A solution to the anisotropy problem in bouncing cosmologies
arXiv:0909.5611 · doi:10.1088/1475-7516/2009/10/014
Abstract
Bouncing cosmologies are often proposed as alternatives to standard inflation for the explanation of the homogeneity and flatness of the universe. In such scenarios, the present cosmological expansion is preceded by a contraction phase. However, during the contraction, in general the anisotropy of the universe grows and eventually leads to a chaotic mixmaster behavior. This would either be hard to reconcile with observations or even lead to a singularity instead of the bounce. In order to preserve a smooth and isotropic bounce, the source for the contraction must have a super-stiff equation of state with . In this letter we propose a new mechanism to solve the anisotropy problem for any low-energy value of by arguing that high energy physics leads to a modification of the equation of state, with the introduction of non-linear terms. In such a scenario, the anisotropy is strongly suppressed during the high energy phase, allowing for a graceful isotropic bounce, even when the low-energy value of is smaller than unity.
9 pages, accepted for publication in JCAP
References in corpus (16)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Brane-World Gravity
- Quantum Nature of the Big Bang
- Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
- A non inflationary model with scale invariant cosmological perturbations
- The Einstein static universe in Loop Quantum Cosmology
- Evolution to a smooth universe in an ekpyrotic contracting phase with w > 1
- Quantum nature of cosmological bounces
- DM: Observational constraints on unified dark matter with constant speed of sound
- Cosmo-dynamics and dark energy with a quadratic EoS: anisotropic models, large-scale perturbations and cosmological singularities
- Affine equation of state from quintessence and k-essence fields
- Affine parameterization of the dark sector: costraints from WMAP5 and SDSS
- Graceful exit via polymerization of pre-big bang cosmology
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- Loop Quantum Cosmology: A Status Report
- Bouncing Cosmologies: Progress and Problems
- Bouncing cosmologies with dark matter and dark energy
- An Extended Matter Bounce Scenario: current status and challenges
- Isotropic and Anisotropic Bouncing Cosmologies in Palatini Gravity
- Particle Creation in Bouncing Cosmologies
- Cuscuton gravity as a classically stable limiting curvature theory
- Reconstruction of a Nonminimal Coupling Theory with Scale-invariant Power Spectrum
- Microphysical manifestations of viscosity and consequences for anisotropies in the very early universe
- Reconstruction method of gravity for isotropic and anisotropic spacetimes
- Fine-tuning challenges for the matter bounce scenario
- Analysis of big bounce in Einstein--Cartan cosmology
- Nonsingular Cosmology from an Interacting Vacuum
- Primordial power spectrum from a matter-Ekpyrotic bounce scenario in loop quantum cosmology
- Massive gravity and the suppression of anisotropies and gravitational waves in a matter-dominated contracting universe
- Can gravity isotropize a pre-bounce contracting universe?
- Quasi-isotropic cycles and non-singular bounces in a Mixmaster cosmology
- Comments on "Growth of Covariant Perturbations in the Contracting Phase of a Bouncing Universe" by A. Kumar
- Bouncing universe with modified dispersion relation
- Observational constraints on anisotropies for bouncing alternatives to inflation
- Nonlinear anisotropy growth in Bianchi-I spacetime in metric cosmology
- Exponential correction to Friedmann equations
- Bouncing solutions from generalized EoS
- Smoking-gun signatures of bounce cosmology from echoes of relic gravitational waves
- Bouncing cosmology without anisotropy