Sound Speed in Extended Chaplygin Fluid
arXiv:2101.10851 · doi:10.1016/j.newast.2021.101569
Abstract
We consider an extended Chaplygin gas equation of state which is driven from D-brane action and construct a cosmological model based on this equation of state. In this regard, we compute the scale factor of the model under a certain approximation. The conservation equation of this case is a non-linear differential equation which should solve using the special conditions. We also analyze the stability of the model by using sound speed as well as adiabatic index and discuss certain special cases of the model. We find special equation of state in this model which yields to dynamical and thermodynamical stability. Furthermore, we study the cosmological consequences of this model under certain conditions.
arXiv comment14 pages, 10 figures, Published in New Astronomy
References in corpus (22)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- An alternative to quintessence
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- Accelerated Universe from Gravity Leaking to Extra Dimensions
- Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
- Role of Modified Chaplygin Gas in Accelerated Universe
- The end of unified dark matter?
- WMAP Constraints on the Generalized Chaplygin Gas Model
- Constraints on the generalized Chaplygin gas from supernovae observations
- You need not be afraid of phantom energy
- Quintessence and Scalar Dark Matter in the Universe
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
- Cosmology with a Variable Chaplygin Gas
- Viscous Modified Cosmic Chaplygin Gas Cosmology
- FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
- Chaplygin-like gas and branes in black hole bulks
- A Note on Classical Solution of Chaplygin-gas as D-brane
- Galileo invariant system and the motion of relativistic d-branes
- The universe dominated by the extended Chaplygin gas
- Viscous dissipative Chaplygin gas dominated homogenous and isotropic cosmological models
- Constructing an Inflaton Potential by Mimicking Modified Chaplygin Gas