Outgoing waves in the Cosmic Microwave Background polarized intensity from localized cosmological perturbations, from Baccigalupi (1999) and Baccigalupi, Perrotta (2000)

Highlights

Hypothesis of our Universe being within one large bubble enucleated during a primordial first order phase transition (1996)

"Acoustic" rings in the early Universe (1998, 1999)

Neural Networks applied to Data Analysis in Cosmology (2000)

Dark Energy & Gravity: Extended Quintessence and the R-boost (2000, 2005, 2006, 2008)

The diffuse Galactic polarized foregrounds are tough for CMB B-modes from Cosmological Gravitational Waves (2003)

Dark Energy and the formation clusters of galaxies (2004, 2005)

Dark Energy records in lensed Cosmic Microwave Background (2004, 2006)

Bayesian Component Separation (2006, 2009, 2010, 2011, 2012)

Lensed Cosmic Microwave Background from N-body Simulations (2008, 2009, 2013, 2014, 2015)

The results of the Planck mission (2011, 2012, 2014, 2016, 2018)

Cross-Correlation of Cosmic Fields (2015, 2016)

Constraints Cosmological Gravitational Waves from the BICEP2 and Planck experiments (2015)

The results of the POLARBEAR experiment (2015, 2017)

Understanding diffuse polarized foregrounds for measuring B-modes of the Cosmic Microwave Background (2016, 2018)