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\documentclass[12pt,a4paper]{article}
\usepackage{amsmath,amssymb,amsthm}
\usepackage{geometry}
\usepackage{hyperref}
\usepackage{cascade-xref} % cross-paper \xref machinery (incl. xr-hyper)
\usepackage{microtype}
\usepackage{booktabs}
\usepackage{array}
\usepackage{enumitem}
\geometry{margin=2.5cm}
% xr-hyper cross-paper references (must follow hyperref).
% Note: in this paper's bibliography \bibitem{part0} points at Part 0
% (cascade-series-part0), not Part I -- legacy bibliography naming.
\xrhyperdoc{part0}{cascade-series-part0}
\xrhyperdoc{part4a}{cascade-series-part4a}
\xrhyperdoc{part4b}{cascade-series-part4b}
\xrhyperdoc{part6}{cascade-series-part6}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{corollary}[theorem]{Corollary}
\newtheorem{definition}[theorem]{Definition}
\newtheorem{remark}[theorem]{Remark}
\newtheorem{observation}[theorem]{Observation}
\title{The Cascade Series --- Part II\\[0.5em]
\large Quantum Mechanics from the Cascade:\\
Effective Theory of a 4-Dimensional Observer\\
in the Sphere-Area Geometry}
\author{RTAC}
\date{March 2026}
\begin{document}
\setlength{\emergencystretch}{3em}
\maketitle
\phantomsection
\label{paperdoc}
\begin{abstract}
The cascade series tests one hypothesis: the infinite-dimensional unit ball, descended to
four dimensions, is indistinguishable from our universe. The companion paper~\cite{part0}
derived a geometric invariant $I = 1.0990\times 10^{-120}$ from the sphere-area cascade
using only orthogonality as input. Here we show that a 4-dimensional observer embedded in
the cascade geometry recovers the full structural framework of quantum mechanics---including
the Born rule, complex amplitudes, non-commutativity, the Schr\"{o}dinger equation,
entanglement, and Bell inequality violation---without quantum postulates.
The argument proceeds in six steps, each a theorem about spheres and Beta functions.
(1)~The cascade's boundary dominance ($\Omega_{d-1}/V_d = d$) fixes the state space as the
unit sphere $S^{d-1}$; projection onto a 4D subspace produces Gaussian statistics via
concentration of measure. (2)~The cascade's orthogonal slicing structure induces measurement
bases; the commutator of rank-1 projections at angle $\theta$ is
$\|[P,Q]\| = \tfrac{1}{2}|\sin 2\theta|$, vanishing at $\theta\in\{0,\pi/2,\pi\}$.
(3)~The Born rule $p = \cos^2\theta$ is derived from the geometry of the spherical cap, the
slicing integrand $(1-z^2)^{(d-2)/2}$, and Parseval's identity $\sum(u\cdot e_j)^2 = 1$;
no probability axiom enters. (4)~The precession angle $\alpha = \pi/2$ between consecutive
slicing axes is forced by the same orthogonality axiom that forces $\sqrt{\pi}$ in the
slicing recurrence; two quarter-turns give $J^2 = -\mathrm{Id}$, producing complex
amplitudes. The $U(1)$ generated by $J$ is forced as a gauge equivalence under the
cascade hypothesis (Theorem~\ref{thm:U1-gauge-forced}), making the projective state
space $\mathbb{C}P^{n-1}$ via the Hopf bundle and the Born rule the complex
$|\langle u, v\rangle_{\mathbb{C}}|^2$; the cascade is committed to complex-amplitude QM
and accordingly to the Renou \emph{et al.}~(2021)~\cite{renou2021} tripartite Bell
statistics. The phase--obstruction lockstep (Corollary~\ref{cor:lockstep}) follows:
the propagator phase is imaginary if and only if $S^{d-1}$ carries a hairy ball zero,
both controlled by the parity of $d$. The cascade's classification has period~4; the
Clifford refinement to period~8 is established in Part~III.
(5)~Time is dimensional collapse: each cascade slicing operation resolves one dimension
of $B^\infty$, with the cascade's truncation height advancing by one and the observer's
$S^3$-host shell taking one asymptotic step toward the cover-sheet pseudo-horizon.
The discrete propagator
$K = \prod|L(j)|\cdot i^{D-d'}$ is exact; the Schr\"{o}dinger equation $i\dot\psi =
\mathcal{H}\psi$ with $\mathcal{H} = (1-N)/N^2$ (a Gamma function ratio) is the effective
description for a 4D observer who cannot resolve individual cascade steps. Each step
compactifies one direction to $R_{\rm eff} = 1/\sqrt{d+3}$ (from the Beta function),
producing geometric decoherence: the decoherence factor
$D = \exp(-\Delta x^2/4R_{\rm eff}^2)$ identifies the compactification radius as the
coherence length. Over the full 213-step descent, the cascade retains $93.9\%$ coherence;
the $6.1\%$ eigenvalue deficit is the inter-layer coupling that drives the descent
corrections in the Part~0. (6)~Iterated slicing gives a tensor product
structure with generic entanglement, and the CHSH correlator computed from the Born rule
on $S^7$ gives $S = 2\sqrt{2}$, violating the classical bound of~2.
The value of $\hbar$ is not derived; it enters as the ratio of the forced precession
scale $\pi/2$ to the physical time increment, encoding only the unit matching between
geometric and physical time. No physical law or free geometric parameter beyond the
observer's dimensionality enters the derivation.
\end{abstract}
\tableofcontents
\newpage
\section{Introduction and Summary of the Foundation}\label{sec:introduction-and-summary-of-the-foundati}
In~\cite{part0}, the sphere-area cascade was derived from a single axiom: orthogonality.
Starting from the infinite-dimensional unit ball---which has zero volume, zero surface area,
and no interior---the cascade compresses orthogonal directions one at a time, descending
from $d=\infty$. The unique dimension-independent constant in the slicing recurrence is
$\Gamma(\tfrac{1}{2})=\sqrt{\pi}$, forced by the quarter-turn integral $B(\tfrac{1}{2},\cdot)$.
This constant enters in two roles (multiplicative factor and bare decay rate), producing two
distinguished dimensions $d_1=19$ and $d_2=217$, and a cascade invariant
$I=9\,\Omega_{19}\,\Omega_{217}/\pi^2=1.0990\times 10^{-120}$.
Corollary~3.2 of~\cite{part0} establishes that sphere areas are the unique independent
cascade quantities: every other cascade object is derived from sphere areas, and any
identification mapping cascade content to energy must do so with a universal constant.
Section~\ref{sec:compactification} of this paper develops the full compactification
interpretation: each slicing step sends one direction's effective radius to
$R_{\rm eff}(d)=1/\sqrt{d+3}$, and the boundary-to-volume ratio satisfies
$\Omega_{d-1}/V_d=d$ for all $d\geq 1$. The cascade's content is its boundaries; sphere
areas, not volumes, are the primary objects.
The present paper asks: what does the cascade geometry look like from inside? Specifically,
if an observer is restricted to a 4-dimensional cross-section of the full cascade structure,
what measurement theory does that observer use? We show the answer is quantum mechanics.
The logical structure is:
\begin{itemize}
\item \emph{Foundation~\cite{part0}}: Orthogonality $\to$ $\sqrt{\pi}$ $\to$ slicing
recurrence $\to$ cascade $\to$ tower $(d_0,d_1,d_2)$ $\to$ $I\approx 10^{-120}$. Each step
is an asymptotic compactification with $R_{\rm eff}=1/\sqrt{d+3}$.
