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Dynamical system analysis of FLRW models with Modified Chaplygin gas
Ali Osman Yılmaz1, Ertan Güdekli2
1Department of Physics, Istanbul University, Istanbul, 34134, Turkey.
This study analyzes Friedmann-Lemaître-Robertson-Walker (FLRW) cosmological models with modified Chaplygin gas and a cosmological constant. We explore the universe
Area of Science:
- Cosmology
- Theoretical Physics
- General Relativity
Background:
- The standard cosmological model faces challenges explaining dark energy.
- Modified Chaplygin gas offers an alternative dark energy candidate.
- Cosmological constant remains a key component in understanding cosmic acceleration.
Purpose of the Study:
- To investigate Friedmann-Lemaître-Robertson-Walker (FLRW) models incorporating modified Chaplygin gas and a cosmological constant.
- To analyze the stability and evolution of these cosmological models using dynamical system methods.
- To determine the long-term fate of the universe under these conditions.
Main Methods:
- Application of dynamical system analysis to FLRW cosmological models.
- Investigation of the equation of state for modified Chaplygin gas: p = (α - 1)ρ/α.
- Analysis of state spaces to understand model singularities and future evolution.
Main Results:
- The study maps the state spaces for various parameter values.
- It identifies conditions for stable and unstable solutions.
- The analysis reveals the universe's potential future evolution, including possible singularities.
Conclusions:
- Certain configurations of modified Chaplygin gas and cosmological constant allow for stable cosmic evolution.
- The presence of a singularity at the beginning of the universe is confirmed in some scenarios.
- The long-term fate of the universe depends critically on the chosen parameters.
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