Bayesian Model Comparison of $R_h=ct$ versus $Λ$CDM using HII galaxy Hubble diagram

Fuente: arXiv
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Autores principales: Pallam, Yuva Himanshu, Desai, Shantanu
Formato: Preprint
Publicado: 2026
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author Pallam, Yuva Himanshu
Desai, Shantanu
author_facet Pallam, Yuva Himanshu
Desai, Shantanu
contents We complement a recent analysis comparing $R_\mathrm{h}=ct$ with $Λ$CDM/$w$CDM using HII galaxies and giant extragalactic HII regions, by carrying out Bayesian model comparison. For this purpose, we calculate the Bayes factors for $R_\mathrm{h}=ct$ compared to flat $Λ$CDM/$w$CDM using the same dataset. When we use uniform priors on cosmological parameters, we find that the Bayes factors are close to 1, implying that $R_\mathrm{h}=ct$ is equally favored compared to $Λ$CDM/$w$CDM. However, when we use normal priors on cosmological parameters based on Planck cosmology, we find that $R_\mathrm{h}=ct$ is strongly favored over flat $Λ$CDM, while $R_\mathrm{h}=ct$ is marginally favored over flat $w$CDM.
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publishDate 2026
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spellingShingle Bayesian Model Comparison of $R_h=ct$ versus $Λ$CDM using HII galaxy Hubble diagram
Pallam, Yuva Himanshu
Desai, Shantanu
Cosmology and Nongalactic Astrophysics
We complement a recent analysis comparing $R_\mathrm{h}=ct$ with $Λ$CDM/$w$CDM using HII galaxies and giant extragalactic HII regions, by carrying out Bayesian model comparison. For this purpose, we calculate the Bayes factors for $R_\mathrm{h}=ct$ compared to flat $Λ$CDM/$w$CDM using the same dataset. When we use uniform priors on cosmological parameters, we find that the Bayes factors are close to 1, implying that $R_\mathrm{h}=ct$ is equally favored compared to $Λ$CDM/$w$CDM. However, when we use normal priors on cosmological parameters based on Planck cosmology, we find that $R_\mathrm{h}=ct$ is strongly favored over flat $Λ$CDM, while $R_\mathrm{h}=ct$ is marginally favored over flat $w$CDM.
title Bayesian Model Comparison of $R_h=ct$ versus $Λ$CDM using HII galaxy Hubble diagram
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2603.28019