Accelerating cold dark matter cosmology (Ω Λ ≡ 0)

DOI10.1088/0264-9381/25/20/205006zbMath1152.83427arXiv0807.3379OpenAlexW2599283816MaRDI QIDQ3535559

No author found.

Publication date: 13 November 2008

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0807.3379

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items

Friedmann cosmology with matter creation in modified \(f(R,T)\) gravity ⋮ Why Noether symmetry of \(F(R)\) theory yields three-half power law? ⋮ Conformally related metrics and Lagrangians and their physical interpretation in cosmology ⋮ Fermion creation in 5D space–time with a warped extra dimension ⋮ Will there be future deceleration? A study of particle creation mechanism in nonequilibrium thermodynamics ⋮ Finite-time cosmological singularities and the possible fate of the universe ⋮ Accelerated expansion of the universe based on particle creation-destruction processes and dark energy in FLRW universes ⋮ Numerical solutions to the cosmological 3-fluid problem ⋮ A cosmological model of thermodynamic open universe ⋮ Schwinger effect in a Robertson-Walker space-time ⋮ Stability of a modified Jordan-Brans-Dicke theory in the dilatonic frame ⋮ On quintessential cosmological models and exponential potentials ⋮ Note on ``Continuous matter creation and the acceleration of the universe: the growth of density fluctuations ⋮ Interacting new generalized Chaplygin gas ⋮ Particle creation in Friedmann-Robertson-Walker universe ⋮ ON THE CREATION OF SCALAR PARTICLES IN A FLAT ROBERTSON–WALKER SPACETIME