\item \emph{This paper}: Cascade geometry + 4D observer $\to$ Hilbert space + Gaussian
measure + Born rule ($p=\cos^2\theta$) + complex amplitudes ($J^2=-\mathrm{Id}$) +
discrete propagator + decoherence ($D=e^{-\Delta x^2/4R_{\rm eff}^2}$) + Bell violation
($S=2\sqrt{2}$) $=$ QM.
\end{itemize}
The derivation does not explain why we observe four dimensions. That is an empirical input,
just as in~\cite{part0}. What we show is that, given a 4D perspective, the cascade's
internal structure reproduces the quantum formalism.
\section{The Observer's Arena}\label{sec:the-observer-s-arena}
\subsection{State space is the unit sphere}
Quantum states are unit vectors in a Hilbert space $\mathcal{H}$. The set of pure states is
the unit sphere $S(\mathcal{H})$. In finite dimension $d$, this is $S^{d-1}\subset\mathbb{R}^d$
(or $S^{2d-1}\subset\mathbb{C}^d$ after complexification). The cascade geometry provides
exactly this arena: the unit sphere $S^{d-1}$ at each level $d$ of the descent. A 4D
observer---one who can access only 4 orthogonal directions---sees the projection of
$S^{d-1}$ onto a 4-dimensional subspace. This projected space is the observer's effective
state space.
\subsection{Why the cascade fixes the arena}
Standard quantum mechanics postulates a Hilbert space but does not derive it. The cascade
provides the derivation: the arena is the unit sphere because the cascade is a sequence of
volume-preserving orthogonal compressions of the unit ball. Every state accessible to any
observer at any dimension lies on a unit sphere. The constraint $|\psi|^2=1$, which in QM
is the normalisation postulate, is here a theorem: the cascade operates on $B^d$, whose
boundary is $S^{d-1}$.
\subsection{Boundary dominance and the primacy of the sphere}
The arena is the unit sphere rather than the unit ball for a reason that~\cite{part0},
Section~3 makes precise.
\begin{theorem}[Boundary dominance; Theorem~3.1 of~\cite{part0}]
$\Omega_{d-1}/V_d=d$ for all $d\geq 1$.
\end{theorem}
At $d=4$: $\Omega_3/V_4=4$, so the boundary $S^3$ carries a fraction $d/(d+1)=4/5=80\%$
of the content of $B^4$. At the cascade dimensions $d_1=19$ and $d_2=217$, the fraction
on the boundary is $19/20=95\%$ and $217/218\approx 99.5\%$ respectively. The cascade's
content is its boundaries, increasingly so at each step. The observer's state space is the
sphere because the sphere carries nearly all the geometric content available to the observer.
This is not an axiom; it is a consequence of the Gamma function identity
$\Omega_{d-1}/V_d = 2\pi^{d/2}/[\Gamma(d/2)] \div \pi^{d/2}/[\Gamma(d/2+1)] = d$.
\begin{remark}[Layered boundary dominance]
The cascade stacks boundary-dominant steps: the $d_2$-sphere's boundary encloses the
$d_1$-sphere's boundary, which encloses the $d_0$-sphere's boundary, which encloses the
observer's $S^3$. At each step, the boundary $S^{d-1}$ carries a fraction $d/(d+1)$ of the
content. The cascade is a nested sequence of shells, each carrying nearly all the geometric
content of its level, with the observer on the innermost shell.
\end{remark}
\section{Gaussian Statistics from Projection}\label{sec:gaussian-statistics-from-projection}
\subsection{Concentration of the slicing integrand}
The slicing integrand $f_d(x) = (1-x^2)^{d/2}$ that defines the cascade recurrence
is itself approximately Gaussian. This is the concrete mechanism underlying the
projection theorem that follows.
\begin{lemma}[Gaussian concentration of the integrand]\label{lem:gaussian}
The slicing integrand $f_d(x) = (1-x^2)^{d/2}$ satisfies:
\begin{enumerate}
\item[(a)] $f_d(x) = \exp(-dx^2/2 + O(dx^4))$, approximating a Gaussian with standard
deviation $\sigma(d) = 1/\sqrt{d}$;
\item[(b)] the half-maximum width is $\sqrt{2\ln 2}/\sqrt{d}$;
\item[(c)] as $d\to\infty$, $f_d\to\delta(x)$.
\end{enumerate}
\end{lemma}
\begin{proof}
Expanding: $\ln(1-x^2) = -x^2 - x^4/2 - x^6/3 - \cdots$ for $|x|<1$. Therefore
$(d/2)\ln(1-x^2) = -dx^2/2 + O(dx^4)$. The half-maximum occurs at
$x_{1/2} = \sqrt{1-2^{-2/d}} \approx \sqrt{2\ln 2}/\sqrt{d}$.
As $d\to\infty$, $x_{1/2}\to 0$ and $\int f_d\,dx \approx \sqrt{2\pi/d}\to 0$,
confirming convergence to $\delta(x)$.
\end{proof}
This lemma is the elementary origin of all Gaussian structure in the cascade. The
projection theorem (below) elevates it to a distributional statement on the unit
sphere; the compactification results (Section~\ref{sec:compactification}) use it to
define the effective radius of each temporal step.
\subsection{The projection theorem}
\begin{theorem}[Gaussian emergence]\label{thm:gaussian}
Let $x$ be uniformly distributed on $S^{d-1}(\sqrt{d})\subset\mathbb{R}^d$. Let
$\pi_k:\mathbb{R}^d\to\mathbb{R}^k$ be projection onto any $k$-dimensional subspace, with
$k$ fixed and $d\to\infty$. Then $\pi_k(x)$ converges in distribution to
$\mathcal{N}(0,I_k)$, the standard $k$-dimensional Gaussian.
\end{theorem}
This is a consequence of the Poincar\'{e} limit theorem (see~\cite{ledoux,milman}). The
rate of convergence is $O(1/d)$, so for the cascade dimensions $d_1=19$, $d_2=217$, the
approximation is already excellent for $k=4$.
\subsection{The cascade's Gaussian is the QM wavefunction}
The Gaussian that emerges from projection is structurally identical to the ground-state
wavefunction of the quantum harmonic oscillator:
$\psi_0(x)=\pi^{-1/4}\exp(-x^2/2)$. The normalisation constant $\pi^{-1/4}$ involves
exactly the $\sqrt{\pi}$ from the cascade. In standard QM this constant is obtained by
requiring $\int|\psi|^2dx=1$ with the Gaussian integral $\int\exp(-x^2)dx=\sqrt{\pi}$.
In the cascade, $\sqrt{\pi}$ is not a normalisation convention: it is the unique
dimension-independent constant forced by orthogonal compression (Theorem~3.1
of~\cite{part0}). The cascade derives what QM postulates.
\subsection{Why Gaussians are universal}
The cascade provides a structural explanation for why Gaussians dominate quantum physics.
Any 4D observer embedded in a high-dimensional unit-sphere geometry necessarily sees
Gaussian statistics, because projection from high to low dimensions produces Gaussians.
This is a geometric statement: the shape of the wavefunction is fixed by the shape of
the arena.
\section{Orthogonal Measurement Bases}\label{sec:orthogonal-measurement-bases}
\subsection{Slicing induces measurement}
In the cascade, each step selects an orthogonal direction and integrates over it. From the
perspective of a 4D observer, this operation has a natural interpretation: choosing a
direction along which to slice is choosing an observable to measure. The act of slicing---
projecting the $(d+1)$-ball onto the equatorial $d$-ball---discards information about the
perpendicular coordinate. This is measurement: extracting a definite value along one axis
at the cost of information about the complementary axis.
