Dirac’s theory of constrained Hamiltonian systems is applied to the minimal conformally invarianl SU(5) grand-unified model studied at one-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 constrains 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 phase 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.
Cosmological restrictions on conformally invariant SU(5) GUT models / Esposito, G.; Miele, Gennaro; Rosa, Luigi. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - STAMPA. - 10:7(1993), pp. 1285-1297. [10.1088/0264-9381/10/7/007]
Cosmological restrictions on conformally invariant SU(5) GUT models
G. EspositoPrimo
;MIELE, GENNAROSecondo
;ROSA, LUIGIUltimo
1993
Abstract
Dirac’s theory of constrained Hamiltonian systems is applied to the minimal conformally invarianl SU(5) grand-unified model studied at one-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 constrains 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 phase 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.| File | Dimensione | Formato | |
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