Cosmological Restrictions on Conformally Invariant SU(5) GUT Models
arXiv:gr-qc/9506093 · doi:10.1088/0264-9381/10/7/007
Abstract
Dirac's theory of constrained Hamiltonian systems is applied to the minimal conformally invariant SU(5) grand-unified model studied at 1-loop level in a de Sitter universe. For this model, which represents a simple and interesting example of GUT theory and at the same time is a step towards theories with larger gauge group like SO(10), second-class constraints in the Euclidean-time regime exist. In particular, they enable one to prove that, to be consistent with the experimentally established electroweak standard model and with inflationary cosmology, the residual gauge-symmetry group of the early universe, during the whole de Sitter era, is bound to be SU(3) x SU(2) x U(1). Moreover, the numerical solution of the field equations subject to second-class constraints is obtained. This confirms the existence of a sufficiently long de Sitter phase of the early universe, in agreement with the initial assumptions.
23 pages, plain-tex, published in Classical and Quantum Gravity, volume 10, pages 1285-1297, year 1993
References in corpus (1)
Cited by in corpus (6)
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- Non-Local Properties in Euclidean Quantum Gravity
- Quantum Effects in Friedmann-Robertson-Walker Cosmologies