CoreLumen Observational Series VI-A : Full Multi-Probe Cosmological Test

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1. Verfasser: Hwang, Jaegue
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Veröffentlicht: Zenodo 2026
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author Hwang, Jaegue
author_facet Hwang, Jaegue
contents <p>COS VI-A presents the first full multi-probe cosmological test of the CoreLumen late-time growth deformation framework.</p> <p>The analysis combines BAO, RSD, Planck prior information, CMB lensing, and weak-lensing constraints within a unified covariance-aware likelihood pipeline.</p> <p>The late-time growth sector is parameterized through a minimal deformation parameter p1 modifying the scalar gravitational response while leaving the background expansion history in the flat ΛCDM form.</p> <p>The likelihood is evaluated in the parameter space (p1, σ8, Ωm), allowing the degeneracy structure between growth deformation and clustering amplitude to be analyzed.</p> <p>The results show that the ΛCDM limit (p1 = 0) remains consistent with the current multi-probe data within observational uncertainties.</p> <p>This document is released in Zenodo archival mode to establish a transparent and reproducible record of the first multi-probe observational confrontation of the CoreLumen growth deformation framework.</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_18997461
institution Zenodo
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publishDate 2026
publisher Zenodo
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spellingShingle CoreLumen Observational Series VI-A : Full Multi-Probe Cosmological Test
Hwang, Jaegue
cosmology
large scale structure
modified gravity
growth of structure
BAO
RSD
weak lensing
multi-probe cosmology
CoreLumen
ΛCDM
CMB lensing
weak lensing
<p>COS VI-A presents the first full multi-probe cosmological test of the CoreLumen late-time growth deformation framework.</p> <p>The analysis combines BAO, RSD, Planck prior information, CMB lensing, and weak-lensing constraints within a unified covariance-aware likelihood pipeline.</p> <p>The late-time growth sector is parameterized through a minimal deformation parameter p1 modifying the scalar gravitational response while leaving the background expansion history in the flat ΛCDM form.</p> <p>The likelihood is evaluated in the parameter space (p1, σ8, Ωm), allowing the degeneracy structure between growth deformation and clustering amplitude to be analyzed.</p> <p>The results show that the ΛCDM limit (p1 = 0) remains consistent with the current multi-probe data within observational uncertainties.</p> <p>This document is released in Zenodo archival mode to establish a transparent and reproducible record of the first multi-probe observational confrontation of the CoreLumen growth deformation framework.</p>
title CoreLumen Observational Series VI-A : Full Multi-Probe Cosmological Test
topic cosmology
large scale structure
modified gravity
growth of structure
BAO
RSD
weak lensing
multi-probe cosmology
CoreLumen
ΛCDM
CMB lensing
weak lensing
url https://doi.org/10.5281/zenodo.18997461