Quantized De Sitter space, the connection to the Pauli principle and an application to Feynman's relativistic quark theory. II
BS>A model of a quantized space-time theory was investigated previously. Consideration is given to further problems of a quartized De Sitter space. It is shown that a De Sitter space is a very useful starting point to a nonlocal relativistic quartum field theory, containing the Pauli principle, for the theory of elemertary particles, as a connection to Feynman's relativistic quark theory, where the group SU(3) has a particular importance. This method offers the possibtlity of treating weak local differences from a space with De Sitter metric as a perturbation. Therefore the problem of a fundamental elementary length 1/ sub 0/ must be considered in connection with the general theory of relativity. (auth)
- Research Organization:
- Univ., Stuttgart
- NSA Number:
- NSA-29-016945
- OSTI ID:
- 4360083
- Journal Information:
- Int. J. Theor. Phys., v. 8, no. 3, pp. 199-209, Journal Name: Int. J. Theor. Phys., v. 8, no. 3, pp. 199-209; ISSN IJTPB
- Country of Publication:
- United Kingdom
- Language:
- English
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*GENERAL RELATIVITY THEORY-- ELEMENTARY LENGTH
*PAULI PRINCIPLE-- DE SITTER GROUP
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ELEMENTARY PARTICLES
FEYNMAN DIAGRAM
MATHEMATICAL SPACE
METRICS
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N76300 --Physics (Theoretical)--Gravitation & General Relativity
PARTICLE MODELS
PERTURBATION THEORY
QUANTUM MECHANICS
QUARKS
SPACE-TIME
SPINORS
SU-3 GROUPS