{
  "annotation_id": "df6b294c-bae9-4866-a5d9-7692d081b7e1",
  "date_created": "2026-03-02T18:00:39.547000Z",
  "date_modified": "2026-03-02T18:00:39.547000Z",
  "file_hash": "7909e2e54129b08fca2273997f72576633a26c8559f6884491d1b068340eb7a3",
  "private": false,
  "record": {
    "abstract": "We propose an effective harmonic oscillator model in order to treat the\nfluctuations of the gravitational, strong and weak nuclear fields. With respect\nto the gravitational field, first we use the model to estimate its fluctuating\nstrength, necessary to decohere the wavefunction of a cubic centimeter of air\nat the standard temperature and pressure conditions. Second, the fluctuation of\na point mass through a distance equal to the Planck length leads to the\nself-gravitational interaction of a particle, which can be related to its de\nBroglie frequency. Third, by making the equality of the fluctuating field\nstrength with the gravitational field of a mass M at half of its Schwarzschild\nradius, we obtain an estimate of the mass of the Universe. We also consider the\nfluctuations of the strong nuclear field, as a means to estimate the separation\nin energy between the ground state and the centroid of the excitated states of\nthe nucleon. Finally, taking into account the neutron-proton mass difference,\nwe use the fluctuations of the weak nuclear field in order to evaluate the weak\ncoupling constant.",
    "arxiv_id": "physics/0112023",
    "authors": [
      "P. R. Silva"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "title": "Fluctuations in the Gravitational, Strong and Weak Nuclear Fields   through an Effective Harmonic Oscillator Model",
    "url": "https://arxiv.org/abs/physics/0112023"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "655d0aac-f3ac-484c-9fba-6c200dbbb944",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}