The idea: deviation from the flat model
Zoom into the magnetic geometry at a point $q_0$ and it looks like the flat Heisenberg model with the constant field $B_0 = B(q_0)$ — that is the tangent cone (Part 2). But zoom out a little and the real field varies, and the geometry departs from Heisenberg. The caustic — the pattern where a family of Larmor orbits refocuses — captures that departure precisely.
For the flat model the orbits refocus at exactly the Larmor period $t_c = 2\pi/(B_0\lvert w\rvert)$. For the real, varying field they refocus a little differently, and the nilpotent deviation
\[\delta \;=\; \Big\langle\, 1 - \frac{|w|\,B_0}{2\pi}\, t_c(\theta_0, w) \,\Big\rangle_{\theta_0}\]measures the fractional departure, averaged over the launch direction $\theta_0$. It is zero for a uniform field, by construction. The question is what it becomes when the field has a gradient.
The only dimensionless knob
Put a clean, constant gradient on the field: $B = B_0\,e^{g x}$, the unique family with exactly constant $\nabla\ln B = g$. A Larmor orbit has one length scale, its radius $r_L = 1/(B_0\lvert w\rvert)$, so there is exactly one dimensionless combination the deviation can depend on:
\[\varepsilon \;=\; g\,r_L \;=\; |\nabla\ln B|\times(\text{Larmor radius}).\]The gradient seen across one orbit. Everything must be a function of $\varepsilon$ alone — in fact a theorem: rescaling lengths by $r_L$ turns the geodesic equations into a system that depends on $g$ and $w$ only through $\varepsilon$. So the content is the shape of that function, and its symmetry.
The result
Measured across sixteen $(g, w)$ pairs — which, by the $\varepsilon$-only reduction above, collapse onto seven distinct values of $\varepsilon$ (the plot shows those seven; different $(g,w)$ pairs sharing an $\varepsilon$ land on the same point, which is itself a check of the reduction) spanning nearly two decades:
\[\boxed{\;\delta(\varepsilon) \;=\; 1 - \tfrac{2}{\pi}\,K(2\varepsilon) \;=\; -\,\varepsilon^{2} \;-\; \tfrac{9}{4}\,\varepsilon^{4} \;-\; \tfrac{25}{4}\,\varepsilon^{6} \;-\;\cdots\;}\]with $K$ the complete elliptic integral of the first kind — an exact period-average law (its reading as the caustic’s law rides on the period identification below, verified to $6\times10^{-8}$ (worst relative gap) but formally open), found by a precision measurement (which pinned $c_4 = 2.2497 \pm 0.0009 = 9/4$ — conditional on fixing the proven leading coefficient $c_2 \equiv 1$; released, the fit drifts to $2.229$ — refuting the $5/2$ a coarser fit once suggested) and then derived: the angular dynamics integrates in one line, the per-angle refocusing time is identified with a pendulum-like period (an identification verified to $6\times10^{-8}$; its formal Jacobian step is the one open link — Appendix D5), and its launch-angle average is proven to be $\tfrac{2}{\pi}K(2\varepsilon)$ — modulus convention $K(k)$, $k = 2\varepsilon$, valid for $\varepsilon < \tfrac12$ — by an exact tangent-half-angle factorisation (Appendix D5), and verified against the geodesic code to $4\times10^{-9}$ or better ($\le 10^{-10}$ for $\varepsilon \le 0.25$). The coefficients are squared normalised central binomials, only even powers — and $K$’s singularity is physics: at the critical gradient $\varepsilon = 1/2$ the mean $\theta$-period diverges (that is the theorem; reading it as the mean refocusing time rides on the period identification above), and measured above it, the slowest launch directions show no conjugate point within the integration window — finite-horizon evidence (Appendix D5, and Part 7 for the full referee-grade chain). The figure shows $\lvert\delta\rvert$ against $\varepsilon$ on log–log: a clean line of slope 2. The complete proofs — the tangent-half-angle factorisation, the Gauss integral, and the precise statement of what remains conjectural — are written out in the companion article Growth Vectors and Caustics of Magnetic Flux Lifts, §3.
research/preferred-directions/artifacts/p1_results.json,
c4_precision.json.
What it says, physically
Three things, each checkable and each a little surprising.
