Date

A Limit on muon-neutrino (anti-muon-neutrino) ---> tau-neutrino (anti-tau-neutrino) oscillations from a precision measurement of neutrino - nucleon neutral current interactions

McFarland, Kevin Scott ; Naples, D. ; Arroyo, C.G. ; et al.
Phys.Rev.Lett. 75 (1995) 3993-3996, 1995.
Inspire Record 396286 DOI 10.17182/hepdata.42343

We present a limit on $\nu_\mu(\overline{\nu}_\mu)\to\nu_\tau(\overline{\nu}_\tau)$ oscillations based on a study of inclusive $\nu N$ interactions performed using the CCFR massive coarse grained detector in the FNAL Tevatron Quadrupole Triplet neutrino beam. The sensitivity to oscillations is from the difference in the longitudinal energy deposition pattern of $\nu_\mu N$ versus $\nu_\tau N$ charged current interactions. The $\nu_\mu$ energies ranged from $30$ to $500$GeV with a mean of $140$GeV. The minimum and maximum $\nu_\mu$ flight lengths are $0.9$km and $1.4$km respectively. The lowest $90\%$ confidence upper limit in $\sin~22\alpha$ of $2.7\times 10~{-3}$ is obtained at $\Delta m~2\sim50$eV$~2$. This result is the most stringent limit to date for $25<\Delta m~2<90$eV$~2$.

2 data tables

ALPHA is the neutrino mixing angle. The result for SIN(ALPHA)**2 from the fit at each Delta(M)**2 for NUMU -->NUTAU oscillations. The 90% CL upper limit is equal to the best fit SIN(ALPHA)**2 + 1.2*SIGMA.

ALPHA is the neutrino mixing angle. The result for SIN(ALPHA)**2 from the fit at each Delta(M)**2 for NUMU -->NUE oscillations. The 90% CL upper limit is equal to the best fit SIN(ALPHA)**2 + 1.2*SIGMA.


Measurement of the reaction C-12 (muon-neutrino, mu-) X near threshold

The LSND collaboration Albert, M. ; Athanassopoulos, C. ; Auerbach, L.B. ; et al.
Phys.Rev.C 51 (1995) 1065-1069, 1995.
Inspire Record 378770 DOI 10.17182/hepdata.25973

The reaction $~{12}{\rm C}(\nu_\mu,\mu~-) {\rm X}$ has been measured near threshold using a $\pi ~+$ decay-in-flight $\nu_\mu$ beam from the Los Alamos Meson Physics Facility and a massive liquid scintillator neutrino detector (LSND). In the energy region $123.7 < {\rm E}_\nu < 280$ MeV, the measured spectral shape is consistent with that expected from the Fermi Gas Model. However, the measured flux--averaged inclusive cross section ($(8.3 \pm 0.7 {\rm stat.} \pm 1.6 {\rm syst.}) \times 10~{-40} {\rm cm}~2$) is more than a factor of 2 lower than that predicted by the Fermi Gas Model and by a recent random phase approximation calculation.

1 data table

No description provided.


Polarization of $\Lambda$ and $\bar{\Lambda}$ Produced by 800 GeV Protons

Ramberg, E.J. ; Bock, G.J. ; Coleman, R. ; et al.
Phys.Lett.B 338 (1994) 403-408, 1994.
Inspire Record 372108 DOI 10.17182/hepdata.42451

We have measured the polarization of Λ and Λ hyperons produced by 800 GeV protons on a Be target at a fixed targeting angle of 4.8 mrad. Comparison with previous data at 400 GeV production energy and twice the targeting angle shows no significant energy dependence for the Λ polarization. This is in striking contrast to the energy dependence found for σ + and Ξ − polarizations. We find no evidence for Λ polarization at 800 GeV.

2 data tables

Errors are combined statistics and systematics.

No description provided.