2D BAO vs 3D BAO: solving the Hubble tension with an alternative cosmological model
Sowmaydeep Dwivedi, Marcus H\"og{\aa}s

TL;DR
This paper investigates how using 2D BAO data instead of 3D BAO data within a bimetric gravity model can reduce the Hubble tension, aligning the Hubble constant with local measurements.
Contribution
It demonstrates that 2D BAO data, combined with a bimetric gravity framework, can reconcile the Hubble constant with local measurements, addressing biases from model-dependent 3D BAO data.
Findings
2D BAO data yields a Hubble constant consistent with local measurements.
Replacing 3D BAO with 2D BAO reduces the Hubble tension.
Bimetric gravity provides a viable framework for this analysis.
Abstract
Ordinary 3D Baryon Acoustic Oscillations (BAO) data are model-dependent, requiring the assumption of a cosmological model to calculate comoving distances during data reduction. Throughout the present-day literature, the assumed model is CDM. However, it has been pointed out in several recent works that this assumption can be inadequate when analyzing alternative cosmologies, potentially biasing the Hubble constant () low, thus contributing to the Hubble tension. To address this issue, 3D BAO data can be replaced with 2D BAO data, which is only weakly model-dependent. The impact of using 2D BAO data, in combination with alternative cosmological models beyond CDM, has been explored for several phenomenological models, showing a promising reduction in the Hubble tension. In this work, we accommodate these models in the theoretically robust framework of bimetric…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Adaptive optics and wavefront sensing · Spacecraft Design and Technology
