Table 3 Cosmological implications of the equilibriums.
From: Dynamical system analysis of FLRW models with Modified Chaplygin gas
F | Flat Friedmann solution | Matter dominated flat universe |
dS | de Sitter Solution | \(\Lambda\) dominated flat universe |
M | Milne solution | The universe with maximum negative curvature |
E | Einstein static solution | Static universe with maximum positive curvature |
CH | Chaplygin gas solution | Chaplygin gas and matter dominated flat universe |
CD | Chaplygin-de Sitter solution line | Pressureless flat universes |
