Interacting closed string tachyon with generalized cosmic Chaplygin gas
From MaRDI portal
Publication:2931896
DOI10.1142/S0219887814500650zbMath1303.81137MaRDI QIDQ2931896
A. R. Amani, Behnam Pourhassan
Publication date: 28 November 2014
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Model quantum field theories (81T10) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30)
Related Items (2)
Self-gravitating gaseous spheres in 5D framework ⋮ Thermodynamics of the viscous f(T,B) gravity in the new agegraphic dark energy model
Cites Work
- Viscous varying generalized Chaplygin gas with cosmological constant and space curvature
- Effect of varying bulk viscosity on generalized Chaplygin gas
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Cosmological constant -- the weight of the vacuum
- Viscous generalized Chaplygin gas with arbitrary \(\alpha\)
- Viscous Chaplygin gas in non-flat universe
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Dynamics of interacting generalized cosmic Chaplygin gas in brane-world scenario
- Interacting two-component fluid models with varying EoS parameter
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Role of modified Chaplygin gas in accelerated universe
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- An alternative to quintessence
This page was built for publication: Interacting closed string tachyon with generalized cosmic Chaplygin gas
