English

A calibration-free null test from anisotropic BAO

Cosmology and Nongalactic Astrophysics 2026-03-20 v1

Abstract

Baryon acoustic oscillation (BAO) analyses usually report the anisotropic shift parameters α(z)\alpha_\perp(z) and α(z)\alpha_\parallel(z) relative to a fiducial cosmology, and these quantities are primarily used for cosmological parameter inference. Here we show that they can also be used to construct a direct internal consistency test of the background geometry. In particular, we derive a new null test of flat Friedmann-Lema\^itre-Robertson-Walker (FLRW) geometry written entirely in terms of the reported BAO shift parameters. The test is calibration free: the sound-horizon ratio rd/rdfidr_{\rm d}/r^{\rm fid}_{\rm d} cancels identically, so the relation is independent of the absolute BAO scale. We also derive a calibration-free reconstruction of the deceleration parameter q(z)q(z) from the radial BAO sector. Applying these results to anisotropic DESI DR2 BAO measurements, we find no evidence for a breakdown of the flat-FLRW distance relation within current uncertainties. Our results show that anisotropic BAO measurements already provide a nontrivial internal geometric consistency test before performing any model fit.

Keywords

Cite

@article{arxiv.2603.18986,
  title  = {A calibration-free null test from anisotropic BAO},
  author = {Domenico Sapone and Savvas Nesseris},
  journal= {arXiv preprint arXiv:2603.18986},
  year   = {2026}
}

Comments

6 pages, 4 figures

R2 v1 2026-07-01T11:28:17.546Z