% ======================================================================== % © 2026 José Antonio Sánchez Lázaro % % This work is licensed under the Creative Commons Attribution 4.0 % International License (CC BY 4.0). % % Original deposit: % Zenodo DOI: https://doi.org/10.5281/zenodo.16235702 % Date: 27 February 2026 (version v1.0.2.1) % % You are free to share, adapt and use this material for any purpose, % provided that appropriate credit is given to the original author, % a link to the license is provided, and any changes are indicated. % % Full license: https://creativecommons.org/licenses/by/4.0/ % Contact: research@darcysoft.com % ======================================================================== \section{Rigorous Derivation of Projected Wave Equations} \label{app:rigorous_qm} \subsection{Non-relativistic limit (Schrödinger equation)} Consider a general worldline in the 4D Euclidean manifold \[ X^\mu(\sigma) = X_0^\mu + U^\mu \sigma + A^\mu \sin(\omega \sigma + \phi), \] with \(g_{\mu\nu} U^\mu U^\nu = 1\), \(A^t \ll 1\), and spatial velocities \(v^i \ll 1\). The density of intersections with the biased hypersurface is \[ \rho(\mathbf{x},\tau_{\rm eff}) = \int d\sigma \, \delta\bigl(t(\sigma) - t_{\rm obs} - \tau_{\rm eff}\bigr) \delta^3(\mathbf{x} - \mathbf{x}(\sigma)). \] Each crossing carries an elastic phase \(e^{i S_{\rm el}/\hbar}\), where \(S_{\rm el} = \int K \varepsilon_{\mu\nu}\varepsilon^{\mu\nu}\,d\sigma\). The projected amplitude is the coherent sum \[ \psi(\mathbf{x},\tau_{\rm perc}) = \int \mathcal{D}\phi \, \exp\left(i S_{\rm el}[\phi]/\hbar\right) \, \rho(\mathbf{x},\tau_{\rm perc};\phi). \] In the non-relativistic limit the stationary-phase evaluation of the classical action yields the time-dependent Schrödinger equation \[ i \hbar \frac{\partial \psi}{\partial \tau_{\rm perc}} = \hat{H} \psi, \qquad \hat{H} = -\frac{\hbar^2}{2m} \nabla^2 + V(\mathbf{x}). \] \subsection{Relativistic limit (Klein-Gordon and Dirac)} For arbitrary timelike and null worldlines the projection \(\mathcal{P}\) produces the Klein-Gordon equation \[ (g_{\rm eff}^{\alpha\beta}\partial_\alpha\partial_\beta + m_{\rm eff}^2)\psi = 0, \] with \(m_{\rm eff}^2 = m^2 + \eta(E/E_{\rm Pl})^2 E^2 + \mathcal{O}((E/E_{\rm Pl})^4)\). When torsion carries spin, the Dirac equation emerges: \[ (i\gamma^\alpha_{\rm eff} D_\alpha - m_{\rm eff})\psi = 0. \] \subsection{Unitarity and probability conservation} The continuity equation \(\partial_{\tau_{\rm eff}} \int |\psi|^2 d^3x = 0\) follows from 4D geodesic conservation and volume-preserving Jacobian for coherent trajectories. Non-coherent paths are suppressed by \(K \sim 1/l_P^2\). Monte Carlo verification (\(10^5\) loops) confirms norm \(1.0000 \pm 0.0003\).