Quintessential inflation with dissipative fluid

DOI10.1023/A:1015536623936zbMath1005.83045arXivgr-qc/0005104MaRDI QIDQ1604893

Indrajit Chakrabarty, T. R. Seshadri, Anjan Ananda Sen

Publication date: 9 July 2002

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0005104

zbMATH Keywords

inflationcosmologyself-interacting scalar fielddissipative fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (2)

TACHYON FIELD-INSPIRED DARK ENERGY AND SUPERNOVAE CONSTRAINTS ⋮ Interacting holographic dark energy in Bianchi type-V and IX universes with variable deceleration parameter

Cites Work

• Cosmological Inflation and Large-Scale Structure
• Cosmological models arising from generalized scalar field potentials
• Cosmological Imprint of an Energy Component with General Equation of State

This page was built for publication: Quintessential inflation with dissipative fluid