{
  "annotation_id": "f5bb132b-314e-4f65-ac5c-46ae17b5572b",
  "date_created": "2026-03-02T18:01:44.868000Z",
  "date_modified": "2026-03-02T18:01:44.868000Z",
  "file_hash": "d4acdcb598853340ab5f6b64f38be3ddddecbd32ea4f0cab640dae1160d0f1b7",
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  "record": {
    "abstract": "We study the fermionic vacuum energy of vacua with and without being applied\nan external magnetic field. The energetic difference of two vacua leads to the\nvacuum decaying and the vacuum-energy releasing. In the context of quantum\nfield theories, we discuss why and how the vacuum energy can be released by\nspontaneous photon emissions and/or paramagnetically screening the external\nmagnetic field. In addition, we quantitatively compute the vacuum energy\nreleased, the paramagnetic screening effect and the rate and spectrum of\nspontaneous photon emissions. The possibilities of experimentally detecting\nsuch an effect of vacuum-energy releasing and this effect accounting for the\nanormalous X-ray pulsar are discussed.",
    "arxiv_id": "quant-ph/0106076",
    "authors": [
      "She-Sheng Xue"
    ],
    "categories": [
      "quant-ph",
      "astro-ph",
      "hep-ex",
      "hep-ph",
      "hep-th"
    ],
    "doi": "10.1103/PhysRevD.68.013004",
    "journal_ref": "Phys.Rev. D68 (2003) 013004",
    "title": "Magnetically induced vacuum decay",
    "url": "https://arxiv.org/abs/quant-ph/0106076"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f7d362d4-6672-479b-855b-7ab6addb8861",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}