The Nuts and Bolts of Inflation Richard Barrett. Dark Energy SeminarGlasgow 29/11/2003 Inflation What is inflation? What is dark energy? Why was inflation.
Glion Colloquium / June 2009 1 The Large Hadron Collider LHC ˗̶ The Large Hadron Collider LHC ˗̶ Shedding Light on the Shedding Light on the EARLY Universe.
Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between.
‘Physics of Radio Galaxies’ Anatomy of Extragalactic Radio Sources Miley Symposium May, 2013, Chris Carilli NRAO ‘Radio Galaxies as beacons to early, massive.
(Pseudo)Scalar Fields in the Early Universe London Centre for Terauniverse Studies (LCTS) AdV 267352 IRAP Ph D School, Nice September 2-21 2013 Nick E.
February 16, 2009Scott Dodelson, AAAS Meeting Gravitational Waves as a Probe of the Early Universe.
John Harris (Yale) Hadron 07 - Frascati, Italy, 8 -13 Oct. 2007 Exploring the Quark-Gluon Plasma at RHIC & LHC – Today’s Perspective.
Future Directions in Parity Violation: From Quarks to the Cosmos M.J. Ramsey-Musolf + many students, post- docs, collaborators, and colleagues PAVI ‘06.
Charged particle multiplicity studies with PHOBOS Birger Back Argonne National Laboratory for the PHOBOS Collaboration.
QED at Finite Temperature and Constant Magnetic Field: 1. The Standard Model of Electroweak Interaction at Finite Temperature and Strong Magnetic Field.
Lepton number violation in cosmology and particle physics M. Yoshimura Introduction: Symmetry and its breakdown ・ Sources of B non-conservation : electroweak.
21cm Constraints on Reionization Benedetta Ciardi MPA T. Di Matteo (CMU), A. Ferrara (SISSA), I. Iliev (CITA), P. Madau (UCSC), A. Maselli (MPA), F. Miniati.