The neutrino velocity anomaly as an explanation of the missing observation of neutrinos in coincidence with GRB

Abstract

The search for neutrinos emitted in coincidence with Gamma-Bay Burst has been so far unsuccessfully. In this paper we show that the recent result reported by the OPERA Collaboration on an early arrival time of muon neutrinos with respect to the one computed assuming the speed of light in vacuum could explain the null search for neutrinos in coincidence with Gamma-Ray Burst.

References in corpus (4)

• Observation of a first ${\nu }_{\tau }$ candidate in the OPERA experiment in the CNGS beam
• IceCube: An Instrument for Neutrino Astronomy
• The detection of neutrino interactions in the emulsion/lead target of the OPERA experiment
• High Energy Neutrino Emission from the Earliest Gamma-Ray Bursts

Cited by in corpus (4)

• Beyond the speed of light on Finsler spacetimes
• Nonlinear bulk viscosity and the stability of accelerated expansion in FRW spacetime
• Constraints on the interpretation of the superluminal motion of neutrinos at OPERA
• Olber's Paradox for Superluminal Neutrinos: Constraining Extreme Neutrino Speeds at TeV-ZeV Energies with the Diffuse Neutrino Background