No Neutron Stars: Black Holes, Pulsars, and Gap Objects as Almost-Perfect All:All Entanglement Graphs
Computational companion to a phenomenological model in which black hole interiors are almost-perfect all:all entanglement graphs, horizon area counts exterior legs (A = 4ln2 k lp^2), and micro-holes undergo a point-to-horizon phase transition. v4.1 (BV scale-up): UV tortuosity-as-scattering derived from ln2 (c = 0.44-0.60, p = 2c); N = 4000/8000/16000 campaigns hold p = 0.93/0.94/0.91 with measured UV turnover; exact shell distance oracle + torch backend; beta(N) log-linear over 6 points. v4.0 (No Neutron Stars): pulsars, gap objects, and black holes unified as low-k graphs; J0737 2PN measured p = 0.913+-0.049 (80 graphs N=1020 exact, 0.1 sigma); leg-shedding kilonovae with a falsifiable gap prediction and O5 protocol. Includes reproducible simulations (Secs 1-3 + Appendices A-BS + BU, BV), paper drafts (Markdown + LaTeX/PDF), figures, tests, and an interactive demo. Code MIT, text/figures CC BY 4.0.
Authors
- Philippe Leblond
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-09-26
- DOI
- https://doi.org/10.5281/zenodo.22983418
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 0.00