Seeking sterile neutrinos in Finslerian cosmology

Autor: Deng Wang, Xin-He Meng
Jazyk: angličtina
Rok vydání: 2017
Předmět:
Zdroj: European Physical Journal C: Particles and Fields, Vol 77, Iss 11, Pp 1-12 (2017)
Druh dokumentu: article
ISSN: 1434-6044
1434-6052
DOI: 10.1140/epjc/s10052-017-5284-9
Popis: Abstract For the first time, to search for sterile neutrinos in the framework of Finler geometry, we constrain four cosmological models using the most stringent constraint we can provide so far. We find that the Finslerian massless sterile neutrino model can, respectively, give a better cosmological fit to data and alleviate the current $$H_0$$ H 0 tension more effectively than the other three models. For the Finslerian massless sterile neutrino model, we obtain the constraint $$N_\mathrm{eff}=3.237^{+0.092}_{-0.185}$$ N eff = 3 . 237 - 0.185 + 0.092 , which is consistent with $$\Delta N_\mathrm{eff} > 0$$ Δ N eff > 0 at the 1.03 $$\sigma $$ σ confidence level (CL). This gives a very weak hint of massless sterile neutrinos and may imply the non-existence of massless sterile neutrinos in the Finslerian cosmological setting. For the Finslerian massive sterile neutrino model, we obtain the constraints $$ N_\mathrm{eff}=3.143^{+0.064}_{-0.066}$$ N eff = 3 . 143 - 0.066 + 0.064 , which favors $$\Delta N_\mathrm{eff} > 0$$ Δ N eff > 0 at the 1.47 $$\sigma $$ σ CL, and $$m_{\nu , \mathrm{sterile}}^\mathrm{eff} < 0.121$$ m ν , sterile eff < 0.121 eV at the 2 $$\sigma $$ σ CL which is much tighter than the Planck results. This very tight restriction appears to indicate the massive sterile neutrinos are also non-existent in the Finslerian scenarios. Consequently, one may conclude that the sterile neutrinos are possibly non-existent in the Finslerian universe. Our results are compatible with the recent results of the neutrino oscillation experiments implemented by the Daya Bay and MINOS collaborations and the cosmic ray one carried out by the IceCube collaboration.
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