Testing Lorentz invariance with neutrino bursts from supernova neutronization
arXiv:1211.7069 · doi:10.1103/PhysRevD.87.017302
Abstract
Quantum-gravity (QG) effects might generate Lorentz invariance violation by the interaction of energetic particles with the foamy structure of the space-time. As a consequence, particles may not travel at the universal speed of light. We propose to constrain Lorentz invariance violation for energetic neutrinos exploiting the neutronization burst from the next galactic supernova (SN). This prompt signal is expected to produce a sharp peak in the SN light curve with a duration of ms. However presence of energy-dependent Lorentz invariance violation would significantly spread out the time structure of this signal. We find that the detection the SN burst from a typical galactic explosion at kpc in a Mton-class water Cerenkov detector, would be sensitive to a quantum-gravity mass scale GeV ( GeV) for the linear (quadratic) energy dependence of Lorentz invariance violation. These limits are rather independent of the neutrino mass hierarchy and whether the neutrino velocity is super or subluminal.
4 pages, 3 figures, Revised version. Minor changes. Matches published version
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- Phenomenological Effects of CPT and Lorentz Invariance Violation in Particle and Astroparticle Physics
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