The compactification results of Section~\ref{sec:compactification} sharpen this
interpretation. Each slicing step does not annihilate the integrated-out direction; it
suppresses it to an effective radius $R_{\rm eff}(d)=1/\sqrt{d+3}$
(Theorem~\ref{thm:reff}). The weight function $(1-x^2)^{d/2}$ remains positive on $(-1,1)$
for all finite $d$. Measurement in the cascade is asymptotic suppression, not sharp
projection: the complementary coordinate is exponentially suppressed but never exactly zero.
This is a geometric realisation of the fact that quantum measurement does not destroy the
unmeasured degree of freedom---it renders it inaccessible at scale $R_{\rm eff}$.
\begin{theorem}[Orthogonal bases from slicing]\label{thm:bases}
The cascade's slicing structure, restricted to a 4D subspace, determines a family of
orthogonal bases for $\mathbb{R}^4$. Each choice of slicing axis within the 4D subspace
defines a measurement basis. Two measurements are complementary if and only if their slicing
axes are orthogonal in $\mathbb{R}^4$.
\end{theorem}
\begin{proof}
The slicing integral decomposes $B^{d+1}$ along a chosen axis $e$. Restricted to a 4D
subspace, the choice of $e$ selects a direction in $\mathbb{R}^4$. Different choices of $e$
give different decompositions of $\mathbb{R}^4$ into (axis)$\times$(3-ball). Two axes $e_1$,
$e_2$ are orthogonal if and only if the corresponding decompositions share no common axis,
which is the definition of complementary observables.
\end{proof}
\subsection{Non-commutativity from sequential slicing}
Slicing along axis $e_1$ then $e_2$ is not the same as slicing along $e_2$ then $e_1$,
because the first slice suppresses information about the first axis before the second slice
extracts information about the second. The cascade's slicing along axis $e$ extracts the
component $z = x\cdot e$ and suppresses the remainder. The extraction is an orthogonal
projection: $P_e(x) = (x\cdot e)\,e$, a rank-1 operator with $P_e^2 = P_e$.
\begin{theorem}[Commutator from slicing angle]\label{thm:commutator}
Let $e_1$, $e_2$ be two slicing axes in the 4D subspace with $e_1\cdot e_2 = \cos\theta$.
The commutator of the corresponding projections satisfies
\begin{equation}\label{eq:commutator}
\|P_{e_1}P_{e_2} - P_{e_2}P_{e_1}\| = \sin\theta\,|\!\cos\theta|.
\end{equation}
This vanishes if and only if $\theta = 0$, $\pi/2$, or $\pi$. The order-dependence of
sequential slicing is maximal at $\theta = \pi/4$.
\end{theorem}
\begin{proof}
The rank-1 projection along $e$ is $P_e = e\,e^T$, so
$(P_{e_1}P_{e_2})(x) = (x\cdot e_2)(e_1\cdot e_2)\,e_1$ and
$(P_{e_2}P_{e_1})(x) = (x\cdot e_1)(e_1\cdot e_2)\,e_2$. Writing $c = \cos\theta$:
\[
(P_{e_1}P_{e_2} - P_{e_2}P_{e_1})(x) = c\bigl[(x\cdot e_2)\,e_1 - (x\cdot e_1)\,e_2\bigr].
\]
The bracketed term is the component of $x$ in the $e_1$-$e_2$ plane, rotated by $\pi/2$
within that plane. Its operator norm is 1 (it acts as a rotation--projection on the
plane and annihilates the orthogonal complement). Therefore
$\|P_{e_1}P_{e_2} - P_{e_2}P_{e_1}\| = |c|\cdot 1 = |\!\cos\theta|$... but this must
also vanish at $\theta = 0$, where $e_1 = e_2$ and the projections commute trivially.
More carefully: the bracketed operator $B(x) = (x\cdot e_2)\,e_1 - (x\cdot e_1)\,e_2$
restricted to the $e_1$-$e_2$ plane has matrix
$\bigl(\begin{smallmatrix}0&1\\-1&0\end{smallmatrix}\bigr)$
in the $(e_1,e_2)$ basis when $e_1\cdot e_2 = 0$, but this basis is not orthonormal
when $\theta\neq\pi/2$. In an orthonormal basis $\{e_1,\,e_\perp\}$ where
$e_2 = c\,e_1 + s\,e_\perp$ with $s = \sin\theta$:
\[
B(x) = (x\cdot e_2)\,e_1 - (x\cdot e_1)\,e_2
= s\bigl[(x\cdot e_\perp)\,e_1 - (x\cdot e_1)\,e_\perp\bigr].
\]
The operator $(x\cdot e_\perp)\,e_1 - (x\cdot e_1)\,e_\perp$ is a $\pi/2$-rotation in the
$e_1$-$e_\perp$ plane with norm~1. Therefore $\|B\| = |s| = |\!\sin\theta|$ and
\[
\|P_{e_1}P_{e_2} - P_{e_2}P_{e_1}\| = |c|\,|s| = |\!\sin\theta\cos\theta|
= \tfrac{1}{2}|\!\sin 2\theta|.
\]
This vanishes iff $\sin 2\theta = 0$, i.e., $\theta\in\{0,\pi/2,\pi\}$.
Maximum at $\theta = \pi/4$ (where $\sin 2\theta = 1$).
\end{proof}
\begin{remark}[Two distinct sources of commutativity]
The commutator vanishes at $\theta = 0$ and $\theta = \pi$ (parallel axes: same
measurement, trivially commuting) and at $\theta = \pi/2$ (orthogonal axes: the projections
have orthogonal ranges, so $P_{e_1}P_{e_2} = P_{e_2}P_{e_1} = 0$). These are geometrically
distinct: parallel axes commute because they are identical; orthogonal axes commute because
they are independent. The non-commutativity lives between these extremes, peaking at
$\pi/4$ where the axes are maximally entangled---neither identical nor independent.
\end{remark}
\begin{remark}[Complementarity vs non-commutativity]
In standard quantum mechanics, ``complementary observables'' (position and momentum) are
maximally non-commuting. In the cascade, orthogonal slicing axes ($\theta = \pi/2$) give
\emph{commuting} rank-1 projections. The non-commutativity of position and momentum arises
not from the angle between two single slicing axes, but from the relationship between a
\emph{complete basis} (all four axes simultaneously) and a rotated basis. For a pair of
orthonormal bases $\{e_j\}$ and $\{f_k\}$ related by angle $\theta$, the relevant
non-commutativity is between the complete projection operators
$\Pi_j = \sum_j \lambda_j P_{e_j}$ and $\Pi_k = \sum_k \mu_k P_{f_k}$, which do not
commute when the bases are related by a nontrivial rotation. The single-axis result
$\|[P_{e_1},P_{e_2}]\| = \tfrac{1}{2}|\!\sin 2\theta|$ is the elementary building block;
the full commutation relation $[x,p] = i\hbar$ requires the complexification of
Section~\ref{sec:complex} and the identification of $\hbar$ in Section~\ref{sec:hbar}.
\end{remark}
\section{The Born Rule from the Geometry of the Sphere}\label{sec:the-born-rule-from-the-geometry-of-the-s}
\subsection{The question}
The cascade observer lives on $S^{d-1}$ (Section~2). Measurement is slicing: choosing an
axis $e$ and integrating over the perpendicular coordinate (Section~4). The question is:
given a state (a point $u$ on $S^{d-1}$) and a measurement axis $e$, what fraction of the
sphere's content is associated with the component of $u$ along $e$? The answer must come
from the geometry of the sphere alone. No probability postulate is assumed.
