GLOBAL AND LOCAL EFFECTS OF ROTATION: OBSERVATIONAL ASPECTS
DOI10.1142/S0218271811019475zbMath1263.85066arXiv1103.5786OpenAlexW2146585300MaRDI QIDQ4914582
Publication date: 15 April 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1103.5786
clusters of galaxiesdark radiationangular momenta of galaxiesgalaxy formation scenariosgalaxy orientationUniverse rotation
Relativistic cosmology (83F05) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Astrophysical cosmology (85A40) Statistical astronomy (85A35)
Cites Work
- Energy and angular momentum densities in a Gödel-type universe in teleparallel geometry
- LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
- Theorems on shear-free perfect fluids with their Newtonian analogues
- Effect of the global rotation of the universe on the formation of galaxies
- Dark energy and global rotation of the universe
- Rotation of the universe and the angular momenta of celestial bodies
- Tilted homogeneous cosmological models
- Some remarks on the angular momenta of galaxies, their clusters and superclusters
- Dynamics of the universe with global rotation
- Rotating Bianchi type V dust models generalizing the k=−1 Friedmann model
- Friedmann limits of rotating hypersurface–homogeneous dust models
- Global aspects of shear-free perfect fluids in general relativity
- Some solutions of the Einstein field equations for a rotating perfect fluid
- Homogeneous Newtonian cosmologies and their perturbations
- Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on uα and wα
- Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. II. One Killing field spanned on uα and wα
- Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα
- Can brane cosmology with a vanishing explain the observations?
- Large Mass Hierarchy from a Small Extra Dimension
- THE VIRGO ALIGNMENT PUZZLE IN PROPAGATION OF RADIATION ON COSMOLOGICAL SCALES
- SEARCH FOR GLOBAL METRIC ANISOTROPY IN TYPE 1a SUPERNOVA DATA
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Minimal conditions for the creation of a Friedman-Robertson-Walker universe from a bounce
- Study of the magnitude-redshift relation for type Ia supernovae in a model resulting from a Ricci-symmetry
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