{
  "abstract": "We establish a controlled, local, and quasi-stationary thermodynamic framework for neutral, nonrotating primordial black holes (PBHs) by combining a local residue prescription with the thermodynamicization of gravitational dynamics. For a nonextremal spherical horizon, we demonstrate that the positive residue of a meromorphic one-form directly determines the inverse Hawking temperature. Applying the first law of thermodynamics recovers the standard Schwarzschild temperature and Bekenstein-Hawking entropy under standard normalization. The resulting entropy defines an off-shell canonical exponent, which reveals that equilibrium thermal production of PBHs is exponentially suppressed in a radiation-dominated universe, thereby confirming that the standard density-perturbation collapse criterion remains the primary formation mechanism. For post-formation evolution, we adopt a detailed-balance mass law, prove the validity of the generalized second law of thermodynamics, and express the evolution dynamics as a free-energy gradient flow where the moving mass acts as an instantaneous evaporation-accretion threshold. Finally, we derive explicit first-order shifts for the temperature, entropy, thermal saddle, and nucleation exponent under small analytic deformations of the residue.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2611.07747",
  "author_total": 1,
  "authors": [
    {
      "name": "Wen-Xiang Chen"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/9pm4z29dw980j.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2611.07747",
  "fulltext_url": null,
  "id": "9pm4z29dw980j",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2611.07747",
  "language": null,
  "licence": "LicenseRef-arXiv-nonexclusive-1.0",
  "licence_label": "arXiv licence",
  "licence_source": "article",
  "licence_url": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "gr-qc"
    ]
  ],
  "openalex": null,
  "pdf_url": "https://arxiv.org/pdf/2611.07747",
  "pmcid": null,
  "pmid": null,
  "published": "2026-11-05",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/9pm4z29dw980j.ris",
  "sources": [
    {
      "first_seen": "2026-11-06T18:21:30Z",
      "native_id": "2611.07747",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2611.07747"
    }
  ],
  "subjects": [
    {
      "field": "physics",
      "origin": "arxiv:gr-qc",
      "subfield": "gravitation"
    }
  ],
  "title": "Gravitational Thermodynamicization of Primordial Black Holes: An RVB Residue Formulation of Thermal Formation and Nonequilibrium Evolution",
  "title_text": "Gravitational Thermodynamicization of Primordial Black Holes: An RVB Residue Formulation of Thermal Formation and Nonequilibrium Evolution",
  "type": "preprint",
  "updated_at": "2026-11-09T00:20:41Z",
  "url": "https://research.draconitic.com/paper/9pm4z29dw980j",
  "venue": "arXiv",
  "versions": []
}