{
  "annotation_id": "0db89471-8515-4e6d-b7d0-03d9bae839f6",
  "date_created": "2026-03-02T18:00:28.757000Z",
  "date_modified": "2026-03-02T18:00:28.757000Z",
  "file_hash": "7dd26d4e7b2b0da9b2d2f83323cc2661303e2da71634e203ff976cb6f177dd72",
  "private": false,
  "record": {
    "abstract": "We reexamine the derivation of relativistic transport equations for fermions\nwhen conserving the most general spinor structure of the interaction and Green\nfunction. Such an extension of the formalism is needed when dealing with {\\it\ne.g.} spin-polarized nuclear matter or non-parity conserving interactions. It\nis shown that some earlier derivations can lead to an incomplete description of\nthe evolution of the system even in the case of parity-conserving,\nspin-saturated systems. The concepts of kinetic equation and mass shell\ncondition have to be extended, in particular both of them acquire a non trivial\nspinor structure which describe a rich polarization dynamics.",
    "arxiv_id": "nucl-th/9909073",
    "authors": [
      "L. Mornas",
      "K. Morawetz"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1142/9789812793812_0027",
    "title": "Relativistic transport equations with generalized mass shell constraints",
    "url": "https://arxiv.org/abs/nucl-th/9909073"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "65fbe605-6cef-4dde-9364-dc9dfbd9dd6b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}