Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-05-22
Phys.Rev. D62 (2000) 123503
Physics
High Energy Physics
High Energy Physics - Phenomenology
6 pages, revised version to appear in PRD
Scientific paper
10.1103/PhysRevD.62.123503
Scalar field models of quintessence typically require that the expectation value of the field today is of order the Planck mass, if we want them to explain the observed acceleration of the Universe. This suggests that we should be considering models in the context of supergravity. We discuss a particular class of supergravity models and analyze their behavior under different choices of the Kahler metric.
Copeland Edmund J.
Nunes Nelson J.
Rosati Francesca
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