Sensitivity to light sterile neutrinos at ESSnuSB

Abstract We present a comprehensive analysis in the 3+1 active-sterile neutrino oscillation scenario for the sensitivity of the ESSnuSB experiment in the presence of light sterile neutrinos assuming both a far (FD) and a near (ND) detector. Our analysis show that when the ND is included, the results...

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Main Authors: Monojit Ghosh, Tommy Ohlsson, Salvador Rosauro-Alcaraz
Format: Article
Language:English
Published: SpringerOpen 2020-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP03(2020)026
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spelling doaj-ce664dd0d5b7418e97870f2e141141832020-11-25T01:31:24ZengSpringerOpenJournal of High Energy Physics1029-84792020-03-012020311710.1007/JHEP03(2020)026Sensitivity to light sterile neutrinos at ESSnuSBMonojit Ghosh0Tommy Ohlsson1Salvador Rosauro-Alcaraz2Department of Physics, School of Engineering Sciences, KTH Royal Institute of Technology, AlbaNova University CenterDepartment of Physics, School of Engineering Sciences, KTH Royal Institute of Technology, AlbaNova University CenterDepartamento de Física Teórica and Instituto de Física Teórica, IFT-UAM/CSIC, Universidad Autónoma de MadridAbstract We present a comprehensive analysis in the 3+1 active-sterile neutrino oscillation scenario for the sensitivity of the ESSnuSB experiment in the presence of light sterile neutrinos assuming both a far (FD) and a near (ND) detector. Our analysis show that when the ND is included, the results are significantly different compared to the ones obtained with the FD only. We find that the capability of ESSnuSB to constrain the sterile mixing parameters is sin2 2θ μe ∼ 10 −4 for ∆m 2 = 1 eV2 if the ND is included and it becomes sin2 2θ μe ∼ 10 −2 without the ND. Furthermore, we show that the sensitivity can go down to sin2 2θ μe ∼ 10 −3 for the most conservative choice of the systematics on the ND. Comparing the sensitivity with T2HK, T2HKK, and DUNE by considering the FD only, we find that the sensitivity of ESSnuSB is smaller for most of the parameter space. Studying the CP violation sensitivity, we find that if the ND is included, it can be larger in the 3+1 scenario than in the standard one. However, if the ND is not included, the sensitivity is smaller compared to the one in the standard scenario. We also find that the CP violation sensitivity due to δ 13 is larger compared to the one induced by δ 24. The sensitivities are slightly better for the dominant neutrino running ratio of ESSnuSB.http://link.springer.com/article/10.1007/JHEP03(2020)026Beyond Standard ModelNeutrino PhysicsCP violation
collection DOAJ
language English
format Article
sources DOAJ
author Monojit Ghosh
Tommy Ohlsson
Salvador Rosauro-Alcaraz
spellingShingle Monojit Ghosh
Tommy Ohlsson
Salvador Rosauro-Alcaraz
Sensitivity to light sterile neutrinos at ESSnuSB
Journal of High Energy Physics
Beyond Standard Model
Neutrino Physics
CP violation
author_facet Monojit Ghosh
Tommy Ohlsson
Salvador Rosauro-Alcaraz
author_sort Monojit Ghosh
title Sensitivity to light sterile neutrinos at ESSnuSB
title_short Sensitivity to light sterile neutrinos at ESSnuSB
title_full Sensitivity to light sterile neutrinos at ESSnuSB
title_fullStr Sensitivity to light sterile neutrinos at ESSnuSB
title_full_unstemmed Sensitivity to light sterile neutrinos at ESSnuSB
title_sort sensitivity to light sterile neutrinos at essnusb
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2020-03-01
description Abstract We present a comprehensive analysis in the 3+1 active-sterile neutrino oscillation scenario for the sensitivity of the ESSnuSB experiment in the presence of light sterile neutrinos assuming both a far (FD) and a near (ND) detector. Our analysis show that when the ND is included, the results are significantly different compared to the ones obtained with the FD only. We find that the capability of ESSnuSB to constrain the sterile mixing parameters is sin2 2θ μe ∼ 10 −4 for ∆m 2 = 1 eV2 if the ND is included and it becomes sin2 2θ μe ∼ 10 −2 without the ND. Furthermore, we show that the sensitivity can go down to sin2 2θ μe ∼ 10 −3 for the most conservative choice of the systematics on the ND. Comparing the sensitivity with T2HK, T2HKK, and DUNE by considering the FD only, we find that the sensitivity of ESSnuSB is smaller for most of the parameter space. Studying the CP violation sensitivity, we find that if the ND is included, it can be larger in the 3+1 scenario than in the standard one. However, if the ND is not included, the sensitivity is smaller compared to the one in the standard scenario. We also find that the CP violation sensitivity due to δ 13 is larger compared to the one induced by δ 24. The sensitivities are slightly better for the dominant neutrino running ratio of ESSnuSB.
topic Beyond Standard Model
Neutrino Physics
CP violation
url http://link.springer.com/article/10.1007/JHEP03(2020)026
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AT tommyohlsson sensitivitytolightsterileneutrinosatessnusb
AT salvadorrosauroalcaraz sensitivitytolightsterileneutrinosatessnusb
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