English

Warm inflationary model in loop quantum cosmology

Cosmology and Nongalactic Astrophysics 2014-11-21 v1 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

A warm inflationary universe model in loop quantum cosmology is studied. In general we discuss the condition of inflation in this framework. By using a chaotic potential, V(ϕ)ϕ2V(\phi)\propto \phi^2, we develop a model where the dissipation coefficient Γ=Γ0=\Gamma=\Gamma_0= constant. We use recent astronomical observations for constraining the parameters appearing in our model.

Keywords

Cite

@article{arxiv.1006.1299,
  title  = {Warm inflationary model in loop quantum cosmology},
  author = {Ramon Herrera},
  journal= {arXiv preprint arXiv:1006.1299},
  year   = {2014}
}

Comments

15 pages, 1 figure, Accepted for publication in Phys. Rev. D

R2 v1 2026-06-21T15:32:53.896Z