1. Cornering (quasi) degenerate neutrinos with cosmology
- Author
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Martina Gerbino, José W. F. Valle, Katherine Freese, Massimiliano Lattanzi, Gordon L. Kane, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), and Generalitat Valenciana
- Subjects
Nuclear and High Energy Physics ,Particle physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::High Energy Astrophysical Phenomena ,Cosmic microwave background ,FOS: Physical sciences ,Lambda-CDM model ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Cosmology ,symbols.namesake ,High Energy Physics - Phenomenology (hep-ph) ,Double beta decay ,0103 physical sciences ,Neutrino Physics ,lcsh:Nuclear and particle physics. Atomic energy. Radioactivity ,Planck ,010306 general physics ,Neutrino oscillation ,Physics ,010308 nuclear & particles physics ,Computer Science::Information Retrieval ,High Energy Physics::Phenomenology ,Cosmology of Theories beyond the SM ,High Energy Physics - Phenomenology ,symbols ,lcsh:QC770-798 ,High Energy Physics::Experiment ,Baryon acoustic oscillations ,Neutrino ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In light of the improved sensitivities of cosmological observations, we examine the status of quasi-degenerate neutrino mass scenarios. Within the simplest extension of the standard cosmological model with massive neutrinos, we find that quasi-degenerate neutrinos are severely constrained by present cosmological data and neutrino oscillation experiments. % % We find that Planck 2018 observations of cosmic microwave background (CMB) anisotropies disfavour quasi-degenerate neutrino masses at $2.4$ Gaussian $\sigma$'s, while adding Baryon acoustic oscillations (BAO) data brings the rejection to 5.9$\sigma$'s. % The highest statistical significance with which one would be able to rule out quasi-degeneracy would arise if the sum of neutrino masses is $\Sigma m_\nu = 60$ \meV (the minimum allowed by neutrino oscillation experiments); % indeed a sensitivity of 15 meV, as expected from a combination of future cosmological probes, would further improve the rejection level up to 17$\sigma$. % We discuss the robustness of these projections with respect to assumptions on the underlying cosmological model, and also compare them with bounds from $\beta$ decay endpoint and neutrinoless double beta decay studies., Comment: 19 pages, 6 figures, 1 table
- Published
- 2020