{
  "annotation_id": "359e5be2-59e2-4d54-aca4-1c2d3af45e1f",
  "date_created": "2026-03-02T18:00:04.860000Z",
  "date_modified": "2026-03-02T18:00:04.860000Z",
  "file_hash": "39f0de6ee0db9c18669e1e830444a65ae9143ce77092d40dada335604a7d8c3d",
  "private": false,
  "record": {
    "abstract": "The quantitative impact of the requirement of relativistic invariance in the\nthree-nucleon problem is examined within the framework of Poincar\\\u0027e invariant\nquantum mechanics. In the case of the bound state, and for a wide variety of\nmodel implementations and reasonable interactions, most of the quantitative\neffects come from kinematic factors that can easily be incorporated within a\nnon-relativistic momentum-space three-body code.",
    "arxiv_id": "nucl-th/0508001",
    "authors": [
      "B. D. Keister",
      "W. N. Polyzou"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.73.014005",
    "journal_ref": "Phys.Rev. C73 (2006) 014005",
    "title": "Quantitative Relativistic Effects in the Three-Nucleon Problem",
    "url": "https://arxiv.org/abs/nucl-th/0508001"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "fce6c9af-db41-42b8-bd47-c90011b40dda",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}