Dark energy, matter creation and curvature
arXiv:1208.6505 · doi:10.1140/epjc/s10052-012-2149-0
Abstract
The most studied way to explain the current accelerated expansion of the universe is to assume the existence of dark energy; a new component that fill the universe, does not clumps, currently dominates the evolution, and has a negative pressure. In this work I study an alternative model proposed by Lima et al. \cite{lima96}, which does not need an exotic equation of state, but assumes instead the existence of gravitational particle creation. Because this model fits the supernova observations as well as the CDM model, I perform in this work a thorough study of this model considering an explicit spatial curvature. I found that in this scenario we can alleviate the cosmic coincidence problem, basically showing that these two components, dark matter and dark energy, are of the same nature, but they act at different scales. I also shown the inadequacy of some particle creation models, and also I study a previously propose new model that overcome these difficulties.
6 pages, 4 figures. Accepted for publication in EPJC. arXiv admin note: substantial text overlap with arXiv:0812.3865
References in corpus (28)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- An alternative to quintessence
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Coupled Quintessence
- Cosmological Results from High-z Supernovae
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Interacting Quintessence
- Interacting quintessence solution to the coincidence problem
- The end of unified dark matter?
- Bulk Viscous Cosmology
- Cosmic anti-friction and accelerated expansion
- Dark energy and dark matter as curvature effects
- Tracking and coupled dark energy as seen by WMAP
- Generalized Chaplygin gas and CMBR constraints
- Are Chaplygin gases serious contenders to the dark energy throne?
- Accelerating Cold Dark Matter Cosmology ()
- CDM Accelerating Cosmology as an Alternative to LCDM model
- An Accelerating Cosmology Without Dark Energy
- Cosmological particle production, causal thermodynamics, and inflationary expansion
- Inflationary Models Driven by Adiabatic Matter Creation
- Phantom damping of matter perturbations
- Strategies for Determining the Nature of Dark Matter
- Constraints on Cold Dark Matter Accelerating Cosmologies and Cluster Formation
- Flat FRW Cosmologies with Adiabatic Matter Creation: Kinematic tests
- Supergravity Inflation on the Brane
- Cosmographic Degeneracy
Cited by in corpus (11)
- f(R,T) gravity
- Thermodynamic interpretation of the generalized gravity models with geometry - matter coupling
- Matter creation and cosmic acceleration
- Challenging matter creation models in the phantom divide
- Cosmic expansion with matter creation and bulk viscosity
- Dark side of the universe in the Stephani cosmology
- Observational Hubble parameter data constraints on the interactive model of gravity with particle creation
- Emulating dark energy models with known equation of state via the created cold dark matter scenario
- Accelerated Expansion of the universe based on Particle Creation-Destruction Processes and Dark Energy in FLRW universes
- Exploring the cosmological degeneracy between decaying dark matter model and viscous CDM
- Correspondence between particle creation and dark components interaction in the context of gravity