conferito da ICRA
- 2018
- For obtaining important constraints on the models of inflationary stage of the Universe and level of
primordial non-Gaussianity; measuring with unprecedented sensitivity gravitational lensing of Cosmic
Microwave Background fluctuations by large-scale structure of the Universe and corresponding B-
polarization of CMB, the imprint on the CMB of hot gas in galaxy clusters; getting unique information about
the time of reionization of our Universe and distribution and properties of the dust and magnetic fields in our
Galaxy
