Cosmological perturbations in warm-tachyon inflationary universe model with viscous pressure

DOI10.1016/J.PHYSLETB.2014.07.008zbMath1317.83083arXiv1407.2604OpenAlexW2027998221MaRDI QIDQ2356362

Vahid Kamali, Mohammad R. Setare

Publication date: 29 July 2015

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1407.2604

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30) Kaluza-Klein and other higher-dimensional theories (83E15)

Related Items (5)

Analysing Hessence intermediate and logamediate universe in loop quantum cosmological background ⋮ On the consistency of tachyon warm inflation with viscous pressure ⋮ Constant-roll inflation driven by q-de Sitter ⋮ Constant roll warm inflation in high dissipative regime ⋮ Warm gauge-flation with general dissipative coefficient

Cites Work

• Unnamed Item
• Reheating in tachyonic inflationary models: Effects on the large scale curvature perturbations
• Inflation from a tachyon fluid?
• Cosmological evolution of the rolling tachyon
• WARM INFLATION MODEL BUILDING
• WARM TACHYONIC INFLATION IN A WARPED BACKGROUND
• \(k\)-inflation
• Density perturbations in warm inflation and COBE normalization

This page was built for publication: Cosmological perturbations in warm-tachyon inflationary universe model with viscous pressure