{
  "annotation_id": "d1b19ab3-8637-4ff0-8306-60d44887bfdb",
  "date_created": "2026-02-17T05:53:24.049000Z",
  "date_modified": "2026-02-17T05:53:24.049000Z",
  "file_hash": "a6bd2aae4f46724c000be6739f37a19633eee8678662b940efdd53f30a9f77b4",
  "private": false,
  "record": {
    "abstract": "Motivated by axion-like inflation and its warm embedding within the Standard Model, we study the early stages of the energy transfer between an axion condensate and an SU(2) gauge ensemble, by employing non-linear classical real-time lattice simulations. The discretized equations of motion are worked out, elaborating on Gauss constraints. A numerical solution is implemented on the CosmoLattice platform. Adopting a quadratic potential, and omitting universe expansion for the moment, we establish initial exponential growth of the low-momentum gauge modes; damping of axion oscillations after some delay; and subsequent energy equipartition between axion and gauge ensembles. A clear difference between the SU(2) and U(1) dynamics is observed, likely associated with non-Abelian self-interactions. We elaborate on what this implies for the possible thermalization of the SU(2) ensemble.",
    "arxiv_id": "2601.09784",
    "authors": [
      "Kim V. Berghaus",
      "Adrien Florio",
      "M. Laine",
      "Franz R. Sattler"
    ],
    "categories": [
      "hep-ph",
      "astro-ph.CO",
      "hep-lat"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "Classical equipartition dynamics between axions and non-Abelian gauge fields",
    "url": "https://arxiv.org/abs/2601.09784",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "96091b68-cf74-493b-a6e3-7c7bd52e9639",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}