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Comparative CMBology: Putting Things Together
Published online by Cambridge University Press: 26 May 2016
Abstract
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I present a series of diagrams which illustrate why the cosmic microwave background (CMB) data favor certain values for the cosmological parameters. Various methods to extract these parameters from CMB and non-CMB observations are forming an ever-tightening network of interlocking constraints. I review the increasingly precise constraints in the Ωm - ΩΛ plane and show why more cosmologists now prefer ΛCDM cosmologies to any other leading model.
- Type
- Part IX: Putting it all together
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2005
References
Bridle, S. L., Zehavi, I., Dekel, A, Lahav, O., Hobson, M. P. & Lasenby, A. N.
2000, MNRAS
astro-ph/0006170.Google Scholar
Carroll, S. M.
2001, Living Reviews of Relativity, submitted, Fig. 11, astro-ph/0004075.Google Scholar
Efstathiou, G., Bridle, S. R., Lasenby, A. N., Hobson, M. P. & Ellis, R. S.
1999, MNRAS, 303, L47–L52.Google Scholar
Parodi, B. R., Saha, A., Sandage, A. & Tammann, G. A.
2000, ApJ, submitted, astro-ph/0004063.Google Scholar
Tegmark, M., Zaldarriaga, M. & Hamilton, A.J.S.
2001, Phys. Rev. D., astro-ph/0008167 v3.Google Scholar
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