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Precision Constraints for Three-Flavor Neutrino Oscillations from the Full <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>MINOS</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math> and MINOS Dataset

P. Adamson, I. M. Anghel, A. Aurisano, G. Barr, A. Blake, S. Cao, Timothy J. Carroll, C. M. Castromonte, R. Chen, S. Childress, J. A. B. Coelho, S. De Rijck, J. J. Evans, G. J. Feldman, W. Flanagan, M. Gabrielyan, S. Germani, R. A. Gomes, P. Gouffon, N. Graf, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, L. W. Koerner, M. Kordosky, A. Kreymer, K. Lang, P. Lucas, W. A. Mann, Marvin L. Marshak, N. Mayer, R. Mehdiyev, J. R. Meier, William H. Miller, G.B. Mills, D. Naples, J. K. Nelson, R. J. Nichol, J. Michael O’Connor, R. B. Pahlka, Ž. Pavlović, G. Pawloski, A. Perch, M. M. Pfützner, D. D. Phan, R. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, P. Sail, M. C. Sánchez, J. Schneps, A. Schreckenberger, R. Sharma, A. Sousa, N. Tagg, J. Thomas, M. Thomson, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, P. Vahle, A. Weber, L. Whitehead, S. G. Wojcicki

2020Physical Review Letters60 citationsDOIOpen Access PDF

Abstract

We report the final measurement of the neutrino oscillation parameters $\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}$ and ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}$ using all data from the MINOS and $\mathrm{MINOS}+$ experiments. These data were collected using a total exposure of $23.76\ifmmode\times\else\texttimes\fi{}{10}^{20}$ protons on target producing ${\ensuremath{\nu}}_{\ensuremath{\mu}}$ and ${\overline{\ensuremath{\nu}}}_{\ensuremath{\mu}}$ beams and 60.75 kt yr exposure to atmospheric neutrinos. The measurement of the disappearance of ${\ensuremath{\nu}}_{\ensuremath{\mu}}$ and the appearance of ${\ensuremath{\nu}}_{e}$ events between the Near and Far detectors yields $|\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}|=2.4{0}_{\ensuremath{-}0.09}^{+0.08}(2.4{5}_{\ensuremath{-}0.08}^{+0.07})\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}\text{ }\text{ }{\mathrm{eV}}^{2}$ and ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}=0.4{3}_{\ensuremath{-}0.04}^{+0.20}(0.4{2}_{\ensuremath{-}0.03}^{+0.07})$ at 68% C.L. for normal (inverted) hierarchy.

Topics & Concepts

MINOSNeutrinoPhysicsParticle physicsFlavorNeutrino oscillationChemistryBiochemistryNeutrino Physics ResearchParticle physics theoretical and experimental studiesAstrophysics and Cosmic Phenomena