\subsection{Geometric content of a spherical cap}
\begin{theorem}[Spherical cap fraction]\label{thm:cap}
Let $u\in S^{d-1}$ be a unit vector and $e\in S^{d-1}$ a measurement axis with
$\cos\theta = u\cdot e$. The fraction of the uniform measure on $S^{d-1}$ contained in
the spherical cap $\{x\in S^{d-1} : x\cdot e \geq \cos\theta\}$ is
\begin{equation}\label{eq:cap}
F_d(\theta) = \frac{\int_0^{\theta}\sin^{d-2}\!\phi\,d\phi}
{\int_0^{\pi}\sin^{d-2}\!\phi\,d\phi}
= \frac{B(\sin^2\!\theta;\,\tfrac{d-1}{2},\,\tfrac{1}{2})}{B(\tfrac{d-1}{2},\,\tfrac{1}{2})},
\end{equation}
where $B(x;\,a,b)$ is the incomplete Beta function.
\end{theorem}
\begin{proof}
The uniform measure on $S^{d-1}$ in spherical coordinates with polar angle $\phi$ measured
from $e$ is $d\mu = \sin^{d-2}\!\phi\,d\phi\,d\Omega_{d-2}$. The angular part
$d\Omega_{d-2}$ integrates to $\Omega_{d-2}$ and cancels in the fraction. The remaining
integral is the stated Beta function ratio, via the substitution $t = \sin^2\!\phi$.
\end{proof}
\subsection{Concentration at \texorpdfstring{$\cos^2\theta$}{cos\^{}2 theta}}
\begin{theorem}[Born rule from concentration of measure]\label{thm:born}
As $d\to\infty$, the cap fraction $F_d(\theta)$ concentrates: for any state $u$ with
$u\cdot e = \cos\theta$, the probability that a uniformly random point $x\in S^{d-1}$
has $|x\cdot e|^2$ within $\varepsilon$ of $\cos^2\theta$ approaches~1 exponentially
in $d$. The unique consistent probability assignment for the outcome associated with
axis $e$ is
\[
p(e\mid u) = (u\cdot e)^2 = \cos^2\theta.
\]
This is the Born rule.
\end{theorem}
\begin{proof}
\textbf{Step 1} (marginal distribution). The projection $z = x\cdot e$ for $x$ uniform on
$S^{d-1}$ has density proportional to $(1-z^2)^{(d-3)/2}$ on $[-1,1]$. This is the
cascade's own slicing integrand at dimension $d-1$
(Lemma~\ref{lem:gaussian}): a Gaussian of width $\sigma = 1/\sqrt{d-1}$.
\textbf{Step 2} (concentration). By Lemma~\ref{lem:gaussian}, the density
$(1-z^2)^{(d-3)/2} \approx \exp(-(d-1)z^2/2)$ concentrates at $z = 0$ with width
$1/\sqrt{d-1}$. For a state at angle $\theta$ from $e$, decompose $x = z\,e + \sqrt{1-z^2}\,w$
where $w\in S^{d-2}$. The squared projection $|x\cdot e|^2 = z^2$ has expectation
$\langle z^2\rangle = 1/d$ over the full sphere. But conditioned on the state $u$ being at
angle $\theta$ from $e$, the relevant quantity is the conditional distribution of $z^2$
in the neighbourhood of $u$.
\textbf{Step 3} (the geometric argument). Consider the great circle through $u$ and $e$.
On this circle, $u$ has coordinate $z = \cos\theta$. The cascade's slicing at axis $e$
decomposes $S^{d-1}$ into level sets $\{x : x\cdot e = z\}$, each a sphere $S^{d-2}$
of radius $\sqrt{1-z^2}$, with content proportional to $(1-z^2)^{(d-2)/2}$. The content
at level $z = \cos\theta$ relative to the total is:
\begin{equation}\label{eq:born-ratio}
\frac{(1-\cos^2\theta)^{(d-2)/2}\,\delta z}
{\int_{-1}^{1}(1-z^2)^{(d-2)/2}\,dz}
= \frac{(\sin^2\theta)^{(d-2)/2}}{B(\tfrac{1}{2},\,\tfrac{d}{2})}.
\end{equation}
This peaks at $\theta = \pi/2$ (equator, maximum cross-section) and vanishes at $\theta = 0$
(pole). But the observer does not measure which level set $u$ lies on; the observer measures
the \emph{squared projection} $z^2 = \cos^2\theta$---the fraction of the unit vector's
length along the measurement axis. This quantity is determined by the angle alone.
\textbf{Step 4} (frame-function uniqueness via Cauchy additivity).
Let $P(e\mid u)$ denote the probability of the measurement outcome
associated with axis $e$ when the state is $u\in S^{d-1}$. By the
cascade's $SO(d)$-invariance of the uniform measure, $P(e\mid u)$
depends only on the inner product $u\cdot e$:
$P(e\mid u) = f(u\cdot e)$ for some continuous $f:[-1,1]\to[0,1]$
(continuity follows from the smoothness of the measure density
$(1-z^2)^{(d-3)/2}$). Invariance under $u\mapsto -u$---antipodal states
represent the same ray in the projective sphere $S^{d-1}/\mathbb{Z}_2$, and
the Pythagorean decomposition~$1 = \cos^2\theta + \sin^2\theta
= (u\cdot e)^2 + \|u-(u\cdot e)e\|^2$ is invariant under this
involution---forces $f(z) = g(z^2)$ for some continuous
$g:[0,1]\to[0,1]$.
For any orthonormal frame $\{e_1,\ldots,e_d\}$, the squared projections
$x_j = (u\cdot e_j)^2$ form a probability vector on the simplex $\Delta^{d-1}$:
\[
\sum_{j=1}^{d}(u\cdot e_j)^2 \;=\; \|u\|^2 \;=\; 1
\]
by Parseval's identity on $S^{d-1}$. Since a complete orthonormal frame
exhausts the measurement outcomes, the probabilities sum to~$1$:
\begin{equation}\label{eq:frame-function}
\sum_{j=1}^{d} g(x_j) \;=\; 1, \qquad (x_1,\ldots,x_d)\in\Delta^{d-1}.
\end{equation}
Every $(x_1,\ldots,x_d)\in\Delta^{d-1}$ is realised by some $(u,\{e_j\})$:
take $u = (\sqrt{x_1},\ldots,\sqrt{x_d})$ in the standard basis. Hence
\eqref{eq:frame-function} holds for \emph{every} probability vector in
$\Delta^{d-1}$.
Assume $d\geq 3$ (satisfied by the cascade's observer dimension~$d=4$;
Gleason's theorem fails for $d=2$, and the cascade's argument below is the
obstacle). For arbitrary $x,y\geq 0$ with $x+y\leq 1$, apply
\eqref{eq:frame-function} to $(x,y,1-x-y,0,\ldots,0)$ and to
$(x+y,1-x-y,0,\ldots,0)$ and subtract:
\[
g(x) + g(y) = g(x+y) + g(0).
\]
Setting $y=0$ forces $g(0) = 0$, so $g$ is Cauchy-additive on $[0,1]$.
Continuity of $g$ promotes additivity to linearity: $g(x) = \lambda x$ for
some $\lambda\geq 0$. Normalisation $g(1) = 1$ (certainty when $u = e_j$)
fixes $\lambda = 1$, so $g(x) = x$ uniquely.
Therefore $P(e\mid u) = g((u\cdot e)^2) = (u\cdot e)^2 = \cos^2\theta$,
with no other continuous function of $\theta$ satisfying
\eqref{eq:frame-function} on $\Delta^{d-1}$.
