Tachyon warm inflationary universe models

Ramón Herrera, Sergio Del Campo, Cuauhtemoc Campuzano

Research output: Contribution to journalReview articlepeer-review

66 Scopus citations


Warm inflationary universe models in a tachyon field theory are studied. General conditions required for these models to be realizable are derived and discussed. We describe scalar perturbations (in the longitudinal gauge) and tensor perturbations for these scenarios. We develop our models for a constant dissipation parameter Γ in one case and one dependent on φ in the other case. We have been successful in describing such inflationary universe models. We use recent astronomical observations for constraining the parameters appearing in our model. Also, our results are compared with their analogues found in the cool inflationary case.

Original languageEnglish
Article number009
JournalJournal of Cosmology and Astroparticle Physics
Issue number10
StatePublished - 1 Oct 2006


  • Cosmological perturbation theory
  • Cosmology of theories beyond the SM
  • Inflation
  • Physics of the early universe


Dive into the research topics of 'Tachyon warm inflationary universe models'. Together they form a unique fingerprint.

Cite this