Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches

Hagstotz, Steffen; de Salas, Pablo F.; Gariazzo, Stefano; Pastor, Sergio; Gerbino, Martina; Lattanzi, Massimiliano; Vagnozzi, Sunny; Freese, Katherine

doi:10.1103/PhysRevD.104.123524

Title: Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches

Journal Article · Thu Dec 09 00:00:00 EST 2021 · Physical Review D

DOI:https://doi.org/10.1103/PhysRevD.104.123524· OSTI ID:1834974

Hagstotz, Steffen;

;

; Lattanzi, Massimiliano; Vagnozzi, Sunny; Freese, Katherine

We provide a consistent framework to set limits on properties of light sterile neutrinos coupled to all three active neutrinos using a combination of the latest cosmological data and terrestrial measurements from oscillations, β-decay and neutrinoless double-β-decay (0νββ) experiments. We directly constrain the full 3+1 active-sterile mixing matrix elements |U_α4|², with α ∈ (e, µ, τ ), and the mass-squared splitting Δm$${^2_4}_1$$ ☰ m$$^2_4$$ – m$$^2_1$$. We find that results for a 3+1 case differ from previously studied 1+1 scenarios where the sterile is only coupled to one of the neutrinos, which is largely explained by parameter space volume effects. Limits on the mass splitting and the mixing matrix elements are currently dominated by the cosmological data sets. The exact results are slightly prior dependent, but we reliably find all matrix elements to be constrained below |U_α4|² ≲ 10^-3. Short-baseline neutrino oscillation hints in favor of eV-scale sterile neutrinos are in serious tension with these bounds, irrespective of prior assumptions. We also translate the bounds from the cosmological analysis into constraints on the parameters probed by laboratory searches, such as m_β or m_ββ, the effective mass parameters probed by β-decay and 0νββ searches, respectively. When allowing for mixing with a light sterile neutrino, cosmology leads to upper bounds of m_β < 0.09 eV and m_ββ < 0.07 eV at 95% CL, more stringent than the limits from current laboratory experiments.

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Research Organization:: Argonne National Laboratory (ANL), Argonne, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Basic Energy Sciences (BES); Swedish Research Council (SRC); European Union, Horizon 2020 Research and Innovation Programme; Marie Skłodowska-Curie

Grant/Contract Number:: W7405-ENG-36; SC007859; AC02-06CH11357; 796941; FPA2017-85216-P; PROMETEO/2018/165

OSTI ID:: 1834974

Alternate ID(s):: OSTI ID: 1868989

Journal Information:: Physical Review D, Journal Name: Physical Review D Vol. 104 Journal Issue: 12; ISSN 2470-0010

Publisher:: American Physical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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