A new method to build the (inverse) distance ladder
David Camarena, Valerio Marra

TL;DR
This paper introduces a novel method for constructing the cosmic distance ladder using the distance-duality relation, avoiding high-redshift modeling, and providing local measurements of key cosmological parameters to address the H0 tension.
Contribution
It presents a new approach that directly uses the distance-duality relation to build the cosmic distance ladder without relying on parametrizations at high redshift, improving the understanding of the H0 tension.
Findings
Low value of the deceleration parameter q0.
Strong inconsistency between angular-only and anisotropic BAO constraints.
Highlights the need to clarify BAO measurement tensions to understand the H0 crisis.
Abstract
The cosmic distance ladder is the succession of techniques by which it is possible to determine distances to astronomical objects. Here, we present a new method to build the cosmic distance ladder, going from local astrophysical measurements to the CMB. Instead of relying on high-redshift cosmography in order to model the luminosity-distance relation and calibrate supernovae with BAO, we exploit directly the distance-duality relation ---valid if photon number is conserved and gravity is described by a metric theory. The advantage is that the results will not depend on the parametrization of the luminosity-distance relation at : no model is adopted in order to calibrate BAO with supernovae. This method yields local measurements of the Hubble constant and deceleration parameter. Furthermore, it can directly assess the impact of BAO observations on the strong…
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