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arXiv · 2210.02816

Redshift Evolution and Non-Universal Dispersion of Quasar Luminosity Correlation

Zhuoyang Li·Lu Huang·Junchao Wang
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Abstract

The standard $Λ$CDM model is recently reported to deviate from the high-redshift Hubble diagram of type Ia supernovae (SNe) and quasars (QSOs) at $\sim4σ$ 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 $Λ$CDM model and the marginalized $3σ$ 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 $Λ$CDM cosmology. Next, we investigate the tension from the perspective of redshift-evolution effects. We find that the QSO correlation coefficient $γ$ calibrated by SNe+low-z QSOs and SNe+high-z QSOs shows $\sim2.7σ$ and $\sim4σ$ tensions in flat and non-flat universes, respectively. The tensions for intrinsic dispersion $δ$ between different data sets are found to be $>4σ$ in both flat and non-flat cases. These results indicate that the QSO luminosity correlation suffers from significant redshift evolution and non-universal intrinsic dispersion. Using a redshift-dependence correlation to build QSO Hubble diagram could lead to biases. Thus, the $\sim4σ$ deviation from the standard $Λ$CDM probably originates from the redshift-evolution effects and non-universal dispersion of the QSO luminosity correlation rather than new physics.

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Zhuoyang Li, Lu Huang, Junchao Wang. 2022-10-06. Redshift Evolution and Non-Universal Dispersion of Quasar Luminosity Correlation. https://doi.org/10.1093/mnras%2Fstac2735

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