Theory of neutrino oscillations using condensed matter physics Including production process and energy-time uncertainty
Harry J. Lipkin

TL;DR
This paper presents a condensed matter physics approach to neutrino oscillations, emphasizing the role of energy-time uncertainty and interference effects at short times, challenging traditional quantum field theory descriptions.
Contribution
It introduces a simplified model deriving neutrino oscillations from energy-time uncertainty and interference, providing a new perspective beyond standard relativistic quantum field theory.
Findings
Interference occurs at short times due to overlapping energy spectra.
The model's squared mass difference estimate aligns with KAMLAND results within a factor of three.
Oscillations depend on laboratory frame conditions and experimental environment.
Abstract
Neutrino scillations cannot arise from an initial isolated one particle state if four-momentum is conserved. The transition matrix element is generally squared and summed over all final states with no interference between orthogonal final states. Lorentz covariant descriptions based on relativistic quantum field theory cannot describe interference between orthogonal states with different masses producing neutrino oscillations. Simplified model presents rigorous derivation of handwaving argument about "energy-time uncertainty". Standard time-dependent perturbation theory for decays shows how energy spectrum of final state is much broader than natural line width at times much shorter than decay lifetime. Initial state containing two components with different energies decay into two orthogonal states with different masses completely separated at long times with no interference.…
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Taxonomy
TopicsNeutrino Physics Research · Dark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies
