| Full text | |
| Author(s): |
Total Authors: 2
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| Affiliation: | [1] Inst Nacl Pesquisas Espaciais, Div Astrofis, Ave Astronautas 1758, BR-12227010 Sao Jose Dos Campos, SP - Brazil
[2] Univ Durham, Dept Phys, Inst Particle Phys Phenomenol, Durham DH1 3LE - England
Total Affiliations: 2
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| Document type: | Journal article |
| Source: | Physical Review D; v. 104, n. 6 SEP 15 2021. |
| Web of Science Citations: | 1 |
| Abstract | |
It has been intensively discussed if modifications in the dynamics of the Universe at late times are able or not able 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 constrain M-B using Pantheon supernovae Ia sample, baryon acoustic oscillations, and big bang nucleosynthesis data, and assess the M-B tension by comparing three theoretical models, namely the standard Lambda CDM, the wCDM, and a nongravitational interaction between dark energy (IDE) and dark matter. 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. (AU) | |
| FAPESP's process: | 18/18036-5 - Investigating physical aspects beyond the standard model linked to the themes of dark energy, modified gravity, neutrinos and gravitational waves |
| Grantee: | Rafael da Costa Nunes |
| Support Opportunities: | Scholarships in Brazil - Post-Doctoral |