Models of dynamical supersymmetry breaking and quintessence

Abstract

We study several models of relevance for the dynamical breaking of supersymmetry which could provide a scalar component with equation of state $p=w\rho$, $-1<w<0$. Such models would provide a natural explanation for recent data on the cosmological parameters.

4 pages, Latex

References in corpus (3)

• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• A Search for Time Variation of the Fine Structure Constant
• Stabilizing the Dilaton in Superstring Cosmology

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