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Friday July 19th, 2013

Observation of νμνe Oscillation by Electron Neutrino Appearance

t2k_overview

Figure 1:Overview of the T2K experiment.

nu_mixing

Figure 2:Flavor mixing of neutrinos.

In the previous article from the High Energy Physics Laboratory News (Indication of νμνe Oscillation by Electron Neutrino Appearance)​, it was mentioned that “Signs of the yet unconfirmed neutrino appearance event νμνe have been captured”. We are now pleased to announce that we have successfully discovered this phenomenon.

The T2K experiment measures the phenomenon of neutrino flavor oscillation by observing a neutrino beam created at the J-PARC and the Super-Kamiokande.  J-PARC is a high-intensity proton accelerator facility in Tokai Village, Ibaraki Prefecture, and Super-Kamiokande is a neutrino observatory located in Kamioka Town, Gifu Prefecture, as illustrated in Figure 1.

Neutrino oscillation is a phenomenon that occurs due to the difference between neutrino mass eigenstates (ν1, ν2, ν3) and flavor eigenstates (νe, νμ, ντ)​ (Figure 2). Each flavor eigenstate is a linear combination of the three mass eigenstates, and the degree of mixing is expressed by mixing angles (θ12, θ23, θ13). From previous experiments, it was known with some precision that θ12​ and θ23​ are non-zero, but only an upper limit was known for θ13​ for a long time. This θ13​ has become measurable recently through experiments detecting neutrinos from reactors around last year.  The T2K experiment discovered the νμνe oscillation phenomenon associated with electron neutrino appearance that had not yet been confirmed and measured the angle from its frequency of appearance. This achievement was made possible by the extremely high-purity νμ​ beam generated at J-PARC and the high sensitivity of Super-Kamiokande in distinguishing νμ​ and νe reactions. Furthermore, to ensure that the events are due to neutrinos generated at J-PARC, the timing of the accelerator beam and the observation time at Super-Kamiokande are confirmed using GPS. Figure 3 shows an example of an event candidate for νe​ reaction by neutrinos from J-PARC observed at Super-Kamiokande, where an electron neutrino reacts with a neutron and creates a Cherenkov ring from the resulting electron.

sk_nue_event

Figure 3 : A candidate event of the electron neutrino reaction observed at Supere-Kamiokande, originating from J-PARC. A Cherenkov ring from an electron produced in which an electron neutrino reacts with a neutron is observed.

Since starting its full-fledged experiments in January 2010 until the accelerator shutdown due to the March 11, 2011, Great East Japan Earthquake, the T2K experiment has obtained data with a statistical quantity represented by 1.43×10²⁰ POT. “POT” stands for “Protons on Target” and represents the amount of proton beam irradiated on a graphite target initially to create neutrinos. This amount already exceeds the data accumulated by the K2K experiment over five years, which is a pioneering experiment of T2K. This indicates the excellent performance of the J-PARC accelerator.

Analyzing all the data obtained so far by the T2K experiment, a total of 532 neutrino events presumed to be originated from the beam at J-PARC were detected within Super-Kamiokande. Among these, after applying several criteria to exclude background events, 28 events of electron neutrino appearance by electron generation were detected. On the other hand, assuming that νμνe neutrino oscillation did not occur and conducting simulations, it was estimated that there would be 4.6 events of electron generation detected at Super-Kamiokande. Statistically considering this result, the probability that these 28 detected events are solely due to statistical errors is less than one in a trillion. In other words, the probability that these 28 events are indeed due to electron neutrino appearance is more than 99.9999999999%. This result conclusively confirms the existence of the electron neutrino appearance phenomenon, marking a world-first achievement. Figure 3 shows the reconstructed energy distribution of neutrinos, where the points with error bars represent the data, and the histogram represents the distribution expected from Monte Carlo simulations. The green area represents the part due to background events unrelated to νμνe​ oscillation, while the red area represents the expected amount of electron neutrino appearance assuming νμνe oscillation. The absence of the red area, i.e., oscillation to electron neutrinos, is evident from this plot, indicating a complete mismatch with the experimental results.

nue_spectrum

図4 : Comparison of electron neutrino appearance phenomenon between data (points with error bars) and Monte Carlo simulations (histograms). The green area shows a background distribution and the red area shows an expected amount of electron neutrinos assuming the electron neutrino appearance phenomenon.

The significance of measuring the neutrino mixing angle θ13 lies in its potential to probe CP asymmetry, which is considered one of the fundamental origins of the vast predominance of matter over antimatter in the current universe. While CP asymmetry in the quark sector has been measured, it is not large enough to explain the entire matter-antimatter asymmetry in the universe. Therefore, it is believed that there are other sources contributing to this asymmetry, with one candidate being CP asymmetry in the lepton sector. Theoretical understanding suggests that the CP asymmetry in the lepton sector cannot be observed if θ13​ were zero. Hence, the measurement of θ13 in this study opens the door to measuring CP asymmetry in the lepton sector, which is of significant importance.

The current amount of data acquired is approximately 2% of the initial goal. In the future, we plan to increase the data volume to further confirm the results, explore the oscillation phenomenon of antineutrinos in detail, and approach CP asymmetry in the lepton sector.