The Dark Universe
arXiv:0906.5036 · doi:10.1103/RevModPhys.82.331
Abstract
For a few years now, cosmology has a standard model. By this term, we mean a consistent theoretical background which is at the same time simple and broad enough to offer coherent explanations for the vast majority of cosmological phenomena. This review will briefly summarise the cosmological model, then proceed to discuss what we know from observations about the evolution of the Universe and its contents, and what we conclude about the origin and the future of the Universe and the structures it contains.
Invited article for Reviews of Modern Physics. 51 pages, 12 figures
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- Observational constraint on the interacting dark energy models including the Sandage-Loeb test
- Nonlinear 3D Cosmic Web Simulation with Heavy-Tailed Generative Adversarial Networks
- Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
- BAO cosmography
- Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
- Galaxy cluster angular size data constraints on dark energy
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- Accelerating bianchi type dark energy cosmological model with cosmic string in f(T) Gravity
- Does the second law hold at cosmic scales?
- Isocurvature bounds on axion-like particle dark matter in the post-inflationary scenario
- From Clock Synchronization to Dark Matter as a Relativistic Inertial Effect
- Weak lensing tomography with orthogonal polynomials
- A framework for the next generation of stationary cosmological models
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- Stringent neutrino flux constraints on anti-quark nugget dark matter
- Time and distance constraints on accelerating cosmological models
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- Latest data constraint of some parameterized dark energy models
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- Baryogenesis and Asymmetric Dark Matter from The Left-Right Mirror Symmetric Model
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