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Title: Atmospheric neutrino observations in the MINOS far detector

Thesis/Dissertation ·
DOI:https://doi.org/10.2172/919081· OSTI ID:919081
 [1]
  1. Univ. of Cambridge (United Kingdom)

This thesis presents the results of atmospheric neutrino observations from a 12.23 ktyr exposure of the 5.42 kt MINOS Far Detector between 1st August 2003 until 1st March 2006. The separation of atmospheric neutrino events from the large background of cosmic muon events is discussed. A total of 277 candidate contained vertex v/$$\bar{v}$$μ CC data events are observed, with an expectation of 354.4±47.4 events in the absence of neutrino oscillations. A total of 182 events have clearly identified directions, 77 data events are identified as upward going, 105 data events are identified as downward going. The ratio between the measured and expected up/down ratio is: R$$data\atop{u/d}$$/R$$MC\atop{u/d}$$ = 0.72$$+0.13\atop{-0.11}$$(stat.)± 0.04 (sys.). This is 2.1σ away from the expectation for no oscillations. A total of 167 data events have clearly identified charge, 112 are identified as vμ events, 55 are identified as $$\bar{v}$$μ events. This is the largest sample of charge-separated contained-vertex atmospheric neutrino interactions so far observed. The ratio between the measured and expected $$\bar{v}$$μ/vμ ratio is: R$$data\atop{$$\bar{v}$v}$/ R$$MC\atop{$$\bar{v}$v}$ = 0.93 $$+0.19\atop{-0.15}$$ (stat.) ± 0.12 (sys.). This is consistent with vμ and $$\bar{v}$$μ having the same oscillation parameters. Bayesian methods were used to generate a log(L/E) value for each event. A maximum likelihood analysis is used to determine the allowed regions for the oscillation parameters Δm$$2\atop{32}$$ and sin223. The likelihood function uses the uncertainty in log(L/E) to bin events in order to extract as much information from the data as possible. This fit rejects the null oscillations hypothesis at the 98% confidence level. A fit to independent vμ and $$\bar{v}$$μ oscillation assuming maximal mixing for both is also performed. The projected sensitivity after an exposure of 25 ktyr is also discussed.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
AC02-07CH11359
OSTI ID:
919081
Report Number(s):
FERMILAB-THESIS-2007-29; TRN: US0806298
Country of Publication:
United States
Language:
English

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