{
  "annotation_id": "e8dd5447-85ad-4633-a3a6-8b8b5dc37513",
  "date_created": "2026-03-02T18:01:17.961000Z",
  "date_modified": "2026-03-02T18:01:17.961000Z",
  "file_hash": "c51144a43949b0bac88366111c71aae3293eb817f64945a84063cb0f89e453aa",
  "private": false,
  "record": {
    "abstract": "When a strong magnetostatic field is present, vacuum effectively appears as a\nlinear, uniaxial, dielectric-magnetic medium for small-magnitude optical\nfields. The availability of the frequency-domain dyadic Green function when the\nmagnetostatic field is spatially uniform facilitates the formulation of an\nintegral equation for the scattering of an optical field by a spatially varying\nmagnetostatic field in vacuum. This integral equation can be numerically\ntreated by using the method of moments as well as the coupled dipole method.\nFurthermore, the principle underlying the strong-property-fluctuation theory\nallows the homogenization of a spatially varying magnetostatic field in the\ncontext of light scattering.",
    "arxiv_id": "physics/0702175",
    "authors": [
      "Akhlesh Lakhtakia",
      "Tom G. Mackay"
    ],
    "categories": [
      "physics.optics"
    ],
    "doi": "10.1080/02726340701492554",
    "journal_ref": "Electromagnetics, Vol. 27, pp. 341-354 (2007)",
    "title": "Integral Equation for Scattering of Light by a Strong Magnetostatic   Field in Vacuum",
    "url": "https://arxiv.org/abs/physics/0702175"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "65042e0b-ea6e-4070-a77e-4406fff51a0e",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}