Setting new Cosmology constraints with ALMA
arXiv:1403.1586 · doi:10.1063/1.4913339
Abstract
I make a short revision of Cosmology questions which ALMA was built to address. Without diving into much detail, I point out the ALMA specifications and strategies which are expected to provide a better handle of: the temperature evolution of the Cosmic Microwave Background (CMB) and the properties of its secondary anisotropies (such as the thermal and kinetic Sunyaev-Zel'dovich and the Ostriker-Vishniac effects); variability of dimensionless fundamental constants; Ho and galaxy initial mass function by means of strong gravitational lensing; black hole science with the greatly expected Event Horizon Telescope.
To appear in the Proceedings of CosmosurII held in Valparaiso on 27th-31st May 2013; 13 pages (6 of text, 7 of references)