Fermion mixing in quasi-free states
arXiv:hep-th/0207268 · doi:10.1088/0305-4470/36/4/101
Abstract
Quantum field theoretic treatments of fermion oscillations are typically restricted to calculations in Fock space. In this letter we extend the oscillation formulae to include more general quasi-free states, and also consider the case when the mixing is not unitary.
10 pages, Plain TeX
References in corpus (1)
Cited by in corpus (24)
- Neutrino mixing contribution to the cosmological constant
- Dark energy and particle mixing
- Neutrinos in curved spacetimes: particle mixing and flavor oscillations
- Decoherent Neutrino Mixing, Dark Energy and Matter-Antimatter Asymmetry
- Dark energy, cosmological constant and neutrino mixing
- Neutrino oscillations from relativistic flavor currents
- Time-energy uncertainty relation for neutrino oscillations in curved spacetime
- Neutrino mixing, flavor states and dark energy
- Revealing neutrino nature and violation with decoherence effects
- Casimir effect for mixed fields
- Flavor Energy uncertainty relations for neutrino oscillations in quantum field theory
- Neutrino mixing and Lorentz invariance
- Mixing and oscillations of neutral particles in Quantum Field Theory
- On flavor conservation in weak interaction decays involving mixed neutrinos
- Dynamical generation of field mixing via flavor vacuum condensate
- Probing dark matter and quantum field theory effects with Rydberg atoms
- Beyond the MSW effect: Neutrinos in a dense medium
- Some non-trivial aspects of Poincaré and CPT invariance of flavor vacuum
- Time-to-space conversion in quantum field theory of flavor mixing
- On the flavor/mass dichotomy for mixed neutrinos: a phenomenologically motivated analysis based on lepton charge conservation in neutron decay
- Time-energy uncertainty relation for neutrino oscillations: historical development, applications and future prospects
- Fermion mixing in curved spacetime
- On the degeneracies of the mass-squared differences for three-neutrino oscillations
- Particle mixing as possible explanation of the dark energy conundrum