Reheating in tachyonic inflationary models: Effects on the large scale curvature perturbations

DOI10.1016/J.NUCLPHYSB.2011.07.003zbMath1229.83082arXiv0902.1067OpenAlexW2156888491MaRDI QIDQ659294

L. Sriramkumar, Pravabati Chingangbam, Rajeev Kumar Jain

Publication date: 18 January 2012

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

Full work available at URL: https://arxiv.org/abs/0902.1067

zbMATH Keywords

reheatinginflationary modelscosmological perturbation theory

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (3)

Irreversible thermodynamic description of dark matter and radiation creation during inflationary reheating ⋮ Power spectra in extended tachyon cosmologies ⋮ Cosmological perturbations in warm-tachyon inflationary universe model with viscous pressure

Cites Work

• Evolution of primordial perturbations and a fluctuating decay rate
• WARM INFLATION MODEL BUILDING
• WARM TACHYONIC INFLATION IN A WARPED BACKGROUND

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