Abstract

The next generation neutrino observatory proposed by the LBNO collaboration will address fundamental questions in particle and astroparticle physics. The experiment consists of a far detector, in its first stage a 20 kt LAr double phase TPC and a magnetised iron calorimeter, situated at 2300 km from CERN and a near detector based on a high-pressure argon gas TPC. The long baseline provides a unique opportunity to study neutrino flavour oscillations over their 1st and 2nd oscillation maxima exploring the $L/E$ behaviour, and distinguishing effects arising from $\delta_{CP}$ and matter. In this paper we have reevaluated the physics potential of this setup for determining the mass hierarchy (MH) and discovering CP-violation (CPV), using a conventional neutrino beam from the CERN SPS with a power of 750 kW. We use conservative assumptions on the knowledge of oscillation parameter priors and systematic uncertainties. The impact of each systematic error and the precision of oscillation prior is shown. We demonstrate that the first stage of LBNO can determine unambiguously the MH to $>5\sigma$C.L. over the whole phase space. We show that the statistical treatment of the experiment is of very high importance, resulting in the conclusion that LBNO has 100% probability to determine the MH in at most 4-5 years of running. Since the knowledge of MH is indispensable to extract $\delta_{CP}$ from the data, the first LBNO phase can convincingly give evidence for CPV on the $3\sigma$C.L. using today's knowledge on oscillation parameters and realistic assumptions on the systematic uncertainties.

Highlights

  • A 3σ C.L. would correspond to an evidence for the tested hypothesis

  • We show the effect of varying the prior on θ13 between 0% and 10% when all the other systematic errors on the oscillation parameters are set to 0%

  • The LBNO experiment is the outcome of intense and comprehensive design studies supported by the European Commission since 2008

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Summary

General principle

Our primary goal is to determine the mass hierarchy and measure CP violation by observing νμ to νe oscillations, through a precise measurement of the neutrino spectrum and the comparison of neutrino- and antineutrino-induced oscillations. The probabilities of νμ → νe and νμ → νe oscillations contain the spectral information which provides an unambiguous determination of the oscillations parameters and allows discriminating between the two CP-conserving scenarios, namely δCP = 0 and δCP = π. If the neutrino energy spectrum of the oscillated events can be reconstructed with sufficiently good resolution in order to distinguish first and second maxima, the spectral information obtained is invaluable for the unambiguous determination of the oscillation parameters. Guish first and second maximum, and extract unambiguous information on the oscillation parameters Using these signals, it is possible to test the standard 3-neutrino mixing framework, by looking for deviations from the expected L/E dependence and by comparing neutrinos and antineutrinos. A detailed description of neutrino event simulations and selection efficiency can be found in ref. [1]

Experimental observables
Analysis method
Statistical approach to MH and CPV determination
Assumption on parameters and systematics
Beam focusing mode optimisation
Significance of a first and second maxima analysis method
Impact of prior uncertainties on the δCP discovery potential
Influence of θ13 on the δCP discovery potential
Influence of θ23 on the δCP discovery potential
Impact of event normalization systematics on the δCP discovery potential
Statistical power as a function of exposure
Findings
Summary and conclusions
Full Text
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