The caustic measures the gradient, invertibly — for this profile class. From the deviation
of the refocusing pattern you recover the field gradient:
$\lvert\nabla\ln B\rvert = \lvert 1-\tfrac34\beta\rvert^{-1/2}\,\sqrt{\lvert\delta\rvert}/r_L$
to leading order, valid only for $\beta \ne \tfrac43$ — at $\beta = \tfrac43$ the
leading statistic is blind (tested — experiment F2 of the companion article’s §4, run_f2_beta43_blind.py) and this estimator is undefined. The profile
factor is $1$ exactly on exponential-class jets ($\beta = 0$),
which is the case this post measures. Follow-up work establishes that the leading coefficient is $1$ only for
exponential-class profiles. The caustic law is $c_2 = 1 - \tfrac34\beta$ with
$\beta = (\ln B)’’/\lvert(\ln B)’\rvert^2$ the dimensionless profile curvature at the
launch point — first measured (linear profile: $\tfrac74$, found $1.7466 \pm 0.0074$),
then derived by exact second-order perturbation of the caustic itself — while the
proven period-average law has $\tfrac12$ in place of $\tfrac34$: the two differ
because the conjugate-time = period identification fails off the exponential profile
(measured — this same experiment discovered it); on the exponential it agrees to
$6\times10^{-8}$ but remains a conjecture (the article’s Conjecture A, §3.4), not a theorem. So the inversion carries a
profile-calibration factor — and only that: at leading order every probe radius reads
the same single combination $(1-\tfrac34\beta)\lvert\nabla\ln B\rvert^2$, so gradient
and curvature are not separately recoverable from this statistic alone.
The derivations and the experiment are
the companion article’s §4.
A gradient delays refocusing — where $1-\tfrac34\beta > 0$ (the exponential class included; past $\beta = \tfrac43$ the derived leading-order effect flips to acceleration). $\delta<0$ means $t_c$ exceeds the Larmor period: orbits in a graded field take longer to refocus than in a uniform one. The gradient shears the family of orbits apart, and they need more time to come back together — at second order in the gradient.
Only even powers appear — proven to all orders on the exponential profile, at first order in general. On the exponential profile the closed form is a series in $\varepsilon^2$; for general one-dimensional profiles the first odd order provably averages away ($\tau_1 = 2\pi\sin\theta_0$ is odd — article Prop. 4.2), while the vanishing of higher odd orders remains open (open problem O6 in the article’s ledger, §7). The mechanism: a gradient points somewhere, and that directional (odd) part cancels when you average over all starting directions, leaving a signal that depends only on the gradient’s magnitude. Which is also the honest limitation: this averaged $\delta$ reads the one calibrated combination $(1-\tfrac34\beta)\lvert\nabla\ln B\rvert^2$ — on the exponential profile that is $\lvert\nabla\ln B\rvert^2$ alone — and not the gradient’s direction. The direction is in the $\theta_0$-dependence we averaged away — a readout still on the table.
Why this result matters beyond magnetism
The nilpotent-deviation statistic $\delta$ is not new here (this series uses the launch-angle average; the sibling program’s Appendix C6 introduced it as a $w$-average — same object, different marginal). It is the central object of the caustics-to-groups program, where it separated one abstract group from another. But there it was only ever checked against structures that program generated itself. This is the first time $\delta$ has been measured against an independently known target — an analytic field $B_0 e^{gx}$ whose gradient is fixed in advance rather than generated by the statistic’s own machinery (a constructed ground truth, not an observed one) — and it passed exactly, with a sharp coefficient and the predicted parity. A statistic invented to tell Lie groups apart turns out to read a magnetic field gradient.
Estimator limits
$\delta$ measures one profile-calibrated gradient combination at a smooth point. At magnetic nulls, the growth vector detects vanishing but does not identify the null type (Part 4). Whether the caustic invariant $\delta$ recovers that type remains an open estimator question. Parts 4 and 5 report the tested comparisons.
Glossary
- Nilpotent deviation $\delta$ — the fractional departure of the real refocusing time from the flat-model (Larmor) period, averaged over launch direction; zero for a uniform field.
- Larmor radius $r_L = 1/(B_0\lvert w\rvert)$ — the size of a Larmor orbit; the geometry’s one length scale.
- Dimensionless gradient $\varepsilon = \lvert\nabla\ln B\rvert\,r_L$ — the fractional change of the field across one orbit; the leading knob. General one-dimensional profiles also enter through the curvature $\beta = (\ln B)’’/[(\ln B)’]^2$ (the $1-\tfrac34\beta$ calibration) and, beyond leading order, higher jets.
- Parity — on the exponential profile $\delta$ is even in $\varepsilon$ (closed form); in general the first odd order provably cancels under the launch average, higher odd orders open (the article’s open problem O6).
References
- L. Sacchelli (2019). “Short geodesics losing optimality in contact sub-Riemannian manifolds and stability of the 5-dimensional caustic.” SIAM J. Control Optim. 57, 2362–2391. arXiv:1812.11340.
- A. Agrachev & D. Barilari (2012). “Sub-Riemannian structures on 3D Lie groups.” J. Dyn. Control Syst. 18, 21–44. arXiv:1007.4970.