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 $10^{-8}$ 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 $10^{-8}$; 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 $10^{-10}$. 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: F2) and this estimator is undefined. The profile factor is $1$ exactly on exponential-class jets ($\beta = 0$), which is the case this post measures. The shape of a caustic is not decoration — it is a readout. One honest qualifier, established by follow-up work: 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 $10^{-8}$ but remains Conjecture A, 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 (O6). 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.
The honest edge
$\delta$ reads one profile-calibrated gradient combination at a smooth point. The real prize is at the nulls, where the field vanishes and the interesting plasma physics happens. The growth vector detects those nulls but cannot tell their type (Part 4). The open question — the one that decides whether this whole framing refines the standard tools or merely agrees with them — is whether a caustic invariant like $\delta$ recovers the null type. Part 4 sets that question up honestly and does not oversell the answer.
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 (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.