Literature DB >> 22107624

Pair creation constrains superluminal neutrino propagation.

Andrew G Cohen1, Sheldon L Glashow.   

Abstract

The OPERA collaboration claims that muon neutrinos with a 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 superluminal neutrinos may lose energy rapidly via the bremsstrahlung of electron-positron pairs (ν → ν + e- + e+). For the claimed superluminal velocity and at the stated mean 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. This presents a significant challenge to the superluminal interpretation of the OPERA data. Furthermore, we appeal to Super-Kamiokande and IceCube data to establish strong new limits on the superluminal propagation of high-energy neutrinos.

Year:  2011        PMID: 22107624     DOI: 10.1103/PhysRevLett.107.181803

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  3 in total

1.  TESTING LORENTZ SYMMETRY USING HIGH ENERGY ASTROPHYSICS OBSERVATIONS.

Authors:  Floyd W Stecker
Journal:  Symmetry (Basel)       Date:  2017-09-25       Impact factor: 2.713

2.  SEARCH FOR THE FOOTPRINTS OF NEW PHYSICS WITH LABORATORY AND COSMIC NEUTRINOS.

Authors:  Floyd W Stecker
Journal:  Mod Phys Lett A       Date:  2017-06-09       Impact factor: 2.066

Review 3.  Quantum-Spacetime Phenomenology.

Authors:  Giovanni Amelino-Camelia
Journal:  Living Rev Relativ       Date:  2013-06-12       Impact factor: 40.429

  3 in total

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