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Bibliographic Details
Main Author: Vallejos, Omar Ariel
Format: Recurso digital
Language:English
Published: Zenodo 2025
Online Access:https://doi.org/10.5281/zenodo.17304825
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author Vallejos, Omar Ariel
author_facet Vallejos, Omar Ariel
contents <p>Problem: The $\Lambda$CDM model predicts smooth structure evolution from Gaussian initial conditions. Method: Bispectral analysis of velocity dispersion (VDISP) in 2.8M SDSS DR17 galaxies using open-source Rust/Python code. Finding: 77.3x increase in non-Gaussianity between $z\sim0.1$ and $z\sim0.7$, incompatible with $\Lambda$CDM. Interpretation: Signature of primordial vorticity in early cosmic plasma. Implication: Requires extension of $\Lambda$CDM with primordial vector fields.</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_17304825
institution Zenodo
language eng
publishDate 2025
publisher Zenodo
record_format zenodo
spellingShingle Strong Redshift Evolution of Non-Gaussian Vorticity in Galaxy Velocity Fields: Bispectral Evidence for Beyond-ΛCDM Physics from 2.8M SDSS Galaxies
Vallejos, Omar Ariel
<p>Problem: The $\Lambda$CDM model predicts smooth structure evolution from Gaussian initial conditions. Method: Bispectral analysis of velocity dispersion (VDISP) in 2.8M SDSS DR17 galaxies using open-source Rust/Python code. Finding: 77.3x increase in non-Gaussianity between $z\sim0.1$ and $z\sim0.7$, incompatible with $\Lambda$CDM. Interpretation: Signature of primordial vorticity in early cosmic plasma. Implication: Requires extension of $\Lambda$CDM with primordial vector fields.</p>
title Strong Redshift Evolution of Non-Gaussian Vorticity in Galaxy Velocity Fields: Bispectral Evidence for Beyond-ΛCDM Physics from 2.8M SDSS Galaxies
url https://doi.org/10.5281/zenodo.17304825