A New Consistency Test for the $\Lambda$CDM Model using Radial and Transverse BAO Measurements
Xing-Han A. Zhao, Zheng Cai

TL;DR
This paper introduces a calibration-free consistency test for flat $\\Lambda$CDM using BAO distance ratios, which should be constant across redshifts, and applies it to DESI data to verify model consistency.
Contribution
The paper proposes a novel, calibration-free method to test flat $\Lambda$CDM by analyzing BAO distance ratios and demonstrates its application to recent DESI data.
Findings
Inferred $\Omega_M^\Lambda$ values are consistent with being redshift-independent.
The method provides an internal consistency check for flat $\Lambda$CDM.
Results are broadly consistent with the model within current uncertainties.
Abstract
We present a calibration-free consistency test of spatially flat CDM based on baryon acoustic oscillation (BAO) distance measurements. The method forms ratios of BAO distances including the Hubble distance, the comoving angular diameter distance, and the volume-averaged distance, so that the sound horizon scale cancels, and then maps each observed ratio to an effective flat-CDM matter density parameter, , defined as the value of that reproduces the measured ratio within CDM. Flat CDM predicts that should be independent of redshift and of the particular ratio used. For ratios involving the integrated distances, we associate them with well-defined effective line-of-sight redshift intervals based on the integral mean value theorem. We apply the test to BAO measurements from the…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Astronomy and Astrophysical Research
