Published February 1992 | Version v1
Journal article

Topological geometrodynamics and the solar neutrino problem

  • 1. Univ. of Helsinki (Finland)
  • 2. Univ. of Oulu (Finland)

Description

A solution of the solar neutrino problem based on certain differences between T(opological) G(eometro) D(ynamics) and the standard model of the electroweak interactions is proposed. First, TGD predicts the existence of a right-handed neutrino inert with respect to ordinary electroweak interactions. Second, the generalization of the massless Dirac equation contains terms mixing different M4 chiralities, unlike the ordinary massless Dirac equation. This and the observation of anticorrelations of the solar neutrino flux with sunspot number suggest that solar neutrinos are transformed to right-handed neutrinos on the convective zone of the Sun. Third, the compactness of CP2 implies topological field quantization: space-time decomposes into regions, topological field quanta, characterized by a handful of vacuum quantum numbers. In particular, there are topological obstructions for the smooth global imbeddings of magnetic fields and the decomposition of the solar magnetic field into flux tubes is predicted. Finally, every electromagnetically neutral mass distribution is accompanied by a long-range Z0 vacuum field. If the vacuum quantum numbers inside the flux tubes of the solar magnetic field are considerably smaller than in the normal phase, the Z0 electric force becomes strong and implies Thomas precession for the spin of the left-handed component of the neutrino. As a consequence, left-handed neutrinos are transformed to right-handed ones and the process is irreversible, since right-handed neutrinos do not couple to Z0. 17 refs., 2 figs

Additional details

Publishing Information

Journal Title
International Journal of Theoretical Physics
Journal Volume
31
Journal Issue
2
Journal Page Range
p. 245-267.
ISSN
0020-7748
CODEN
IJTPBM