CMB Polarization as complementary information to anisotropies
arXiv:astro-ph/0310650 · doi:10.1016/j.crhy.2003.10.006
Abstract
The origin of CMB polarization is reviewed. Special emphasis is placed on the cosmological information encoded in it: the nature of primordial fluctuations, the connection with the inflation paradigm. Insights into more recent epochs are also discussed: early reionization and high redshift matter distribution from CMB lensing.
9 pages, 6 figures, One reference added in section 6.2
References in corpus (16)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
- Detection of Polarization in the Cosmic Microwave Background using DASI
- CMB Lensing Reconstruction on the Full Sky
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- The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops
- Lensing Reconstruction with CMB Temperature and Polarization
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- The Dark Age of the Universe
- Model-Independent Reionization Observables in the CMB
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- The Polarization of the Cosmic Microwave Background
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- Polarization experiments
- CMB Signatures of Extended Reionization