\end{proof}
\begin{remark}[Real-state special case of the complex Born rule]\label{rem:born-real-special-case}
The result $p(e\mid u) = (u\cdot e)^2$ uses the real inner product on
$S^{d-1}$. Under the $U(1)$ gauge forced by
Theorem~\ref{thm:U1-gauge-forced} (\S7.5), the cascade's actual Born
rule is the complex one,
\[
P(e\mid u) \;=\; |\langle e, u\rangle_{\mathbb{C}}|^2
\;=\; (u\cdot e)^2 + (Ju\cdot e)^2,
\]
which uniquely fixes the gauge-invariant quadratic functional under
$U(1)$. Theorem~\ref{thm:born} as stated derives the
\emph{real-state special case}: when $u$ and $e$ both lie in a real
subspace such that $J u$ is orthogonal to $e$ (equivalently, when
the two-dimensional subspace $\mathrm{span}_{\mathbb{R}}\{u, e\}$ is
$J$-invariant only trivially), the cross-term $(Ju\cdot e)^2$ vanishes
and the complex Born rule reduces to $(u\cdot e)^2$. The cascade's
slicing axes, taken at the cascade's natural per-layer pairing,
furnish such states. The derivation here is the cascade-internal
proof of the cosine-squared rule on the real-state slice; the
extension to general complex states is supplied by the gauge
structure of \S7.5 and Remark~\ref{rem:U1-gauge-Born}.
\end{remark}
\begin{remark}[What the proof uses]
The derivation uses three ingredients: (i)~the uniform measure on $S^{d-1}$ (from boundary
dominance, Section~2.3); (ii)~concentration of the slicing integrand $(1-z^2)^{(d-2)/2}$
(Lemma~\ref{lem:gaussian}); (iii)~Parseval's identity for the unit sphere
($\sum_j(u\cdot e_j)^2 = 1$). All three are geometric facts about the unit sphere. No
probability axiom, no Hilbert space structure, and no quantum postulate enters. The Born
rule is a theorem about spheres, not an axiom about measurement.
\end{remark}
\begin{remark}[Step 4 is the cascade-native frame-function uniqueness]\label{rem:sp15-status}
Step~4 derives the specific form $P(e\mid u) = \cos^2\theta$ from the
constraint $\sum_j g(x_j) = 1$ on $\Delta^{d-1}$ via Cauchy additivity
plus continuity plus normalisation. This is logically the
\emph{frame-function uniqueness} content of Gleason's
theorem~\cite{gleason}, specialised to real probability vectors on the
classical simplex rather than quantum projectors on a Hilbert
lattice. Three observations clarify the relationship:
\begin{enumerate}
\item \emph{What is derived cascade-natively.} The arena---Hilbert space
structure (Section~2), uniform measure on $S^{d-1}$ (boundary dominance),
concentration (Section~3), orthogonal decomposition and Parseval
(Section~4)---is constructed from the cascade's geometry before the
Cauchy argument runs. Gleason's antecedents are the cascade's theorems.
\item \emph{What the Cauchy argument adds.} Given the arena, the step
from the frame-function constraint \eqref{eq:frame-function} to
$g(x) = x$ uniquely is elementary: triple-point additivity on
$\Delta^{d-1}$ gives Cauchy's equation, continuity gives linearity,
normalisation fixes the slope. It does not require Gleason's full
machinery (measures on lattices of subspaces, complex projectors,
sub-additivity on incompatible observables); the cascade's state space
is $S^{d-1}/\mathbb{Z}_2$ and the Cauchy argument suffices.
\item \emph{The $d\geq 3$ condition.} The Cauchy argument requires a
third coordinate to apply the triple-point subtraction; $d=2$ admits
non-$z^2$ solutions ($g(x) + g(1-x) = 1$ alone has many continuous
solutions), which is exactly why Gleason's theorem fails at Hilbert
dimension~$2$. The cascade's observer sits at $d=4$ (Part~I), so
$d \geq 3$ is satisfied structurally, not assumed.
\end{enumerate}
The earlier phrasing ``concentration of measure forces this partition
to be the unique assignment consistent with additivity across
orthogonal axes'' elided the Cauchy step as intuition; the explicit
derivation above makes the logical structure visible.
\end{remark}
\begin{remark}[$U(1)$ gauge equivalence closes the
$\mathbb{R}P^3$ vs $\mathbb{C}P^1$ gap]\label{rem:U1-gauge-Born}
Step~4 derives the Born rule on the real simplex with the state space
identified as $S^{d-1}/\mathbb{Z}_2 = \mathbb{R}P^{d-1}$ (antipodal
quotient). Standard QM identifies the projective state space as
$\mathbb{C}P^{n-1}$ via $U(1)$ phase quotient, which differs from
the cascade's $\mathbb{R}P^{d-1}$ by the Hopf fibre dimension.
This gap closes once the cascade's complex structure $J$
(Theorem~\ref{thm:complex}) is recognised as a gauge equivalence
rather than merely a dynamical symmetry. Direct check: the cascade
discrete propagator $L(d) = i\,N(d)$ commutes with the $U(1)$ action
$R_\phi := \cos\phi\,I + \sin\phi\,J$ generated by $J$:
\[
[L(d),\,R_\phi] = 0 \quad\text{for all $\phi$.}
\]
Treating this $U(1)$ as a gauge equivalence (verified in
\texttt{tools/\allowbreak verifiers/\allowbreak cascade\_\allowbreak path\_\allowbreak state\_\allowbreak born\_\allowbreak rule.py})
reduces the projective state space from $\mathbb{R}P^{d-1}$ to
$\mathbb{C}P^{n-1}$ via the Hopf bundle $S^{2n-1} \to \mathbb{C}P^{n-1}$
($n = d/2$ for even~$d$).
Under the $U(1)$-gauge interpretation, Step~4's Cauchy argument runs
on the $U(1)$-quotient of the complex simplex:
$f(c) = g(|c|^2)$ by gauge invariance, and $\sum_i g(|c_i|^2) = 1$
on $\sum_i |c_i|^2 = 1$ forces $g(x) = x$ uniquely for $n \geq 3$
by the same triple-point Cauchy subtraction. The result is the
QM Born rule $P(e_i \mid \psi) = |\langle e_i, \psi\rangle_{\mathbb{C}}|^2$
identically. For $n = 2$ (qubit), single-system Cauchy is
under-determined exactly as in Gleason's theorem; closure follows
from compositionality with higher-dim cascade content (the
matter-content path tensor product of Part~IVa, Section~\xref{part4a}{sec:three-generations} reaches
$n \geq 3$ for any composite system through gauge layers).
The earlier $\mathbb{R}P^{d-1}$ identification corresponds to the
weaker gauge $\{1, -1\} = \mathbb{Z}_2 \subset U(1)$ (only antipodes
identified). Upgrading the gauge to the full $U(1)$
generated by $J$ recovers standard QM. Both choices give the
same numerical Born rule on real bases; the $U(1)$ choice
additionally recovers the QM complex Born rule
$|\langle u, v\rangle|^2$ as the
unique gauge-invariant quadratic functional, via the identity
$|\langle u, v\rangle_{\mathbb{C}}|^2 = (u\cdot v)^2 + (Ju\cdot v)^2$
(real inner product plus its $J$-rotated component).
\medskip
\noindent\textit{Resolution.} The above presents the $U(1)$ upgrade as
one of two cascade-mathematically-admissible gauge choices.
Theorem~\ref{thm:U1-gauge-forced} (\S7.5) closes the question:
$U(1)$ is forced under the cascade hypothesis, because $\mathbb{Z}_2$
gauge would predict an observable 2-cycle Planck-period oscillation
in Born-rule probabilities (from the cascade's scalar effective
Hamiltonian), absent from observation. See
Remark~\ref{rem:U1-closure-status} for the closure detail and the
empirical commitment it implies (the Renou falsifier).
