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arXiv · 2107.09151

Dark sector interaction and the supernova absolute magnitude tension

Rafael C. Nunes·Eleonora Di Valentino
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Abstract

It has been intensively discussed if modifications in the dynamics of the Universe at late times is able or not to solve the $H_0$ tension. On the other hand, it has also been argued that the $H_0$ tension is actually a tension on the supernova absolute magnitude $M_B$. In this work, we robustly constraint $M_B$ using Pantheon Supernovae Ia (SN) sample, Baryon Acoustic Oscillations (BAO), and Big Bang Nucleosynthesis (BBN) data, and assess the $M_B$ tension by comparing three theoretical models, namely the standard $\Lambda$CDM, the $w$CDM and a non-gravitational interaction (IDE) between dark energy (DE) and dark matter (DM). We find that the IDE model can solve the $M_B$ tension with a coupling different from zero at 95\% CL, confirming the results obtained using a $H_0$ prior.

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Rafael C. Nunes, Eleonora Di Valentino. 2021-07-19. Dark sector interaction and the supernova absolute magnitude tension. https://doi.org/10.1103/physrevd.104.063529

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