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KAMIOKANDE-II
1987
Earlier work this paper cites.
R. Bionta, G. Blewitt, C. Bratton, D. Casper, A. Ciocio, et al
1987
Earlier work this paper cites.
M. J. Longo, “TESTS OF RELATIVITY FROM SN1987a,” Phys.Rev
1987
Earlier work this paper cites.

Similar

S. R. Coleman and S. L. Glashow, “Cosmic ray and neutrino tests of special relativity,” Phys.Lett
1997
Cited alongside, same era.
S. R. Coleman and S. L. Glashow, “High-energy tests of Lorentz invariance,” Phys.Rev
1999
Cited alongside, same era.
Super-Kamiokande
2005
Cited alongside, same era.

Then

Super-Kamiokande
2006
Later among the works it cites.
Super-Kamiokande
Original
2008
Later among the works it cites.

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2011

New Constraints on Neutrino Velocities

Cohen, Andrew G., Glashow, Sheldon L.

Understand

The OPERA collaboration has claimed that muon neutrinos with mean energy of 17.5 GeV travel 730 km from CERN to the Gran Sasso at a speed exceeding that of light by about 7.5 km/s or 25 ppm.

However, we show that such superluminal neutrinos would lose energy rapidly via the bremsstrahlung of electron-positron pairs ($\nu\rightarrow \nu+e^-+e^+$).
For the claimed superluminal neutrino velocity and at the stated mean neutrino energy, we find that most of the neutrinos would have suffered several pair emissions en route, causing the beam to be depleted of higher energy neutrinos.
Thus we refute the superluminal interpretation of the OPERA result.