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Evidence for $\barν_μ\to\barν_e$ Oscillations from the LSND Experiment at LAMPF

C. Athanassopoulos, L. B. Auerbach, R. L. Burman, I. Cohen, D. O. Caldwell, B. D. Dieterle, J. B. Donahue, A. M. Eisner, A. Fazely, F. J. Federspiel, G. T. Garvey, M. Gray, R. M. Gunasingha, R. Imlay, K. Johnston, H. J. Kim, W. C. Louis, R. Majkic, J. Margulies, K. McIlhany, W. Metcalf, G. B. Mills, R. A. Reeder, V. Sandberg, D. Smith, I. Stancu, W. Strossman, R. Tayloe, G. J. VanDalen, W. Vernon, N. Wadia, J. Waltz, Y-X. Wang, D. H. White, D. Works, Y. Xiao, S. Yellin, LSND Collaboration

Abstract

A search for $\barν_μ\to \barν_{e}$ oscillations has been conducted at the Los Alamos Meson Physics Facility by using $\barν_μ$ from $μ^+$ decay at rest. The $\barν_e$ are detected via the reaction $\barν_e\,p \rightarrow e^{+}\,n$, correlated with a $γ$ from $np\rightarrow dγ$ ($2.2\,{\rm MeV}$). The use of tight cuts to identify $e^+$ events with correlated $γ$ rays yields 22 events with $e^+$ energy between 36 and $60\,{\rm MeV}$ and only $4.6 \pm 0.6$ background events. A fit to the $e^+$ events between 20 and $60\,{\rm MeV}$ yields a total excess of $51.8^{+18.7}_{-16.9} \pm 8.0$ events. If attributed to $\bar ν_μ\rightarrow \bar ν_e$ oscillations, this corresponds to an oscillation probability of ($0.31^{+0.11}_{-0.10} \pm 0.05$)\%.

Evidence for $\barν_μ\to\barν_e$ Oscillations from the LSND Experiment at LAMPF

Abstract

A search for oscillations has been conducted at the Los Alamos Meson Physics Facility by using from decay at rest. The are detected via the reaction , correlated with a from (). The use of tight cuts to identify events with correlated rays yields 22 events with energy between 36 and and only background events. A fit to the events between 20 and yields a total excess of events. If attributed to oscillations, this corresponds to an oscillation probability of ()\%.

Paper Structure

This paper contains 3 figures, 1 table.

Figures (3)

  • Figure 1: The energy distribution for events which pass selection B with (a) $R \ge 0$ and (b) $R>30$. Shown in the figure are the beam-excess data, estimated neutrino background (dashed), and expected distribution for neutrino oscillations at large $\Delta m^2$ plus estimated neutrino background (solid).
  • Figure 2: The R distribution, beam on minus beam-off excess, for events that satisfy selection B and that have energies in the range $20<E_e<60$ MeV. The solid curve is the best fit to the data, the dashed curve is the uncorrelated $\gamma$ component of the fit, and the dotted curve is the correlated $\gamma$ component.
  • Figure 3: Plot of the LSND $\Delta m^{2}~$$\sl vs$$\sin^2 2 \theta~$ favored regions. The shaded regions are the 90% or 99% likelihood regions as defined in the text, not confidence regions. Also shown are $90\%$ C.L. limits from KARMEN at ISIS (dashed curve), E776 at BNL (dotted curve), and the Bugey reactor experiment (dot-dashed curve).