Setting new Cosmology constraints with ALMA
  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.
