Dark sector interaction and the supernova absolute magnitude tension

It has been intensively discussed if modifications in the dynamics of Universe at late times is able or not to solve $H_0$ tension. On other hand, it also argued that tension actually a on 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, assess by comparing three theoretical models, namely standard $\Lambda$CDM, $w$CDM non-gravitational interaction (IDE) between dark energy (DE) matter (DM). We find IDE model can with coupling different from zero 95\% CL, confirming results obtained prior.