TQNT-V5.19 — Compact stellar/dark objects catalog: dark matter pearls + 5 additional classes from V5 principles, with JWST high-z contribution audit

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Authors: Lilian Cariou
Cited by: 10
References: 1

Abstract

Catalog of 6 classes of compact objects derivable from TQNT-V5 principles: (A) DM Pearls [ref dm_pearls v2, 10.5281/zenodo.20559268], (B) Topological PBH seeds from Vassiliev-suppressed heavy proton clustering, (C) Knot-Baryon Hybrid Stars, (D) Heavy proton plasma BBN-transient, (E) Strange Knot Stars (6 STRICT V5 amphichirals), (F) Primordial unknot defects (V5.17 cascade analogs). For each class: typical mass scale, primordial abundance, JWST observational signature. Confrontation with JWST 'impossible early galaxies' SMF residual (post Krishnan+Abazajian 2026 audit): V5 compact objects do NOT explain the residual SMF (gap +5 to +25 dex). But they remain valuable for: AGN seeding (Class B), DM sub-population (A, E), microlensing (A), IMBH population (F), BBN primordial abundance tests (D). Validation: 25/25 pytest tests passing. Part of the TQNT-V5 monograph (10.5281/zenodo.19131538); complements V5.7 v1.4 (10.5281/zenodo.20674849); references DM pearls v2 (10.5281/zenodo.20559268).

Fields of Study & Subjects

Galaxies: Formation Evolution Phenomena Astronomy and Astrophysical Research Dark Matter and Cosmic Phenomena

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
15 June 2026
Language
EN
Document type
Preprint