Fixed points and FLRW cosmologies: Flat case [PDF]
We use phase space method to study possible consequences of fixed points in flat FLRW models. One of these consequences is that a fluid with a finite sound speed, or a differentiable pressure, reaches a fixed point in an infinite time and has no finite-time singularities of types I, II and III described in hep-th/0501025.
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Dynamics and constraints of the unified dark matter flat cosmologies [PDF]
Spyros Basilakos +1 more
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Is There a Flatness Problem in Classical Cosmology? [PDF]
I briefly review the flatness problem within the context of classical cosmology and examine some of the debate in the literature with regard to its definition and even the question whether it exists. I then present some new calculations for cosmological models which will collapse in the future; together with previous work by others for models which ...
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100 years of mathematical cosmology: Models, theories and problems, Part B. [PDF]
Cotsakis S, Yefremov AP.
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Holographic dark energy with time depend gravitational constant in the non-flat Hořava-Lifshitz cosmology [PDF]
Ali Aghamohammadi +2 more
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Publisher’s Note: Fixed points and FLRW cosmologies: Flat case [Phys. Rev. D87, 103001 (2013)PRVDAQ1550-7998] [PDF]
Adel Awad
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Constraints on Non-Flat Starobinsky f(R) Dark Energy Model. [PDF]
Geng CQ, Hsu YT, Lu JR.
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When can we compute analytically lookback time, age of the universe, and luminosity distance? [PDF]
Jose S, Leblanc A, Faraoni V.
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Global existence of solutions to the Einstein-massive scalar field equations with a cosmological constant for a perfect fluid on the flat Robertson-Walker space-time [PDF]
Alexis Nangue
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Proposed physical mechanism that gives rise to cosmic inflation. [PDF]
Law BM.
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