx}{M\Omega^2}\Bigr)^2 -f(t)\,x ,\tag{106} and retain X=(x,v)TX=(x,v)^T while eliminating Z=(y,w)TZ=(y,w)^T. With δ≡c2/(mMΩ2)\delta\equiv c^2/(mM\Omega^2), the first-order generator has blocks A=(01−(ω02+δ)0),B=(00c/m0),C=(00c/M0),D=(01−Ω20),(107) A=\begin{pmatrix}0&1\\-(\omega_0^2+\delta)&0\end{pmatrix}, \quad B=\begin{pmatrix}0&0\\c/m&0\end{pmatrix}, \quad C=\begin{pmatrix}0&0\\c/M&0\end{pmatrix}, \quad D=\begin{pmatrix}0&1\\-\Omega^2&0\end{pmatrix},\tag{107} with etD=(cos⁡Ωtsin⁡Ωt/Ω−Ωsin⁡Ωtcos⁡Ωt)e^{tD}=\begin{pmatrix}\cos\Omega t&\sin\Omega t/\Omega\\ -\Omega\sin\Omega t&\cos\Omega t\end{pmatrix}. Variation of constants evaluates every projected term: X˙(t)=AX(t)+BetDZ0+∫0tK(t−s)X(s) ds+(0f(t)/m),(108) \dot X(t)=AX(t)+Be^{tD}Z_0 +\int_0^t\mathcal K(t-s)X(s)\,ds +\binom{0}{f(t)/m},\tag{108}   K(t)=BetDC=(00c2mMΩsin⁡Ωt0).  (109) \boxed{\; \mathcal K(t)=Be^{tD}C =\begin{pmatrix} 0&0\\[2pt] \dfrac{c^2}{mM\Omega}\sin\Omega t&0 \end{pmatrix}. \;}\tag{109} Equivalently, after one integration by parts,   x¨+ω02x+∫0tδcos⁡[Ω(t−s)]x˙(s) ds=f(t)m+ζ(t),  (110) \boxed{\; \ddot x+\omega_0^2x +\int_0^t\delta\cos\bigl[\Omega(t-s)\bigr]\dot x(s)\,ds =\frac{f(t)}{m}+\zeta(t), \;}\tag{110} ζ(t)=cm[(y0−cx0MΩ2)cos⁡Ωt+w0Ωsin⁡Ωt].(111) \zeta(t)=\frac{c}{m} \Bigl[\Bigl(y_0-\frac{cx_0}{M\Omega^2}\Bigr)\cos\Omega t +\frac{w_0}{\Omega}\sin\Omega t\Bigr].\tag{111} Two states with equal (x0,v0)(x_0,v_0) and different (y0,w0)(y_0,w_0) have different later trajectories , the instantaneous readout is nonprojectable, exactly as in Proposition 3.1, with ζ\zeta playing the role of ηz0\eta_{z_0} in (88). The smallest generic Markov completion carries the two hidden coordinates, exactly as EdynRSE^{\mathrm{RS}}_{\mathrm{dyn}} does. The exact retarded susceptibility is   χxxR(ω)=Ω2−z2m[(ω02−z2)(Ω2−z2)−δz2],z=ω+i0+.  (112) \boxed{\; \chi^R_{xx}(\omega) =\frac{\Omega^2-z^2} {m\bigl[(\omega_0^2-z^2)(\Omega^2-z^2)-\delta z^2\bigr]}, \qquad z=\omega+i0^+ . \;}\tag{112}

And yet eliminating yy also gives a local, Tier-1-only, higher-derivative equation,   [(∂t2+ω02)(∂t2+Ω2)+δ ∂t2]x=1m(∂t2+Ω2)f.  (113) \boxed{\; \bigl[(\partial_t^2+\omega_0^2)(\partial_t^2+\Omega^2) +\delta\,\partial_t^2\bigr]x =\frac1m(\partial_t^2+\Omega^2)f . \;}\tag{113} Its extra initial derivatives encode precisely the two missing constants. This exactly soluble example exposes the logical boundary: nonprojectability of (x,x˙)(x,\dot x) proves the need for completion relative to that state choice, and proves nothing about the nonexistence of a higher-derivative or history-level theory written in xx alone. This is the finite-dimensional shadow of Lemma 11.1.

Einstein–Cartan and Aharonov–Bohm comparisons

These two examples distinguish a genuine propagating source degree of freedom from an auxiliary variable and from an incomplete choice of observable state: Einstein–Cartan–Dirac torsion is auxiliary and introduces no same-readout fiber, whereas the Aharonov–Bohm phase is already determined once the observable state is chosen completely.

Einstein–Cartan–Dirac.

Minimal Einstein–Cartan–Dirac theory fails as the required propagating source-projection antecedent , not as a theory , because its torsion is auxiliary: it introduces no independent propagating degree of freedom, and hence no same-readout fiber of the kind Proposition 3.1 exhibits. The connection equation determines the contorsion algebraically from the axial current, and substitution gives the four-fermion term [15] Seff=SEH+SDirac[ω˚]+3κ16∫d4x  e J5aJ5a,(114) S_{\mathrm{eff}} =S_{\mathrm{EH}}+S_{\mathrm{Dirac}}[\mathring\omega] +\frac{3\kappa}{16}\int d^4x\;e\,J_{5a}J_5^a,\tag{114} up to signature and current conventions. A torsion-free theory containing this operator has identical retained observables. There is no independent propagating fiber analogous to a remote RS2 wave packet , which is exactly what RS2 supplies and Einstein–Cartan does not.

Aharonov–Bohm.

The Aharonov–Bohm effect [19] remains a clean control for readout incompleteness: equal local curvature can coexist with different gauge-invariant holonomy and different interference phases. But holonomy is already a standard observable of four-dimensional gauge theory. The effect shows that a curvature-only state is incomplete; it does not show that a deeper source ontology has been observed. It is the correct model for “the readout you chose was too small,” not for “there is a hidden dimension.”

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