A search for sterile neutrinos with the latest cosmological observations

Abstract We report the result of a search for sterile neutrinos with the latest cosmological observations. Both cases of massless and massive sterile neutrinos are considered in the $$\Lambda $$ Λ CDM cosmology. The cosmological observations used in this work include the Planck 2015 temperature and...

Full description

Bibliographic Details
Main Authors: Lu Feng, Jing-Fei Zhang, Xin Zhang
Format: Article
Language:English
Published: SpringerOpen 2017-06-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-4986-3
id doaj-2d18e6e0f8c344a9a5231da1c70c670f
record_format Article
spelling doaj-2d18e6e0f8c344a9a5231da1c70c670f2020-11-25T00:42:44ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-06-017761910.1140/epjc/s10052-017-4986-3A search for sterile neutrinos with the latest cosmological observationsLu Feng0Jing-Fei Zhang1Xin Zhang2Department of Physics, College of Sciences, Northeastern UniversityDepartment of Physics, College of Sciences, Northeastern UniversityDepartment of Physics, College of Sciences, Northeastern UniversityAbstract We report the result of a search for sterile neutrinos with the latest cosmological observations. Both cases of massless and massive sterile neutrinos are considered in the $$\Lambda $$ Λ CDM cosmology. The cosmological observations used in this work include the Planck 2015 temperature and polarization data, the baryon acoustic oscillation data, the Hubble constant direct measurement data, the Planck Sunyaev–Zeldovich cluster counts data, the Planck lensing data, and the cosmic shear data. We find that the current observational data give a hint of the existence of massless sterile neutrino (as dark radiation) at the 1.44 $$\sigma $$ σ level, and the consideration of an extra massless sterile neutrino can indeed relieve the tension between observations and improve the cosmological fit. For the case of massive sterile neutrino, the observations give a rather tight upper limit on the mass, which implies that actually a massless sterile neutrino is more favored. Our result is consistent with the recent result of neutrino oscillation experiment done by the Daya Bay and MINOS collaborations, as well as the recent result of cosmic ray experiment done by the IceCube collaboration.http://link.springer.com/article/10.1140/epjc/s10052-017-4986-3
collection DOAJ
language English
format Article
sources DOAJ
author Lu Feng
Jing-Fei Zhang
Xin Zhang
spellingShingle Lu Feng
Jing-Fei Zhang
Xin Zhang
A search for sterile neutrinos with the latest cosmological observations
European Physical Journal C: Particles and Fields
author_facet Lu Feng
Jing-Fei Zhang
Xin Zhang
author_sort Lu Feng
title A search for sterile neutrinos with the latest cosmological observations
title_short A search for sterile neutrinos with the latest cosmological observations
title_full A search for sterile neutrinos with the latest cosmological observations
title_fullStr A search for sterile neutrinos with the latest cosmological observations
title_full_unstemmed A search for sterile neutrinos with the latest cosmological observations
title_sort search for sterile neutrinos with the latest cosmological observations
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2017-06-01
description Abstract We report the result of a search for sterile neutrinos with the latest cosmological observations. Both cases of massless and massive sterile neutrinos are considered in the $$\Lambda $$ Λ CDM cosmology. The cosmological observations used in this work include the Planck 2015 temperature and polarization data, the baryon acoustic oscillation data, the Hubble constant direct measurement data, the Planck Sunyaev–Zeldovich cluster counts data, the Planck lensing data, and the cosmic shear data. We find that the current observational data give a hint of the existence of massless sterile neutrino (as dark radiation) at the 1.44 $$\sigma $$ σ level, and the consideration of an extra massless sterile neutrino can indeed relieve the tension between observations and improve the cosmological fit. For the case of massive sterile neutrino, the observations give a rather tight upper limit on the mass, which implies that actually a massless sterile neutrino is more favored. Our result is consistent with the recent result of neutrino oscillation experiment done by the Daya Bay and MINOS collaborations, as well as the recent result of cosmic ray experiment done by the IceCube collaboration.
url http://link.springer.com/article/10.1140/epjc/s10052-017-4986-3
work_keys_str_mv AT lufeng asearchforsterileneutrinoswiththelatestcosmologicalobservations
AT jingfeizhang asearchforsterileneutrinoswiththelatestcosmologicalobservations
AT xinzhang asearchforsterileneutrinoswiththelatestcosmologicalobservations
AT lufeng searchforsterileneutrinoswiththelatestcosmologicalobservations
AT jingfeizhang searchforsterileneutrinoswiththelatestcosmologicalobservations
AT xinzhang searchforsterileneutrinoswiththelatestcosmologicalobservations
_version_ 1725280584936194048