Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1997-02-20
Phys.Rev. D56 (1997) 1989-2001
Physics
High Energy Physics
High Energy Physics - Phenomenology
28 pages, latex, 11 figures, submitted to Phys. Rev. D
Scientific paper
10.1103/PhysRevD.56.1989
We investigate the observable consequences of creating cosmic texture by breaking a global SU(3) symmetry, rather than the SU(2) case which is generally studied. To this end, we study the nonlinear sigma model for a totally broken SU(3) symmetry, and develop a technique for numerically solving the classical field equations. This technique is applied in a cosmological context: the energy of the collapsing SU(3) texture field is used as a gravitational source for the production of perturbations in the primordial fluids of the early universe. From these calculations, we make predictions about the appearance of the anisotropies in the cosmic microwave background radiation (CMBR) which would be present if the large scale structure of the universe was gravitationally seeded by the collapse of SU(3) textures.
Barnes Chris
Turok Neil
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