A Cold-Remnant Temperature Law: Where the Specific Heat of an Evaporating Hole Changes Sign
The turnover sits at 1.500e+11 kilograms by the analytic route and 1.499e+11 kilograms by the numerical scan, agreement at the quoted precision. The maximum temperature is 5.454e+11 kelvin. At ten remnant masses the model gives 1.403e+11 kelvin against the uncorrected Hawking value 1.417e+11 kelvin, a one-percent correction, so the law is invisible until the end-stage and decisive only there, exactly the behaviour a candidate endpoint law should have. Below the turnover mass the specific heat is positive: losing mass lowers the temperature, evaporation throttles itself, and the approach to the remnant is asymptotic and gentle rather than explosive. Computed from stated assumptions, not measured.
Authors
- William Alexander Aldred (ORCID: https://orcid.org/0009-0000-1215-577X)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-11-11
- DOI
- https://doi.org/10.5281/zenodo.24125687
- Primary Topic
- Black Holes and Theoretical Physics
- Type
- article
- Field-Weighted Citation Impact
- 0.00