{
  "annotation_id": "643182a7-2dcc-4b31-9d79-03513b97a221",
  "date_created": "2026-02-17T05:53:11.672000Z",
  "date_modified": "2026-02-17T05:53:11.672000Z",
  "file_hash": "d37797838a8f39e17d0032cac990bb0db4b799ffd4d2399a3a25730975ef75fd",
  "private": false,
  "record": {
    "abstract": "For generic theories of nonlinear electrodynamics (NLED) we investigate the restrictions imposed by causality on spherically-symmetric charged black-hole solutions of the Einstein-NLED equations. For a large class of (acausal) Born-type NLED theories, we find that the Reissner-Nordstrom (RN) metric is an exact, but unstable, solution for some dyonic black holes. For all causal NLED we show that there are no regular black holes, and that the entropy of extremal black holes is less than the RN entropy for fixed charge. We also find the conditions for a parameter-space transition between RN-type and Schwarzschild-type global structure. For the transition from Schwarzschild-type to naked singularity, which occurs at finite mass, we show that the metric at the transition point is a Barriola-Vilenkin global monopole.",
    "arxiv_id": "2601.07789",
    "authors": [
      "Jorge G. Russo",
      "Paul K. Townsend"
    ],
    "categories": [
      "hep-th",
      "gr-qc"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "Black holes and causal nonlinear electrodynamics",
    "url": "https://arxiv.org/abs/2601.07789",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "640699cf-9026-4fc9-8cfb-d5c4da285085",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}