Explores dark matter interactions in a physical model, suggesting a new candidate for dark matter.
The nature of dark matter remains unknown after four decades of increasingly sensitive searches. Weakly Interacting Massive Particles (WIMPs) are excluded over most of their natural parameter space; axions remain undetected; the conventional smooth‑halo picture is demonstrably wrong at the scale of our own solar neighborhood. We present the neutral chaoiton — a stable, time‑periodic, localized l=1 soliton of the Ouroboros Lagrangian — as a concrete, falsifiable dark matter candidate requiring no new free parameters. The model also predicts J‑field wave components of light mass and bosonic character, behaving like photons; the empirical data point to a mix of both aspects. The Ouroboros Lagrangian (Werbos 2026, Paper I) is a superrenormalizable classical field theory whose soliton solutions follow from the classical equations of motion, independently of the quantization. The neutral chaoiton has mass m_χ = 0.460 MeV and J‑field mediator mass m_J = 0.618 MeV. Its l=1 angular structure forces the zero‑momentum electromagnetic coupling to vanish by an exact angular‑momentum selection rule; the leading dipole interaction gives a chaoiton–proton cross‑section σ_p = 9×10⁻⁴¹ cm², eleven orders of magnitude below LZ CRBDM limits. The self‑interaction is likewise dipole‑suppressed to ∼10⁻⁶ cm²/g, compatible with the Bullet Cluster bound, so chaoitons can constitute 100 % of dark matter. The two‑component picture (chaoitons + J‑field waves) remains a physically natural possibility whose local manifestation can be probed by the six‑peak annual modulation from Gaia Dark Shards, providing a falsifiable signature for a dedicated J‑field sensor.
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Paul Werbos (2026) studied this question.
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