CONSTRAINTS ON THE COSMOLOGICAL DENSITY PARAMETERS AND COSMIC TOPOLOGY
From MaRDI portal
Publication:5293921
DOI10.1142/S0218271807009942zbMath1117.83138arXivastro-ph/0605214OpenAlexW3103886192MaRDI QIDQ5293921
Publication date: 5 July 2007
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0605214
observational cosmologycosmic topologycircles in the skyconstraints on cosmological density parameters
Cites Work
- Spikes in cosmic crystallography. II: Topological signature of compact flat universes
- Topology and cosmology
- Topology and the cosmic microwave background
- Detectability of cosmic topology in flat universes
- A topological signature in cosmic topology
- Are small hyperbolic universes observationally detectable?
- Detectability of cosmic topology in almost flat universes
- Constraining the Topology of the Universe
- What do very nearly flat detectable cosmic topologies look like?
- Inflation in string-inspired cosmology and suppression of CMB low multipoles
- Topological lensing in spherical spaces
- Detecting topology in a nearly flat spherical universe
- Constraints on the detectability of cosmic topology from observational uncertainties
- A hint of Poincaré dodecahedral topology in the WMAP first year sky map
- SPIKES IN COSMIC CRYSTALLOGRAPHY
- The topology of the universe: the biggest manifold of them all
- Circles in the sky: finding topology with the microwave background radiation
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Relativistic effects of our galaxy's motion on circles-in-the-sky in CMB maps
- CMB anisotropy of the Poincaré dodecahedron
- CMB anisotropy of spherical spaces
This page was built for publication: CONSTRAINTS ON THE COSMOLOGICAL DENSITY PARAMETERS AND COSMIC TOPOLOGY
