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arxiv: astro-ph/9912463 · v2 · submitted 1999-12-22 · 🌌 astro-ph · hep-ph

Kinetically Driven Quintessence

classification 🌌 astro-ph hep-ph
keywords kineticmodelquintessencetermscomponentdrivenequationfield
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Recently, a novel class of models for inflation has been found in which the inflationary dynamics is driven solely by (non-canonical) kinetic terms rather than by potential terms. As an obvious extension, we show that a scalar field with non-canonical kinetic terms alone behaves like an energy component which is time-varying and has negative pressure presently, i.e. quintessence. We present a model which has a constant equation of state, that is, a ``kinetic'' counterpart of the Ratra-Peebles model of a quintessence field with a potential term. We make clear the structure of the phase plane and show that the quintessential solution is a late-time attractor. We also give a model for the ``phantom'' component which has an equation of state with $w=p/\rho <-1$.

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