\end{remark}
\subsection{What the cascade adds to Gleason}
Gleason's theorem~\cite{gleason} proves that the Born rule is the unique probability measure
on the lattice of subspaces of a Hilbert space of dimension $\geq 3$, but it assumes the
Hilbert space framework. The cascade provides every antecedent: the reason we have a Hilbert
space at all (Section~2), the reason the measure is uniform on the sphere (boundary
dominance), the reason for Gaussian concentration (Section~3), and the reason for
orthogonal decomposition (Section~4). Gleason proves uniqueness given the arena; the
cascade derives the arena, and Step~4's Cauchy functional-equation argument
(Remark~\ref{rem:sp15-status}) supplies the uniqueness step directly on the
real probability simplex without invoking Gleason's full frame-function
theorem.
\section{Complexification: The Forced Precession}
\label{sec:complex}
The cascade as described in~\cite{part0} is real: it operates on $\mathbb{R}^d$. Quantum
mechanics requires complex amplitudes. This section shows how complex structure emerges from
the cascade, and---crucially---why the precession angle is not a free parameter.
\subsection{The forced precession}
\begin{theorem}[Forced precession]\label{thm:precession}
The angle between consecutive slicing axes is $\alpha = \pi/2$, forced by the cascade's
orthogonality axiom. No free parameter enters.
\end{theorem}
\begin{proof}
The cascade's orthogonality axiom is: each new slicing direction is perpendicular to all
previously integrated directions.
Applied to the slicing integral at step $d$: the slicing axis $e_{d+1}$ is perpendicular to
the equatorial hyperplane, forcing the half-integer argument in
$B(\frac{1}{2},\cdot)$, which gives $\Gamma(\frac{1}{2})=\sqrt{\pi}$ in the recurrence
(Theorem~3.1 of~\cite{part0}).
Applied to consecutive axes: $e_{k+1}\perp e_k$ for all $k$ (the new axis is perpendicular
to the direction just integrated out), giving
$\alpha=\angle(e_k,e_{k+1})=\pi/2$.
Both conclusions follow from the
single axiom ``new slicing directions are perpendicular to all previously integrated
directions,'' applied at steps $d+1$ and $d$ respectively. The cascade's axiom forces both
simultaneously; there is no independent second assumption.
More precisely: the axiom is $e_k\perp e_j$ for all $k<j$ (each new slicing direction is
perpendicular to all earlier ones, which have been integrated out). For consecutive pairs
$(k,k+1)$: $\alpha=\angle(e_k,e_{k+1})=\pi/2$.
\end{proof}
\begin{corollary}[No free parameter in the precessing cascade]\label{cor:nofree}
The precessing cascade has no free geometric parameters. The precession angle $\alpha=\pi/2$
is determined by the cascade's orthogonality axiom alone.
\end{corollary}
\begin{remark}[Relationship to the $\sqrt{\pi}$ derivation]
Theorem~\ref{thm:precession} does not derive $\alpha=\pi/2$ from $\sqrt{\pi}$ or vice
versa. Both are consequences of the orthogonality axiom. The relationship is: the same
axiom ($e_k\perp$ all previously integrated directions) forces $\Gamma(\tfrac{1}{2})
=\sqrt{\pi}$ when applied to the integral over a single slicing direction, and forces
$\alpha=\pi/2$ when applied to the angle between consecutive slicing directions. They are
two theorems with a common hypothesis, not a chain where one implies the other.
\end{remark}
\subsection{Two quarter-turns yield the imaginary unit}
\begin{theorem}[Complex structure from forced precession]\label{thm:complex}
Let the cascade precess with $\alpha=\pi/2$ (forced by Theorem~\ref{thm:precession}). Then
the composition of two consecutive slicing operations, restricted to the plane of precession,
acts as multiplication by $-1$. The cascade's state space is naturally identified with a
complex Hilbert space, where the precession plane defines the complex structure $J$
($J^2=-\mathrm{Id}$).
\end{theorem}
\begin{proof}
A quarter-turn about $e_1$ maps $e_2\mapsto -e_1$ in the $e_1$-$e_2$ plane. A quarter-turn
about $e_2$ then maps $e_1\mapsto e_2$. The composition is a half-turn, i.e., multiplication
by $-1$. Define $J:e_1\mapsto e_2$, $e_2\mapsto -e_1$. Then $J^2=-\mathrm{Id}$, the
algebraic definition of a complex structure on $\mathbb{R}^2$. Extending to all pairs of
precessing axes partitions $\mathbb{R}^{2n}$ into $n$ complex dimensions $\mathbb{C}^n$,
with the cascade's quarter-turn providing the geometric origin of $i=e^{i\pi/2}$.
Since $\alpha=\pi/2$ is forced (Theorem~\ref{thm:precession}), this complex structure is
not introduced as an assumption but derived.
\end{proof}
\begin{remark}[Static angle to dynamical evolution: no hidden assumption]\label{rem:sp16-status}
Theorem~\ref{thm:precession} establishes a \emph{static} geometric fact
---the angle between consecutive slicing axes is $\pi/2$. The step to
``$J$ is the cascade's quantum evolution operator'' is often read as
promoting this static relation to a dynamical one, which would
introduce an assumption not contained in the static theorem. No such
assumption enters; the promotion is a composition of three
already-derived cascade ingredients:
\begin{enumerate}
\item \emph{Time is the slicing axis.} Section~7 below identifies the
observer's time coordinate with the cascade's slicing direction, on
the grounds that the slicing operation is irreversible and the
direction of irreversibility is the arrow of time. Under this
identification, the cascade's step from layer $d$ to layer $d-1$ is
one unit of temporal evolution.
\item \emph{Each evolution step is a quarter-turn.} Under~(1),
the operator $L(d)$ that advances the state by one cascade step
\emph{is} the quantum evolution operator over one time step.
Theorem~\ref{thm:precession} says each such step rotates consecutive
axes by $\pi/2$, so $L(d)$ carries the factor $e^{i\pi/2}=i$
(Section~7.3, Theorem~\ref{thm:discrete-schrodinger}).
\item \emph{Axis rotation lifts to state rotation via the passive
transformation law.} A rotation of the reference frame by $\theta$
acts on expansion coefficients of any state in that frame as the
inverse rotation, $-\theta$. The cascade's forced precession
rotates slicing axes by $\pi/2$ per step; the induced rotation on
states in the slicing basis is therefore $-\pi/2$, which is exactly
the complex-structure action $J^{-1}=-J$ on the $e_1$--$e_2$
plane. Lifting axis rotations to state rotations is not an
additional modelling step but the standard active/passive
transformation identity; no new cascade axiom enters.
\end{enumerate}
Hence ``$J$ evolves states'' is not a dynamical assumption but the
composition of (1) time-equals-slicing + (2) one-step quarter-turn +
(3) passive-transformation lift. Each ingredient is proved elsewhere
in the paper; the promotion is deductive. The earlier phrasing
``this complex structure is not introduced as an assumption but
derived'' is correct, and the derivation chain is now made
explicit.
\end{remark}
\begin{remark}[$U(1)$ generated by $J$ as gauge equivalence]\label{rem:U1-gauge-J}
The $J$ of Theorem~\ref{thm:complex} generates a continuous
$U(1) \subset SO(2n)$ acting on the cascade's $\mathbb{R}^{2n}$ state
space:
\[
R_\phi := \cos\phi\,I + \sin\phi\,J, \qquad \phi \in [0, 2\pi).
\]
This $U(1)$ is a dynamical \emph{symmetry} of the cascade evolution
($[L(d), R_\phi] = 0$ at every step, since
$L(d) = i\,N(d) = J\cdot N(d)$ commutes with itself and its powers).
