{
  "annotation_id": "f59a1818-338f-4142-878f-93fe5b67725e",
  "date_created": "2026-02-17T05:53:12.590000Z",
  "date_modified": "2026-02-17T05:53:12.590000Z",
  "file_hash": "042ee8c8a78f451902bfd2b5e6b0fb75691402feee54b36fcf035ff7a03eaa65",
  "private": false,
  "record": {
    "abstract": "In scenarios where the Peccei-Quinn symmetry breaks after inflation, small-scale axion inhomogeneities may gravitationally collapse into bound structures. The evolution of these systems is typically modeled through cosmological perturbation theory applied to the Einstein-Klein-Gordon equations. In the non-relativistic regime, this framework reduces to the Gross-Pitaevskii-Poisson or Schr\\\"odinger-Poisson equations, depending on whether axion self-interactions are taken into account. In this work, a non-minimal gravitational coupling term $\\xi R \\phi^4$ is included into the axion\u0027s relativistic action as a way to introduce a gravitationally mediated pairwise interaction. By performing a perturbative expansion and subsequently taking the non-relativistic limit, an alternative set of equations that govern the early stages of structure formation is obtained.",
    "arxiv_id": "2601.07420",
    "authors": [
      "Bryan Cordero-Patino",
      "\u00c1lvaro Duenas-Vidal",
      "Jorge Segovia"
    ],
    "categories": [
      "hep-ph",
      "gr-qc",
      "hep-ex",
      "hep-th"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "Gross-Pitaevskii-Poisson equations with a $\\xi R \\phi^4$ non-minimal coupling term",
    "url": "https://arxiv.org/abs/2601.07420",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "fdf5d1b5-368e-46c0-9c1a-98c369c5ae7b",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}