Interactions in the dark sector of the Universe
arXiv:1404.7334 · doi:10.1142/S0219887814600147
Abstract
Interactions inside the cosmological dark sector influence the cosmological dynamics. As a consequence, the future evolution of the Universe may be different from that predicted by the CDM model. We review main features of several recently studied models with nongravitational couplings between dark matter and dark energy.
arXiv comment21 pages, Proceedings of the 49th Winter School of Theoretical Physics, Ladek-Zdroj, Poland, February 10-16, 2013
References in corpus (33)
- Planck 2013 results. XVI. Cosmological parameters
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Information criteria for astrophysical model selection
- Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Interacting Quintessence
- The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
- The end of unified dark matter?
- Phenomenology of a realistic accelerating universe using only Planck-scale physics
- Is cosmic acceleration slowing down?
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- Opportunities for future supernova studies of cosmic acceleration
- The Luminosity Distance, the Equation of State, and the Geometry of the Universe
- Statefinder parameters for interacting dark energy
- Scaling Cosmology
- A cosmological constant from the QCD trace anomaly?
- Friedmann cosmology with decaying vacuum density
- Growth factor parametrization and modified gravity
- Scalar-field-dominated cosmology with a transient accelerating phase
- A Two-Field Quintessence Model
- Cosmological dynamics with non-linear interactions
- Dynamics of dark energy models and centre manifolds
- Can the Universe escape eternal acceleration?
- Density Perturbations for Running Cosmological Constant
- Could the cosmic acceleration be transient? A cosmographic evaluation
- A cosmological concordance model with dynamical vacuum term
- AIC, BIC, Bayesian evidence against the interacting dark energy model
- Evolution of density perturbations in decaying vacuum cosmology
- Using a phenomenological model to test the coincidence problem of dark energy
- Roles of dark energy perturbations in the dynamical dark energy models: Can we ignore them?
- Perturbations for transient acceleration
Cited by in corpus (6)
- Covariantizing the interaction between dark energy and dark matter
- Null test for interactions in the dark sector
- Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
- Dynamics of the diffusive DM-DE interaction--dynamical system approach
- Multi-fluid cosmology in Einstein gravity: analytical solutions
- A causal viscous cosmology without singularities