scholarly journals An atmospheric muon neutrino disappearance measurement with the MINOS far detector

2007 ◽  
Author(s):  
Jeremy Peter Gogos
Keyword(s):  
Muon Neutrino ◽  
Atmospheric Muon ◽  
Minos Far Detector

scholarly journals Uncertainties in atmospheric muon-neutrino fluxes arising from cosmic-ray primaries

2017 ◽  
Vol 95 (2) ◽  
Author(s):  
Justin Evans ◽  
Diego Garcia Gamez ◽  
Salvatore Davide Porzio ◽  
Stefan Söldner-Rembold ◽  
Steven Wren
Keyword(s):  
Cosmic Ray ◽  
Muon Neutrino ◽  
Atmospheric Muon ◽  
Neutrino Fluxes

Atmospheric Muon Neutrino Fraction above 1 GeV [Phys. Rev. Lett. 79, 345 (1997)]

1997 ◽  
Vol 79 (14) ◽  
pp. 2754-2754 ◽  
Author(s):  
R. Clark ◽  
R. Becker-Szendy ◽  
C. B. Bratton ◽  
J. Breault ◽  
D. Casper ◽  
...  
Keyword(s):  
Muon Neutrino ◽  
Atmospheric Muon

scholarly journals Atmospheric Muon Neutrino Fraction above 1 GeV

1997 ◽  
Vol 79 (3) ◽  
pp. 345-348 ◽  
Author(s):  
R. Clark ◽  
R. Becker-Szendy ◽  
C. B. Bratton ◽  
J. Breault ◽  
D. Casper ◽  
...  
Keyword(s):  
Muon Neutrino ◽  
Atmospheric Muon

scholarly journals eV-Scale Sterile Neutrino Search Using Eight Years of Atmospheric Muon Neutrino Data from the IceCube Neutrino Observatory

2020 ◽  
Vol 125 (14) ◽  
Author(s):  
M. G. Aartsen ◽  
R. Abbasi ◽  
M. Ackermann ◽  
J. Adams ◽  
J. A. Aguilar ◽  
...  
Keyword(s):  
Sterile Neutrino ◽  
Muon Neutrino ◽  
Atmospheric Muon

NEUTRINO MASSES AND MIXINGS IN FLIPPED SU(5)

1994 ◽  
Vol 09 (20) ◽  
pp. 1827-1834 ◽  
Author(s):  
MORIMITSU TANIMOTO
Keyword(s):  
Mass Operator ◽  
Renormalization Group Equation ◽  
Muon Neutrino ◽  
Neutrino Masses ◽  
Group Equation ◽  
Mass Matrices ◽  
Low Energies ◽  
Atmospheric Muon ◽  
Type Mass ◽  
Neutrino Masses And Mixings

We study the neutrino masses and mixings in the flipped SU(5) model assuming the Dimopoulos-Hall-Raby type mass matrices. The neutrino masses are evolved down to low energies by using the renormalization group equation of the effective seesaw mass operator. The ντ mass and the νµ−ντ mixing are predicted by using the solar neutrino data. The predicted mass is consistent with the condition of the hot dark matter expected from COBE results. Our results are also compared with the ones in SO(10). Although the large νµ−ντ mixing could be obtained in our model, the ντ mass is too small to be consistent with the atmospheric muon neutrino deficit from KAMIOKA and IMB.

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