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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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 |
work_keys_str_mv |
AT monojitghosh sensitivitytolightsterileneutrinosatessnusb AT tommyohlsson sensitivitytolightsterileneutrinosatessnusb AT salvadorrosauroalcaraz sensitivitytolightsterileneutrinosatessnusb |
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1725086924747571200 |