We present measurements of nu(mu) disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment. One-hundred and twelve beam-originated neutrino events are observed in the fiducial volume of Super-Kamiokande with an expectation of 158.1(-8.6)(+9.2) events without oscillation. A distortion of the energy spectrum is also seen in 58 single-ring muonlike events with reconstructed energies. The probability that the observations are explained by the expectation for no neutrino oscillation is 0.0015% (4.3 sigma). In a two-flavor oscillation scenario, the allowed Delta m(2) region at sin(2)2 theta=1 is between 1.9 and 3.5x10(-3) eV(2) at the 90% C.L. with a best-fit value of 2.8x10(-3) eV(2).

Measurement of neutrino oscillation by the K2K experiment / M. H., A., E., A., S., A., S., A., Y., A., J., A., K., A., R., A., F., B., H. G., B., H., B., A., B., S., B., J., B., S. C., B., J., B.C., D., C., J., C., C., C., A., C., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 74:7(2006). [10.1103/physrevd.74.072003]

Measurement of neutrino oscillation by the K2K experiment

DORE, Ubaldo;LOVERRE, Pier Ferruccio;
2006

Abstract

We present measurements of nu(mu) disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment. One-hundred and twelve beam-originated neutrino events are observed in the fiducial volume of Super-Kamiokande with an expectation of 158.1(-8.6)(+9.2) events without oscillation. A distortion of the energy spectrum is also seen in 58 single-ring muonlike events with reconstructed energies. The probability that the observations are explained by the expectation for no neutrino oscillation is 0.0015% (4.3 sigma). In a two-flavor oscillation scenario, the allowed Delta m(2) region at sin(2)2 theta=1 is between 1.9 and 3.5x10(-3) eV(2) at the 90% C.L. with a best-fit value of 2.8x10(-3) eV(2).
2006
01 Pubblicazione su rivista::01a Articolo in rivista
Measurement of neutrino oscillation by the K2K experiment / M. H., A., E., A., S., A., S., A., Y., A., J., A., K., A., R., A., F., B., H. G., B., H., B., A., B., S., B., J., B., S. C., B., J., B.C., D., C., J., C., C., C., A., C., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 74:7(2006). [10.1103/physrevd.74.072003]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/90905
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