New cosmological solutions and stability analysis in full extended thermodynamics
Luis P. Chimento, Alejandro S. Jakubi, Vicenç Méndez
Abstract
The Einstein's field equations of FRW universes filled with a dissipative fluid described by full theory of causal transport equations are analyzed. New exact solutions are found using a non-local transformations on the nonlinear differential equation for the Hubble factor. The stability of the de Sitter and asymptotically friedmannian solutions are analyzed using Lyapunov function method.
Create a lesson
Related papers
Non-Commutativity in Geodesic Congruences
Aarav Shah, Louis H. Kauffman
Scalar wave dark matter imprints on binary black hole mergers: dependence on field mass and density
Yu-Peng Zhang, Shao-Wen Wei, Yu-Xiao Liu
Quantum Energy Inequalities with a twist: rotating frames along stationary worldlines
Christopher J. Fewster, Daniel Lomax Ford
Analytic Electromagnetic Effective Source for Geodesic Orbit in Schwarzschild Spacetime
Xuchen Lu, Yungui Gong, Bokai Zhang et al.
Stability conditions for light rings in circular stationary axisymmetric spacetimes
Jake O. Shipley
Post-Newtonian secular dynamics of hierarchical triples II. Canonical derivation of the 1PN\,×\,quadrupole cross terms and of the quadrupole-squared term
Hideyoshi Arakida