Two Parameter-Free Predictions of the U-Cell Model: A Multi-Scale Consistency Test and the Two Characteristic Halo Radii

Fuente: Zenodo
Salvato in:
Dettagli Bibliografici
Autore principale: Prebeck, Norbert
Natura: Recurso digital
Lingua:inglese
Pubblicazione: Zenodo 2026
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866901228076662784
author Prebeck, Norbert
author_facet Prebeck, Norbert
contents <p>The U-Cell Model (UCM) derives gravity, dark matter, and cosmological expansion from a single substrate dispersion relation without free parameters. This record contains two companion papers. Paper 1 compiles four independent parameter-free UCM predictions — rotation curves (median chi²=0.73 for 150 SPARC galaxies), the MDAR acceleration scale (0.5% agreement with McGaugh et al. 2016), the local dark matter density (0.1 sigma from Gaia/PDG), and the Milky Way virial radius (5% agreement with Gaia satellite kinematics) — all controlled by the single constant f_cold = sqrt(2-pi/2). Paper 2 derives two physically distinct characteristic radii for every UCM halo: r_200 (the conventional virial radius) and r_virial (the Euler junction radius), with a universal ratio r_virial/r_200 = f_cold*sqrt(150) ≈ 8.02 independent of galaxy mass. Between these radii the halo maintains an isothermal r^{-2} profile containing 88% of the total halo mass, producing a weak-lensing excess relative to NFW at r > r_200. Both results are directly testable with Euclid DR1 (October 2026).</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_19389292
institution Zenodo
language eng
publishDate 2026
publisher Zenodo
record_format zenodo
spellingShingle Two Parameter-Free Predictions of the U-Cell Model: A Multi-Scale Consistency Test and the Two Characteristic Halo Radii
Prebeck, Norbert
dark matter
isothermal halo
virial radius
U-Cell Model
MDAR
SPARC
rotation curves
weak lensing
Euclid
f_cold
parameter-free prediction
<p>The U-Cell Model (UCM) derives gravity, dark matter, and cosmological expansion from a single substrate dispersion relation without free parameters. This record contains two companion papers. Paper 1 compiles four independent parameter-free UCM predictions — rotation curves (median chi²=0.73 for 150 SPARC galaxies), the MDAR acceleration scale (0.5% agreement with McGaugh et al. 2016), the local dark matter density (0.1 sigma from Gaia/PDG), and the Milky Way virial radius (5% agreement with Gaia satellite kinematics) — all controlled by the single constant f_cold = sqrt(2-pi/2). Paper 2 derives two physically distinct characteristic radii for every UCM halo: r_200 (the conventional virial radius) and r_virial (the Euler junction radius), with a universal ratio r_virial/r_200 = f_cold*sqrt(150) ≈ 8.02 independent of galaxy mass. Between these radii the halo maintains an isothermal r^{-2} profile containing 88% of the total halo mass, producing a weak-lensing excess relative to NFW at r > r_200. Both results are directly testable with Euclid DR1 (October 2026).</p>
title Two Parameter-Free Predictions of the U-Cell Model: A Multi-Scale Consistency Test and the Two Characteristic Halo Radii
topic dark matter
isothermal halo
virial radius
U-Cell Model
MDAR
SPARC
rotation curves
weak lensing
Euclid
f_cold
parameter-free prediction
url https://doi.org/10.5281/zenodo.19389292