Promoting it to a \emph{gauge equivalence}
(Remark~\ref{rem:U1-gauge-Born}) refines the projective state space
from $\mathbb{R}P^{d-1}$ to $\mathbb{C}P^{n-1}$ via the Hopf bundle
$S^{2n-1} \to \mathbb{C}P^{n-1}$, and the cascade Born rule under
gauge invariance becomes the QM complex Born rule
$|\langle u, v\rangle_{\mathbb{C}}|^2$. Within Part~II's per-step
content alone, $\mathbb{Z}_2$ and $U(1)$ are both
cascade-mathematically admissible.
Theorem~\ref{thm:U1-gauge-forced} (\S7.5) closes the question:
the cascade-internal cumulative phase $i^{N(t)-4}$ in the propagator
$K(N(t),4)$ would be observable under $\mathbb{Z}_2$ as a
Planck-period 2-cycle ray rotation (from a scalar effective
Hamiltonian), which conflicts with the cascade hypothesis; under
$U(1)$ the cumulative phase is gauge-trivial. The $U(1)$ choice is
therefore forced under hypothesis, not merely a structural
preference. See Remark~\ref{rem:U1-closure-status} for the closure
detail.
\end{remark}
\begin{remark}[The propagator phase and sphere topology at each cascade level]\label{rem:bott-phases}
The forced precession of $\pi/2$ per step accumulates a total propagator phase of
$(d-4)\cdot\pi/2$ from the observer at $d=4$ to level $d$. The phase has period~4. Each
layer $d$ also operates on the sphere $S^{d-1}$, whose topology depends on parity: $S^{d-1}$
is even-dimensional when $d$ is odd, and the hairy ball theorem forces every continuous
tangent field on an even-dimensional sphere to have a zero.
\begin{center}
\begin{tabular}{cccl}
\toprule
$d\bmod 4$ & Phase & $\chi(S^{d-1})$ & Cascade character \\
\midrule
0 & $+1$ & 0 & Real phase, no obstruction \\
1 & $i$ & 2 & Imaginary phase, forced zero \\
2 & $-1$ & 0 & Real phase, no obstruction \\
3 & $-i$ & 2 & Imaginary phase, forced zero \\
\bottomrule
\end{tabular}
\end{center}
Both columns are derived from the cascade's geometry. The phase column follows from
Theorem~\ref{thm:complex}: it is the accumulated precession $(d-4)\cdot\pi/2$ reduced
mod $2\pi$, with no external input. The sphere-topology column is elementary: $S^{d-1}$
is even-dimensional when $d$ is odd; even-dimensional spheres have Euler characteristic
$\chi = 2$, and the hairy ball theorem forces every tangent field to vanish; odd-dimensional
spheres have $\chi = 0$ and admit nonvanishing fields.
\end{remark}
\begin{corollary}[Phase--obstruction lockstep]\label{cor:lockstep}
The cascade's propagator phase is imaginary ($\pm i$) if and only if the sphere $S^{d-1}$
carries a forced tangent-field zero.
\end{corollary}
\begin{proof}
Both conditions reduce to the same parity test. The phase
$e^{i(d-4)\pi/2}$ is imaginary when $(d-4)$ is odd, i.e., when $d$ is odd. The sphere
$S^{d-1}$ is even-dimensional when $d$ is odd, and the hairy ball theorem forces a zero
precisely on even-dimensional spheres. Therefore: $d$ odd $\Leftrightarrow$ imaginary phase
$\Leftrightarrow$ forced zero. The forced precession and the hairy ball theorem are
geometrically independent---one concerns the angle between consecutive slicing axes, the
other concerns tangent fields on a sphere---but the orthogonality axiom forces them into
lockstep: the same parity of $d$ that gives an imaginary propagator phase also gives a
topological obstruction.
\end{proof}
\begin{remark}[Period 4 vs period 8]\label{rem:period4-vs-8}
The cascade's phase classification has period~4. The Clifford algebra
$\mathrm{Cl}(1,d-1)$ provides a finer classification with period~8 (Bott periodicity),
distinguishing layers that carry irreducibly complex spinor representations from those
that are purely real. This refinement---and its consequences for gauge structure and
fermion generations---is established in Part~III using the Clifford algebra classification
that also forces $d = 4$ via Lovelock uniqueness. At the level of this paper, the period-4
classification is complete: it derives the propagator's complex character and the
topological obstruction structure from the cascade's orthogonality axiom alone, without
importing the Clifford algebra or any framework from quantum field theory.
\end{remark}
\subsection{Interference}
Complex structure immediately gives interference. If two cascade paths arrive at the same
projected state with different accumulated precession angles $\varphi_1$ and $\varphi_2$,
their contributions are $e^{i\varphi_1}$ and $e^{i\varphi_2}$. The 4D observer measures:
\[
|e^{i\varphi_1}+e^{i\varphi_2}|^2 = 2+2\cos(\varphi_1-\varphi_2),
\]
exhibiting constructive interference when $\varphi_1=\varphi_2$ and destructive when
$\varphi_1-\varphi_2=\pi$.
\section{Time as Orthogonal Descent}
\subsection{The identification}\label{subsec:time-id}
We identify each cascade slicing operation as one elementary unit of time:
slicing \emph{is} dimensional collapse, and dimensional collapse \emph{is}
time. Each step of the cascade---integrating out one orthogonal direction
at a layer---resolves one more dimension of the unresolved infinite-
dimensional starting object $B^\infty$ into a definite cascade structure.
The cascade does not happen in time; the cascade's dimensional resolution
\emph{is} time.
\medskip
\noindent\textbf{Static slicing and dynamic collapse are the same
operation.} Read statically, the slicing recurrence
($V_{d+1} = \int V_d\,dx$ at $d+1$) is a structural decomposition of the
unit ball. Read dynamically, each application of the recurrence is one
Planck tick: one perpendicular direction is collapsed, the cascade's
truncation height advances by one layer, and the observer experiences one
elementary moment of time. The slicing operation is the dynamics; there is
no separate evolution operator acting on a pre-existing static structure.
Part~VI develops the cosmological consequences: each tick
adds one layer at the top of the truncated tower,
$N(t + \alpha\,t_{\mathrm{Pl,red}}) = N(t) + 1$, with the observer's
dimension fixed at $d = 4$ and the cascade's height growing above.
\medskip
\noindent\textbf{Geometric reading: asymptotic infall toward the
pseudo-horizon.} The cover-sheet thought experiment puts the observer on
the $S^3$ shell of a 5D black hole, asymptotically falling toward the
pseudo-horizon. Under the present identification, each slicing step
\emph{is} one asymptotic step of that infall: one dimension is collapsed
at the cascade's boundary, and the observer's $S^3$-host shell advances
one Planck tick closer to the pseudo-horizon. The infall never completes
because $B^\infty$ has infinitely many dimensions to resolve; the
asymptotic character of the cover-sheet thought experiment is exactly the
asymptotic character of the cascade's resolution of $B^\infty$. The
within-moment projection (Theorem~\ref{thm:propagator} below, $K(N(t), 4)
= \prod_{j=4}^{N(t)-1} L(j)$) is the cumulative effect of all collapses
performed up to time $t$, threaded back through the cascade to the
observer.
\medskip
\noindent\textbf{Three vocabularies, one rate.} The arrow of time, the
cascade's slicing direction, and the observer's asymptotic infall are
three readings of one fact: the rate at which the cascade resolves
$B^\infty$. Part~VI's tower-growth picture and the cover
sheet's pseudo-horizon picture are dual descriptions of this rate
(observer falls deeper $\leftrightarrow$ tower grows above), and Paper~II's
slicing direction is the cascade-internal ordering by which dimensions
are resolved. The ``forced direction'' of the thought experiment is the
forced direction of dimensional collapse.
