Search results for "Big Rip"

showing 3 items of 3 documents

Unduland universe: expansion with alternating eras of acceleration and deceleration

2005

If the equation of state for 'dark energy' varies periodically, the expansion of the Universe may have undergone alternating eras of acceleration and deceleration. We examine a specific form that survives existing observational tests, does not single out the present state of the Universe as exceptional, and suggests a future much like the matter-dominated past: a smooth expansion without a final inflationary epoch.

PhysicsNuclear and High Energy PhysicsCosmologiaSteady State theoryBig RipAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsParticle horizonMetric expansion of spaceDe Sitter universeDark energyInflationary epochScale factor (cosmology)
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Dark energy cosmologies for codimension-two branes

2005

A six-dimensional universe with two branes in the "football-shaped" geometry leads to an almost realistic cosmology. We describe a family of exact solutions with time dependent characteristic size of internal space. After a short inflationary period the late cosmology is either of quintessence type or turns to a radiation dominated Friedmann universe where the cosmological constant appears as a free integration constant of the solution. The radiation dominated universe with relativistic fermions is analyzed in detail, including its dimensional reduction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBig RipFOS: Physical sciencesNon-standard cosmologyLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsMetric expansion of spaceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyScale factor (cosmology)
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Constraining inverse-curvature gravity with supernovae

2005

We show that the current accelerated expansion of the Universe can be explained without resorting to dark energy. Models of generalized modified gravity, with inverse powers of the curvature can have late time accelerating attractors without conflicting with solar system experiments. We have solved the Friedman equations for the full dynamical range of the evolution of the Universe. This allows us to perform a detailed analysis of Supernovae data in the context of such models that results in an excellent fit. Hence, inverse curvature gravity models represent an example of phenomenologically viable models in which the current acceleration of the Universe is driven by curvature instead of dar…

High Energy Physics - TheoryPhysicsPhantom energyAstrophysics (astro-ph)FOS: Physical sciencesGeneral Physics and AstronomyBig RipGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyParticle horizonMetric expansion of spaceTheoretical physicsHigh Energy Physics - Theory (hep-th)De Sitter universeZero-energy universeFlatness problemScale factor (cosmology)
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