A New Consistency Test for the $Λ$CDM Model using Radial and Transverse BAO Measurements
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arXiv
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| Formato: | Preprint |
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2026
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| author | Zhao, Xing-Han A. Cai, Zheng |
| author_facet | Zhao, Xing-Han A. Cai, Zheng |
| contents | We present a calibration-free consistency test of spatially flat $Λ$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-$Λ$CDM matter density parameter, $Ω_{\rm M}^Λ$, defined as the value of $Ω_{\rm M}$ that reproduces the measured ratio within $Λ$CDM. Flat $Λ$CDM predicts that $Ω_{\rm M}^Λ$ 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 Dark Energy Spectroscopic Instrument (DESI) Data Release~1 and Data Release~2, propagating the full published BAO covariance matrices into all derived ratios and $Ω_{\rm M}^Λ$ constraints. Within current uncertainties, the inferred $Ω_{\rm M}^Λ$ values are broadly consistent with a redshift-independent constant, providing an internal consistency check of flat $Λ$CDM that can be strengthened straightforwardly as BAO measurements improve. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2601_07075 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | A New Consistency Test for the $Λ$CDM Model using Radial and Transverse BAO Measurements Zhao, Xing-Han A. Cai, Zheng Cosmology and Nongalactic Astrophysics We present a calibration-free consistency test of spatially flat $Λ$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-$Λ$CDM matter density parameter, $Ω_{\rm M}^Λ$, defined as the value of $Ω_{\rm M}$ that reproduces the measured ratio within $Λ$CDM. Flat $Λ$CDM predicts that $Ω_{\rm M}^Λ$ 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 Dark Energy Spectroscopic Instrument (DESI) Data Release~1 and Data Release~2, propagating the full published BAO covariance matrices into all derived ratios and $Ω_{\rm M}^Λ$ constraints. Within current uncertainties, the inferred $Ω_{\rm M}^Λ$ values are broadly consistent with a redshift-independent constant, providing an internal consistency check of flat $Λ$CDM that can be strengthened straightforwardly as BAO measurements improve. |
| title | A New Consistency Test for the $Λ$CDM Model using Radial and Transverse BAO Measurements |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2601.07075 |