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arXiv:astro-ph/9912463 (astro-ph)
[Submitted on 22 Dec 1999 (v1), last revised 29 Jan 2000 (this version, v2)]

Title:Kinetically Driven Quintessence

Authors:Takeshi Chiba, Takahiro Okabe, Masahide Yamaguchi
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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 $w=p/\rho <-1$.
Comments: 18 pages, minor changes, to be published in Physical Review D
Subjects: Astrophysics (astro-ph); High Energy Physics - Phenomenology (hep-ph)
Report number: UTAP-352
Cite as: arXiv:astro-ph/9912463
  (or arXiv:astro-ph/9912463v2 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/9912463
arXiv-issued DOI via DataCite
Journal reference: Phys.Rev.D62:023511,2000
Related DOI: https://doi.org/10.1103/PhysRevD.62.023511
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Submission history

From: Takeshi Chiba [view email]
[v1] Wed, 22 Dec 1999 12:12:41 UTC (34 KB)
[v2] Sat, 29 Jan 2000 04:38:58 UTC (34 KB)
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