Redshift Evolution and Non-Universal Dispersion of Quasar Luminosity Correlation
Zhuoyang Li, Lu Huang, Junchao Wang

TL;DR
This study investigates the deviation of quasar and supernova data from the standard cosmological model, attributing the discrepancy to redshift evolution and non-universal dispersion in quasar luminosity correlations rather than new physics.
Contribution
It demonstrates that redshift-dependent effects and intrinsic dispersion in quasar luminosity correlations explain the observed deviations from the $ ext{Lambda}$CDM model.
Findings
Significant tension between SNe+QSOs constraints and $ ext{Lambda}$CDM in PAge space.
Detected $ ext{2.7}\sigma$ and $ ext{4}\sigma$ tensions in correlation coefficient $oldsymbol{\gamma}$.
Intrinsic dispersion $oldsymbol{\delta}$ shows $>4 \sigma$ differences across data sets.
Abstract
The standard CDM model is recently reported to deviate from the high-redshift Hubble diagram of type Ia supernovae (SNe) and quasars (QSOs) at confidence level. In this work, we combine the PAge approximation (a nearly model-independent parameterization) and a high-quality QSO sample to search for the origins of the deviation. By visualizing the CDM model and the marginalized constraints of SNe+QSOs into PAge space, we confirm that the SNe+QSOs constraints in both flat and non-flat PAge cases are in remarkable tension with the standard CDM cosmology. Next, we investigate the tension from the perspective of redshift-evolution effects. We find that the QSO correlation coefficient calibrated by SNe+low-z QSOs and SNe+high-z QSOs shows and tensions in flat and non-flat universes, respectively. The…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Galaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories
