Qualitative Stability Analysis of Cosmological Parameters in Gravity
arXiv:2211.07376 · doi:10.1140/epjc/s10052-023-11458-2
Abstract
We analyze the cosmological solutions of gravity using dynamical system analysis where is the torsion scalar and be the boundary term scalar. In our work, we assume two specific cosmological models. For first model, we consider , where and are constants. For second model, we consider . We generate an autonomous system of differential equations for each models by introducing new dimensionless variables. To solve this system of equations, we use dynamical system analysis. We also investigate the critical points and their natures, stability conditions and their behaviors of Universe expansion. For both models, we get four critical points. The phase plots of this system are analyzed in detail and study their geometrical interpretations also. In both model, we evaluated density parameters such as , , and and deceleration parameter and find their suitable range of the parameter for stability. For first model, we get and for second model, we get . This shows that both the models are in quintessence phase. Further, we compare the values of EoS parameter and deceleration parameter with the observational values.
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