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2024

2D BAO vs 3D BAO: Hints for new physics?

Ruchika

Understand

As next-generation telescopes and observational surveys continue to expand the boundaries of our understanding, tensions and discrepancies between observational datasets are becoming increasingly prominent.

In this work, we focus on one such discrepancy: the differences between 2D and 3D Baryon Acoustic Oscillation (BAO) measurements.
Without extending beyond the standard $\Lambda$CDM framework, we systematically study and highlight this discrepancy in different parameter spaces.
This work examines the constraints on fundamental cosmological parameters ($H_0$, $r_d$, $\Omega_m$) derived from Baryon Acoustic Oscillation (BAO) and Type Ia Supernovae (SNIa) data.