The universe dominated by the extended Chaplygin gas

DOI10.1142/S0217732315500704zbMath1314.83056arXiv1502.01189OpenAlexW2055765133MaRDI QIDQ5252723

E. O. Kahya, Behnam Pourhassan

Publication date: 3 June 2015

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1502.01189

zbMATH Keywords

cosmologydark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Classical and relativistic thermodynamics (80A10)

Related Items (13)

Thermodynamics of modified cosmic Chaplygin gas ⋮ A cosmological model of the early universe based on ECG with variable \(\Lambda\)-term in Lyra geometry ⋮ Chaplygin-gas solutions of f(R) gravity ⋮ Simple waves for two-dimensional magnetohydrodynamics with extended Chaplygin gas ⋮ Future stability of the FLRW spacetime for a large class of perfect fluids ⋮ Nonlinear stability of self-gravitating irrotational Chaplygin fluids in a FLRW geometry ⋮ Thin tubes of a massless scalar field as a possible source of dark energy ⋮ Interacting modified Chaplygin gas in f(T) gravity framework and analysis of its stability against gravitational perturbation ⋮ Behavior of Riemann solutions of extended Chaplygin gas under the limiting condition ⋮ Deformation of the quintom cosmological model and its consequences ⋮ Modified Chaplygin gas equation of state on viscous dissipative extended holographic Ricci dark energy and the cosmological consequences ⋮ A note on the relations between thermodynamics, energy definitions and Friedmann equations ⋮ Holographic Dark Energy with Extended Chaplygin Gas Model

Cites Work

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