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Title: Sensitivities to neutrino non-standard interactions from the disappearance of muon (anti)neutrinos at the NOvA experiment

Thesis/Dissertation ·
OSTI ID:1835861

The experimental confirmation of the phenomenon of neutrino oscillations provided evidence for a non-zero value for the mass of neutrinos, a property not initially predicted by the Standard Model of Physics. Investigations of the existence of the so called Physics Beyond the Standard Model is a subject of growing interest and effort in the field of particle physics. Interactions of neutrinos with matter are well described by the Standard Model, however in the presence of new Physics, additional phenomena regarding neutrino properties would be possible, including non-standard interactions of neutrinos with matter. The NOvA experiment, at Fermilab, has been investigating neutrino oscillations through studies of νµ produced at the Fermilab accelerator facilities, and also comprise a suitable environment for investigation of additional phenomena taking part in the neutrino oscillation framework. We show in this thesis the results of the sensitivity studies to neutrino non standard interactions in the NOvA experiment through investigation of the disappearance of muon (anti)neutrinos during their evolution in the NOvA 810 km baseline. We investigate the effect of the NSI parameters, |εµτ| and δµτ, on the determination of the standard oscillation parameters sin223) and Δ$$m^2_{32}$$, as well as the relation between each parameter, for both neutrino mass hierarchies. This study makes use of an exposure of 9.48 × 1020 POT for neutrino beam (FHC), and 12.33 × 1020 POT for antineutrino beam (RHC). No deviations from the standard oscillation scenario is found at the 90% CL limit. The joint neutrino and antineutrino fit yields a limit of |εµτ| ≤ 0.086 (0.085) for a fixed value of δµτ = 0, and |εµτ| ≤ 1.054 (1.053) for the case where both NSI parameters are fitted, for the normal (inverted) neutrino mass hierarchy, at the 90% CL. In the current sensitivity, all values of δµτ are found to be allowed. The 90% CL interval for the standard oscillation parameters are Δ$$m^2_{32}$$ ϵ [2.379, 2.580] and sin223) ϵ [0.420, 0.602] for the normal hierarchy scenario, and Δ$$m^2_{32}$$ ϵ [-2.639, - 2.438] and sin223) ϵ [0.418, 0.602] for the inverted hierarchy scenario.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1835861
Report Number(s):
FERMILAB-MASTERS-2020-08; oai:inspirehep.net:1988798
Country of Publication:
United States
Language:
English

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