The hyperspin structure of Einstein universes and their neutrino spectrum
This thesis formulates and studies a sequence of homogeneous, isotropic, and compact solutions to the empty space hypergravity equations (Finkelstein 1987). These solutions are hyperspin manifolds constructed from unitary groups U{sub N}:= U(N,C) and describe the static compact N{sup 2} dimensional Einstein universes of the Kaluza-Klein type with Finslerian geometry. By taking the universal covering group of U{sub N} we obtain a manifold with topology IRxSU{sub N}, where the abelian group IR is the time axis and SU{sub N} provides a compact homogeneous spatial part. To describe the geometry of these manifolds we extend the exterior Cartan-Penrose calculus from spinors to hyperspinors and apply the Maurer-Cartan equations to obtain the hyperspin structure of U{sub N}. We present a natural extension to curved time space of the relativistic wave equations which are in general of differential order N and discuss the discrete symmetries of the hyperneutrino equation. We solve the linear neutrino equation exactly and present the energy spectra of the neutrino and antineutrino, which differ for N > 2. The neutrino acquires a negligible rest mass of O(10{sup {minus}31}eV). Our most important conclusion is that there is a consistent alternative to the usual Riemannian geometry for spaces with internal dimensions, which deserves further study.
- Research Organization:
- Georgia Inst. of Tech., Atlanta, GA (USA)
- OSTI ID:
- 5116641
- Resource Relation:
- Other Information: Thesis (Ph. D.)
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
GENERAL PHYSICS
GRAVITATIONAL FIELDS
MATHEMATICAL MODELS
CALCULATION METHODS
FIELD THEORIES
KALUZA-KLEIN THEORY
MATHEMATICAL MANIFOLDS
WAVE EQUATIONS
DIFFERENTIAL EQUATIONS
EQUATIONS
PARTIAL DIFFERENTIAL EQUATIONS
UNIFIED-FIELD THEORIES
657003* - Theoretical & Mathematical Physics- Relativity & Gravitation