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arxiv: hep-th/0204070 · v3 · submitted 2002-04-08 · ✦ hep-th · astro-ph· gr-qc· hep-ph

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Inflation from a Tachyon Fluid?

Malcolm Fairbairn , Michel H.G. Tytgat (ULB)
Authors on Pith no claims yet
classification ✦ hep-th astro-phgr-qchep-ph
keywords tachyoninflationanalyseconditionsdominatedearlyevolutionfield
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Motivated by recent works of Sen and Gibbons, we study the evolution of a flat and homogeneous universe dominated by tachyon matter. In particular, we analyse the necessary conditions for inflation in the early roll of a single tachyon field.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway

    astro-ph.CO 2026-04 unverdicted novelty 4.0

    Einstein-Gauss-Bonnet corrections with exponential or sech couplings shift quintessential inflation into the 1 sigma ACT region for r and ns, while tanh coupling remains disfavored.