Status of CMB observations in 2015
arXiv:1606.03375 · doi:10.1142/S2010194516601885
Abstract
The 2.725 K cosmic microwave background has played a key role in the development of modern cosmology by providing a solid observational foundation for constraining possible theories of what happened at very large redshifts and theoretical speculation reaching back almost to the would-be big bang initial singularity. After recounting some of the lesser known history of this area, I summarize the current observational situation and also discuss some exciting challenges that lie ahead: the search for B modes, the precision mapping of the CMB gravitational lensing potential, and the ultra-precise characterization of the CMB frequency spectrum, which would allow the exploitation of spectral distortions to probe new physics.
17 pages, 3 figures, Latex, conference proceeding based on talk at CosPA 2015 in Daejeon, South Korea in October 2015, minor typos corrected
References in corpus (7)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array
- Toward an Understanding of Foreground Emission in the BICEP2 Region
- Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
- Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes