Table of Contents
Fetching ...

Electron neutrino and antineutrino appearance in the full MINOS data sample

P. Adamson, I. Anghel, C. Backhouse, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, D. Cherdack, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, M. V. Frohne, H. R. Gallagher, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Himmel, A. Holin, J. Hylen, G. M. Irwin, Z. Isvan, D. E. Jaffe, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, M. Mathis, N. Mayer, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. P. Ochoa-Ricoux, J. O'Connor, W. P. Oliver, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, S. Phan-Budd, R. K. Plunkett, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, G. Tinti, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, S. G. Wojcicki, T. Yang, R. Zwaska

TL;DR

This analysis is the first use of this technique and includes the first accelerator long-baseline search for ν (μ) → ν(e), and the data disfavor 31% (5%) of the three-parameter space defined by δ, the octant of the θ23, and the mass hierarchy at the 68% (90%) C.L.

Abstract

We report on $ν_e$ and $\barν_e$ appearance in $ν_μ$ and $\barν_μ$ beams using the full MINOS data sample. The comparison of these $ν_e$ and $\barν_e$ appearance data at a 735 km baseline with $θ_{13}$ measurements by reactor experiments probes $δ$, the $θ_{23}$ octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for $\barν_μ\rightarrow\barν_e$. Our data disfavor 31% (5%) of the three-parameter space defined by $δ$, the octant of the $θ_{23}$, and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sin$^2(2θ_{13})$sin$^2(θ_{23})$ that is consistent with reactor experiments.

Electron neutrino and antineutrino appearance in the full MINOS data sample

TL;DR

This analysis is the first use of this technique and includes the first accelerator long-baseline search for ν (μ) → ν(e), and the data disfavor 31% (5%) of the three-parameter space defined by δ, the octant of the θ23, and the mass hierarchy at the 68% (90%) C.L.

Abstract

We report on and appearance in and beams using the full MINOS data sample. The comparison of these and appearance data at a 735 km baseline with measurements by reactor experiments probes , the octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for . Our data disfavor 31% (5%) of the three-parameter space defined by , the octant of the , and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sinsin that is consistent with reactor experiments.

Paper Structure

This paper contains 4 figures, 2 tables.

Figures (4)

  • Figure 1: Distributions of $\alpha_{LEM}$. The plots in the left column correspond to the $\nu$ beam mode. The plots in the right column correspond to the $\bar{\nu}$ beam mode. The top row shows the distributions for ND selected events with a band about the simulation representing the systematic uncertainty. The bottom row shows the distributions for the predicted FD background and signal multiplied by 10 with 2sin$^2(2\theta_{13})$sin$^2(\theta_{23})$$=$$0.1$, $\delta$$=$ 0, and a normal mass hierarchy.
  • Figure 2: The reconstructed energy distributions for three $\alpha_{LEM}$ ranges. The events with energy greater than 5 GeV are combined into a single bin for the fits. The vertical bars through the data points denote statistical uncertainties. The signal predictions assume sin$^2$(2$\theta_{13}$) = 0.051, $\Delta m^{2}_{32}$$>$ 0, $\delta$ = 0, and $\theta_{23}$ = $\pi/4$. The plots in the left column correspond to data collected in the $\nu$ beam mode. The plots in the right column correspond to data collected in the $\bar{\nu}$ beam mode.
  • Figure 3: The 68% and 90% confidence intervals of allowed values for 2sin$^2(2\theta_{13})$sin$^2(\theta_{23})$ as a function of $\delta$ for the two mass hierarchies.
  • Figure 4: The resulting values of the likelihood $L$, shown here as $-2\Delta$ln$L$, from a fit of $\delta$ to our data using constraints from reactor experiments ref:DCref:DBref:RENO, assuming various values of the mass hierarchy and the sign of $\theta_{23}-\pi/4$. The difference is taken with respect to the best-fitting solution. Values above the horizontal dashed lines are disfavored at either 68% or 90% C.L.