{
  "annotation_id": "4437115d-034a-45bf-ba7f-e49004bfbbe2",
  "date_created": "2026-03-02T18:00:05.096000Z",
  "date_modified": "2026-03-02T18:00:05.096000Z",
  "file_hash": "554af677e7cb131d09967adf5ca9733413b906768427ba143e623b0ada8fa3d8",
  "private": false,
  "record": {
    "abstract": "We search for non-trivial relativistic solutions of the hydrodynamic\nequations with quasi-inertial flows such as in the Bjorken-like models. The\nproblem is analyzed in general and the known results are reproduced by a method\nproposed. A new class of 3D anisotropic analytic solutions with quasi-inertial\nproperty is found. An ellipsoidal generalization of the spherically symmetric\nHubble flow with constant pressure is proposed as a particular case. The\nrelativistic expansion of finite systems into vacuum is also described within\nthis class. A region of applicability and possible utilization of the new\nsolutions for processes of A+A collisions is discussed.",
    "arxiv_id": "nucl-th/0505041",
    "authors": [
      "Yu. M. Sinyukov",
      "Iu. A. Karpenko"
    ],
    "categories": [
      "nucl-th",
      "hep-ph",
      "nucl-ex"
    ],
    "title": "Quasi-inertial ellipsoidal flows in relativistic hydrodynamics",
    "url": "https://arxiv.org/abs/nucl-th/0505041"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c3e1ebff-bd74-41eb-9f7f-1fe8e9b8c245",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}