Orbital Jerk Exposure and Shell Width Universality: A First-Principles Account of the Density–Anisotropy Relation

Numerical simulations of collisionless dark matter halos reveal a persistent correlation between the local density slope and velocity anisotropy of particle orbits. Although widely reproduced, the physical origin of this density–anisotropy relation remains uncertain. Orbital Jerk Exposure and Shell Width Universality: A First-Principles Account of the Density–Anisotropy Relation This paper proposes a structural interpretation of the dark matter halo density–anisotropy relation within the Emergent Reality Architecture (ERA) framework. Numerical simulations consistently show that halos populate a restricted band in the parameter space defined by the logarithmic density slope (γ) and the velocity anisotropy parameter (β). Despite its robustness across cosmological simulations, the underlying mechanism producing this relation remains unclear. This paper proposes a structural explanation for the dark matter halo density–anisotropy relation based on a finite orbital complexity threshold applied to gravitational jerk exposure along particle trajectories. The jerk exposure measure and threshold condition stand on their own dynamical footing; the Emergent Reality Architecture (ERA) framework provides interpretive context for why such a threshold should exist and why its normalization should be universal. The paper introduces a measure of orbital complexity based on the time-averaged gravitational jerk exposure experienced along particle trajectories. Evaluating this quantity for particle orbits in spherical halos reveals that the complexity of a trajectory depends primarily on how deeply the orbit penetrates into the halo’s gravitational gradient field. Radial orbits that plunge toward the halo center experience rapidly increasing gradient exposure and therefore impose larger configurational demands. Extending this calculation to an ensemble of halo orbits shows that the aggregate orbital complexity depends on the distribution of low-angular-momentum trajectories within the system. Imposing a finite complexity threshold produces a structural accessibility boundary in the (γ, β) plane that links the halo density slope to the allowable orbital anisotropy. The resulting prediction defines a family of curves describing the maximum anisotropy accessible to halos with a given density slope. For parameter values consistent with cosmological simulations, the predicted slopes reproduce the sign and approximate magnitude of the empirically observed density–anisotropy relation. This interpretation suggests that the density–anisotropy relation reflects a structural constraint on accessible orbital configurations rather than solely the outcome of dynamical relaxation processes. In this view, halo structure emerges from the requirement that collisionless systems remain below a threshold of sustainable orbital complexity. The paper concludes with direct particle-level verification across all five Aquarius level-2 halos using 170–192 million particles each, confirming the geometric shell width ln λ ∈ 0.103, 0.127 across six systems spanning four orders of magnitude in mass, with the curvature tensor derivation reproducing these values to sub-0.45% accuracy. Related work: This paper builds on the Emergent Reality Architecture (ERA) framework developed in Emergent Reality Architecture: A Unified Structural Account of Physical Law from Quantum Mechanics to Cosmological Expansion (Zenodo). ERA proposes a layered structural interpretation of physical regimes in which quantum behavior, null propagation, and gravitation arise from representational constraints rather than independent dynamical mechanisms. The present work applies this framework to the phase-space structure of collisionless dark matter halos. A complementary interpretation of dark matter phenomenology is developed in Representational Limits and Dark Matter: Spatial Suppression and Halo Structure, which explores how structural restrictions on localization pathways may explain the extended halo configurations observed in cosmological structure formation. Additional conceptual clarifications within general relativity appear in Orbits as Inertial States: Rethinking Rest in General Relativity and Geodesics as Regimes of Persistence. Together these works examine how persistence, ordering, and metric structure emerge across different physical regimes. Revision notes (Version 8.1): Title updated: Retitled to "Orbital Jerk Exposure and Shell Width Universality: A First-Principles Account of the Density–Anisotropy Relation" to foreground the astrophysical mechanism and central empirical result. Physics-forward reframing: ERA repositioned as interpretive context rather than causal driver. The jerk exposure measure and threshold condition are explicitly stated to stand on their own dynamical footing independently of ERA. "ERA accessibility boundary" replaced with "jerk-exposure boundary" throughout. Falsifiability conditions added (Section 2): Three specific conditions that would rule out the framework are now stated explicitly: systematic variation of ln λ with halo mass or formation history; failure of the χMD decomposition to separate geometric and anisotropy contributions; or violation of the shell-bracketing condition rmin < rs < rmax in cusped halos. M–σ subsection removed: The black hole structural parallel subsection has been removed to keep the paper focused on collisionless halo structure. This material is developed in the ERA framework paper. Abstract and conclusion updated: ERA language minimized; Aquarius results and curvature tensor result foregrounded as the central empirical and geometric claims. Correspondence: Peter Nowicki — peternowicki@proton.me