{
  "annotation_id": "c8e9dc1e-1045-4597-bee7-b2aff6f3715a",
  "date_created": "2026-03-02T18:01:24.167000Z",
  "date_modified": "2026-03-02T18:01:24.167000Z",
  "file_hash": "2c8d6379a345026a4a1e497342b5f108b7637586922ff34e68aebacdf437432c",
  "private": false,
  "record": {
    "abstract": "The thermal noise is expected to be one of the main limiting factors on the\nsensitivity of interferometric gravitational-wave detectors like LIGO and\nVIRGO. Thermal fluctuations of internal modes of the interferometer\u0027s test\nmasses and of suspension modes will dominate the noise spectrum at the\nimportant frequency range between 50 and 200 Hz. It is assumed that losses in\nthe test masses and suspensions will occur mainly due to internal friction in\ntheir materials, which is related to anelasticity effects in solids. The\npresent notes comprise some basic results on the theory of anelasticity and\nthermal noise in pendulum suspensions. This collection is by no means complete\nand focus on aspects which are of interest for the author.",
    "arxiv_id": "physics/9909014",
    "authors": [
      "Constantin Brif"
    ],
    "categories": [
      "physics.ins-det",
      "gr-qc",
      "physics.gen-ph"
    ],
    "title": "Notes on anelastic effects and thermal noise in suspensions of test   masses in interferometric gravitational-wave detectors",
    "url": "https://arxiv.org/abs/physics/9909014"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "27a5f897-44f9-45e8-8bb7-0f3c441543ad",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}