- Gain assisted superluminal light propagation driver#
- Gain assisted superluminal light propagation code#
- Gain assisted superluminal light propagation free#
Sterile Neutrino Production Through a Matter Effect Enhancement at Long Baselines Our "brane" (spacetime hypersurface) and wander in the "bulk" (hyperspace).
Gain assisted superluminal light propagation free#
In flavourless "sterile" neutrinos, which in certain models are free to leave Perhaps these oscillations can also result Various flavour and mass eigenstates in a manner resonantly enhanced when theyĪre slowed passing through matter. "solar-neutrino problem") is the hypothesis that neutrinos oscillate between The basis of many neutrino-detection schemes (and the accepted solution to the famous Light Cone Reflection and the Spectrum of Neutrinos Neutrino Velocity and the Variability of Fundamental Constants Kappa-Poincaré phase space: speed of massless particlesĭouble Special Relativity with a minimum speed and the Uncertainty Principle Argues that spacetime is both non-differentiable and What if Superluminal Neutrinos Exist but not Higgs Bosons? The deformation-stability fundamental length and deviations from c Noncommutative model: Phenomenology and Quantum properties Photon-neutrino interaction in theta-exact covariant The OPERA Superluminal Neutrinos from Deformed Lorentz Invarianceĭispersion Relations Explaining OPERA Data From Deformed Lorentz Transformation Įven in the limit of infinitely small noncommutativity" "We find our deformed dispersion relation toīe capable to account for the recent results. Neutrino propagation in noncommutative spacetimes Speed of particles and a relativity of locality in kappa-Minkowski quantum spacetimeĬomplement to Special Relativity at Superluminal Speeds: Cern Neutrinos ExplainedĪ note on superluminal neutrinos and deformed special relativity Taming nonlocality in theories with Planck-scale-deformed Lorentz symmetry Violation in a Finslerian Geometrical Model Neutrino Oscillations and Lorentz Invariance Neutrino fluxes in the presence of LIV-induced energy losses."
Gain assisted superluminal light propagation code#
We simulate via detailed Monte Carlo code the propagation of cosmogenic Observation of predicted fluxes from several mainstream cosmogenic neutrino models, and specifically those recentlyĬonstrained by the ANITA and RICE experiments. We derive the implied level of LIV required to suppress (Coleman-Glashow Lorentz-invariance) in the neutrino sector. "We show that future observations of cosmogenic neutrinos will provide by far the most stringent limit on LIV Implications of ultra-high energy neutrino flux constraints for Lorentz-invariance violating cosmogenic neutrinos Particle-dependent deformations of Lorentz symmetryĮxtended Lorentz code of a superluminal particle Superluminal neutrinos and the Standard Model Superluminal neutrino, flavor, and relativity OPERA, SN1987a and energy dependence of superluminal neutrino velocity Limiting velocities as running parameters and superluminal neutrinos The Hypothesis of Superluminal Neutrinos: comparing OPERA with other Dataīeyond the speed of light on Finsler spacetimesīy Christian Pfeifer and Mattias N. OPERA-reassessing data on the energy dependence of the speed of neutrinos Coleman-Glashow Proposal: Different particles see different speeds of light.In addition to presenting the authors' own ideas about faster-than-light particles, provides an introduction to the condensed-matter-analogy approach to special relativity. Is an approximation to the theory of an underlying medium? Properties of the medium) can also behave in ways which a relativistic particle cannot. Motion resembling those of special relativity, but (for reasons connected with the microscopic Analogy with Condensed-Matter Physics: Moving dislocations obey equations of.Neutrinos as probes of Lorentz invariance Propagation of Superluminal PeV IceCube Neutrinos:Ī High Energy Spectral Cutoff or New Constraints on
Gain assisted superluminal light propagation driver#
Right-handed to an even faster driver who passes them on the highway. The "Autobahn Paradox" is the fact that subluminal neutrinos are supposed to be necessarily left-handed, but would appear The Phantom of the OPERA: Superluminal NeutrinosĪn Infinitesimally Superluminal Neutrino is Left-Handed, Conserves Lepton Number and Solves the Autobahn Paradox (Illustrative Discussion) Neutrino Tests of General and Special Relativity Neutrino velocity as a test of special relativity. The speed of light and the speed of neutrinos Is the right-handed Majorana neutrino a tachyon? Written in part to supplyĮarlier references overlooked by Chodos et al. Theories with Neutrino Speed Greater Than Light SpeedĪ comment on fermionic tachyons and Poincaré representationsĪre muon neutrinos faster-than-light particles?