The universe dominated by the extended Chaplygin gas
E.O. Kahya, B. Pourhassan

TL;DR
This paper investigates a universe dominated by the extended Chaplygin gas, analyzing its stability through density perturbations and thermodynamics, and confirming its viability as a cosmological model.
Contribution
It introduces the second order extended Chaplygin gas model and demonstrates its stability without phase transitions or critical points.
Findings
Model is stable in relativistic and Newtonian regimes
No phase transition or critical point observed
Thermodynamic analysis confirms stability
Abstract
In this paper, we consider a universe dominated by the extended Chaplygin gas which recently proposed as the last version of Chaplygin gas models. Here, we only consider the second order term which recovers quadratic barotropic fluid equation of state. The density perturbations analyzed in both relativistic and Newtonian regimes and show that the model is stable without any phase transition and critical point. We confirmed stability of the model using thermodynamics point of view.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
