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      Kinetically Driven Quintessence

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          Abstract

          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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          Author and article information

          Journal
          22 December 1999
          2000-01-28
          Article
          10.1103/PhysRevD.62.023511
          astro-ph/9912463
          ef7e1457-1b29-4f32-9924-e65b19a2b569
          History
          Custom metadata
          UTAP-352
          Phys.Rev.D62:023511,2000
          18 pages, minor changes, to be published in Physical Review D
          astro-ph hep-ph

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