Dynamical system analysis of logotropic dark fluid with a power law in the rest-mass energy density
Preprint
Abstract
We consider a spatially flat FLRW universe. We assume that it is filled with dark energy in the form of logotropic dark fluid coupled with dark matter in the form of a perfect fluid having a barotropic equation of state. We employ dynamical system tools to obtain a complete qualitative idea of the evolution of such a universe. It is interesting to note that we ought to consider an approximation for the pressure of the logotropic dark fluid in the form of an infinite series so as to be able to construct the autonomous system required for a dynamical system study. This series form provides us with a power law in the rest-mass energy density of the logotropic dark fluid. We compute the critical points of the autonomous system and analyze these critical points by applying linear stability theory. Our analysis reveal a scenario of late-time accelerated universe dominated by the logotropic fluid which behaves as cosmological constant, preceded by an intermediate phase of the Universe dominated by logotropic fluid which behaves as dark matter in the form of perfect fluid. Moreover, it also crosses the phantom divide line.Keywords
All Related Versions
This publication has 45 references indexed in Scilit:
- Autonomous dynamical system of Einstein–Gauss–Bonnet cosmologiesAnnals of Physics, 2020
- Generalized logarithmic equation of state in classical and loop quantum cosmology dark energy–dark matter coupled systemsAnnals of Physics, 2019
- Dynamical systems applied to cosmology: Dark energy and modified gravityPhysics Reports, 2018
- The Logotropic Dark Fluid as a unification of dark matter and dark energyPhysics Letters B, 2016
- Dynamics of dark energy with a coupling to dark matter2009
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: Observational constraintsAstronomy & Astrophysics, 2004
- Cosmological constant—the weight of the vacuumPhysics Reports, 2003
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gasPhysics Letters B, 2002
- Letter: Density Perturbations in a Universe Dominated by the Chaplygin GasGeneral Relativity and Gravitation, 2002
- An alternative to quintessencePhysics Letters B, 2001