{
  "annotation_id": "09b814e2-b39a-4711-9e04-4ddfc4c59942",
  "date_created": "2026-03-02T18:02:16.427000Z",
  "date_modified": "2026-03-02T18:02:16.427000Z",
  "file_hash": "34bd5ce2f00000f7ccb66dd5b191ecf08cd617c8675dbc17f081402f08157124",
  "private": false,
  "record": {
    "abstract": "Stochastic backgrounds of gravitational waves are intrinsic fluctuations of\nspacetime which lead to an unavoidable decoherence mechanism. This mechanism\nmanifests itself as a degradation of the contrast of quantum interferences. It\ndefines an ultimate decoherence border for matter-wave interferometry using\nlarger and larger molecules. We give a quantitative characterization of this\nborder in terms of figures involving the gravitational environment as well as\nthe sensitivity of the interferometer to gravitational waves. The known level\nof gravitational noise determines the maximal size of the molecular probe for\nwhich interferences may remain observable. We discuss the relevance of this\nresult in the context of ongoing progresses towards more and more sensitive\nmatter-wave interferometry.",
    "arxiv_id": "quant-ph/0505074",
    "authors": [
      "Brahim Lamine",
      "R\u00e9my Herv\u00e9",
      "Astrid Lambrecht",
      "Serge Reynaud"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1103/PhysRevLett.96.050405",
    "journal_ref": "Physical Review Letters 96 (2006) 050405",
    "title": "Ultimate decoherence border for matter-wave interferometry",
    "url": "https://arxiv.org/abs/quant-ph/0505074"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b5140729-cfb9-4f4e-b153-ea9fe9f02e48",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}