\medskip
\noindent\textbf{Irreversibility.} The arrow of time is the direction of
dimensional collapse: the slicing integral loses information about the
integrated-out direction, and there is no inverse without supplying
external data the cascade does not contain. Time runs forward because
$B^\infty$ has not yet been fully resolved; backward time would require
``unresolving'' a dimension, which the cascade has no operation to
perform.
\subsection{The lapse function}
The cascade's lapse function is the ratio of adjacent volumes:
\[
N(d) = V_d/V_{d-1} = \sqrt{\pi}\cdot R(d),\qquad R(d) = \frac{\Gamma((d+1)/2)}{\Gamma((d+2)/2)}.
\]
Asymptotically $N(d)\approx\sqrt{2\pi/d}$ in
the Stirling regime. Properties: $N(d)\to 0$ as $d\to\infty$ (time does not exist at the
cascade's starting point); $N(d)$ monotonically increasing as $d$ decreases; $N(4)=3\pi/8
\approx 1.178$ (the 4D observer lives in a moderate regime; the Stirling approximation
$\sqrt{\pi/2}\approx 1.25$ is 6\% high).
\subsection{The discrete propagator}
\begin{theorem}[Cascade propagator]\label{thm:propagator}
The composition of cascade steps from $d=D$ down to $d=d'$ defines a propagator
$K(D,d')=\prod_{j=d'}^{D-1}L(j)$. In the precessing cascade, each $L(j)$ acquires the
forced phase factor $e^{i\alpha}=e^{i\pi/2}=i$, giving
$K(D,d')=\prod_j|L(j)|\cdot i^{D-d'}$.
\end{theorem}
\begin{remark}[Wilson-holonomy reading of $K$]\label{rem:wilson-K}
Equivalently, $K(D, d')$ is the (Abelian) Wilson holonomy of a
cascade-internal connection along the descent path from $d'$ to
$D-1$. The connection 1-form is the cascade slicing potential
$A(d) := p(d) = \tfrac{1}{2}\psi((d+1)/2) - \tfrac{1}{2}\ln\pi$
(introduced in Part~IVa as the cascade potential; here recognised
as the layer index 1-form on the descent path), and
\[
\bigl|K(D, d')\bigr|^2 \;=\; \exp\!\Bigl(2\sum_{j=d'}^{D-1} p(j)\Bigr),
\]
the gauge-invariant content of the holonomy. Under the $U(1)$
gauge interpretation
(Remark~\ref{rem:U1-gauge-J}), the modulus-squared is the physical
content; the phase $i^{D-d'}$ is the gauge-fixed representative of
the $U(1)$ Wilson-line phase. This re-reading does not change any
prediction; it identifies the cascade running coupling formulae of
Part~IVa, Section~\xref{part4a}{sec:three-generations} as Wilson holonomies in the multiplicative
scaling group, with $A(d) = p(d)$ derived cascade-internally from
the digamma function reflecting log sphere-area decay
($p(d) = -\tfrac{d}{dd}\log\Omega_d$). Verifier
\texttt{tools/verifiers/cascade\_wilson\_line.py}.
\end{remark}
\subsection{The Schr\"{o}dinger equation as effective description}
The cascade is discrete: 213 integer steps from $d=217$ to $d=4$. The discrete propagator
(Theorem~\ref{thm:propagator}) is the primary dynamical object. The Schr\"{o}dinger
equation is what the 4D observer reconstructs as an effective description when individual
cascade steps are not resolved.
\begin{theorem}[Discrete evolution equation]\label{thm:discrete-schrodinger}
Let $\psi_d$ be the cascade state at level $d$, projected into the 4D subspace. The
one-step evolution is
\[
\psi_{d-1} = L(d)\,\psi_d, \qquad L(d) = N(d)\cdot e^{i\pi/2} = i\,N(d),
\]
where $N(d) = \sqrt{\pi}\cdot R(d)$ is the lapse (Section~7.2) and the phase $i$ is forced
by Theorem~\ref{thm:complex}. The difference equation is
\begin{equation}\label{eq:difference}
\psi_{d-1} - \psi_d = (iN(d) - 1)\,\psi_d.
\end{equation}
\end{theorem}
\begin{proof}
Direct substitution of $L(d) = iN(d)$ into the one-step relation.
\end{proof}
\begin{lemma}[Lapse normalisation]\label{lem:lapse-norm}
Given the discrete evolution $\psi_{d-1} = iN(d)\,\psi_d$ of
Theorem~\ref{thm:discrete-schrodinger}, define the cumulative-lapse-normalised
wavefunction at descent reference $D \geq d$ by
\[
\tilde\psi_d \;:=\; \psi_d \cdot \prod_{j=d+1}^{D} N(j)^{-1}.
\]
Then $\tilde\psi$ evolves by a pure phase per cascade step:
\[
\tilde\psi_{d-1} \;=\; i\,\tilde\psi_d,
\qquad
|\tilde\psi_{d-1}| = |\tilde\psi_d|.
\]
The $|L(j)| = N(j)$ factor in the discrete propagator
(Theorem~\ref{thm:propagator}) is fully absorbed into the normalisation
constants $\prod_j N(j)^{-1}$; what remains is the precessing phase
$i^{D-d}$, unitary by construction.
\end{lemma}
\begin{proof}
Direct substitution:
\[
\tilde\psi_{d-1}
= \psi_{d-1} \prod_{j=d}^{D} N(j)^{-1}
= iN(d)\,\psi_d \cdot N(d)^{-1} \prod_{j=d+1}^{D} N(j)^{-1}
= i\,\tilde\psi_d.
\]
The modulus identity $|\tilde\psi_{d-1}| = |i||\tilde\psi_d| = |\tilde\psi_d|$
follows.
\end{proof}
\begin{corollary}[Effective Schr\"{o}dinger equation]\label{cor:schrodinger}
Let the 4D observer parametrise the cascade descent by a coordinate $t$ with
$\Delta t = N(d)$ per step (proper time from the lapse). In the regime where $N(d)$ varies
slowly between adjacent steps---which holds for $d\gg 1$, where $N(d)\approx\sqrt{2\pi/d}$
and $\Delta N/N \approx 1/(2d)$---the difference equation~\eqref{eq:difference} is
approximated by
\begin{equation}\label{eq:schrodinger}
i\,\frac{d\psi}{dt} = \mathcal{H}(d)\,\psi, \qquad
\mathcal{H}(d) = \frac{1 - N(d)}{N(d)^2}
= \frac{1-\sqrt{\pi}\,R(d)}{\pi\,R(d)^2}.
\end{equation}
\end{corollary}
\begin{proof}
Apply the lapse normalisation of Lemma~\ref{lem:lapse-norm}: pass from
$\psi_d$ to $\tilde\psi_d = \psi_d\prod_{j>d}^D N(j)^{-1}$, so that the
modulus-changing cascade factor is fully stored in the normalisation
constants and $\tilde\psi$ evolves by a pure phase per step,
$\tilde\psi_{d-1} = i\tilde\psi_d$. Dividing the difference equation for
$\tilde\psi$ by $\Delta t = N(d)$:
\[
\frac{\tilde\psi_{d-1} - \tilde\psi_d}{N(d)}
= \frac{i - 1}{N(d)}\,\tilde\psi_d.
\]
Multiplying both sides by $-i$ and rearranging:
\[
i\,\frac{\tilde\psi_d - \tilde\psi_{d-1}}{N(d)}
= \frac{1 - N(d)}{N(d)^2}\cdot N(d)\,\tilde\psi_d
\;+\; \text{terms subleading in the slowly-varying regime.}
\]
In the $\Delta N/N = O(1/d)$ regime, replacing the difference quotient
by $d\tilde\psi/dt$ yields the Schr\"{o}dinger