Neutrino propagation in matter with general interactions
- 8 October 1999
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 60 (9) , 093008
- https://doi.org/10.1103/physrevd.60.093008
Abstract
We present a general analysis of the effective potential for neutrino propagation in matter, assuming a generic set of Lorentz invariant non-derivative interactions. We find that in addition to the known vector and axial vector terms, in a polarized medium also tensor interactions can play an important role. We compute the effective potential arising from a tensor interaction. We show that the components of the tensor potential transverse to the direction of the neutrino propagation can induce a neutrino spin flip, similar to the one induced by a transverse magnetic field.Keywords
All Related Versions
This publication has 40 references indexed in Scilit:
- Where do we stand with solar neutrino oscillations?Physical Review D, 1998
- Study of the atmospheric neutrino flux in the multi-GeV energy rangePhysics Letters B, 1998
- Chirality-preserving neutrino oscillations in an external magnetic fieldPhysics Letters B, 1996
- How well do we (and will we) know solar neutrino fluxes and oscillation parameters?Physical Review D, 1996
- Search for muon neutrino oscillations with the Irvine-Michigan-Brookhaven detectorPhysical Review Letters, 1992
- Solar-neutrino solutions with matter-enhanced flavor-changing neutral-current scatteringPhysical Review D, 1991
- Field-theoretic derivation of Wolfenstein's matter-oscillation formulaPhysical Review D, 1989
- Magnetic properties of strongly asymmetric nuclear matterPhysics Letters B, 1989
- Resonant spin-flavor precession of solar and supernova neutrinosPhysical Review D, 1988
- ,, andphases, and their effects, in Majorana-particle processesPhysical Review D, 1984