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SUMMARY:Future cosmology from arcminute CMB data - Erminia Calabrese
DTSTART:20181112T130000Z
DTEND:20181112T140000Z
UID:TALK109459@talks.cam.ac.uk
CONTACT:Tobias Baldauf
DESCRIPTION:High-resolution observations of the Cosmic Microwave Backgroun
 d (CMB) radiation provide constraints on a large number of extensions to t
 he standard cosmological model\, and will play a key role in future cosmol
 ogical results. Assuming that contamination from Galactic and extra-galact
 ic emission can be kept under control\, damping tail data from ground-base
 d CMB experiments inform us on the properties of the primordial scalar flu
 ctuations\, on the particle and dark matter content of the Universe\, on t
 he Universe evolution and on the epoch of reionization. The Atacama Cosmol
 ogy Telescope (ACT) is one of the leading experiments currently operating 
 and will be superseded by the new Simons Observatory (SO) from 2021. In th
 is talk I will describe past and future observations from ACT and SO\, and
  show scientific forecasts for the next five years.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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