Lecture 2 Temperature anisotropies cont: what we can learn CMB polarisation: what it is and what we can learn.
Hydrodynamical description of first order phase transitions Vladimir Skokov (GSI, Darmstadt) in collaboration with D. N. Voskresensky Strongly Interacting.
Ginés MARTINEZ, SUBATECHRencontres de Moriond March 17-24 20011 The heavy ion collider experiment @ LHC A L I C E Ginés MARTINEZ # for the ALICE Collaboration.
Science with Future CMB Observations Lloyd Knox UC Davis.
Matthew von Hippel 1. Outline What is Big Bang Nucleosyntheis? How does it work? How can we check it? The Primordial Lithium Problem Problem or problem?
Neutron stars and the properties of matter at high density Gordon Baym, University of Illinois Future Prospects of Hadron Physics at J-PARC and Large Scale.
Hyperon Suppression in Hadron- Quark Mixed Phase T. Maruyama (JAEA), S. Chiba (JAEA), H.-J. Schhulze (INFN-Catania), T. Tatsumi (Kyoto U.) 1 Property of.
Design in the Cosmos Dr. Hugh Ross Reasons To Believe.
Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS.
Suzanne Staggs (Princeton) Rencontres de Blois, 1 June 2011 The Atacama Cosmology Telescope (ACT): Still More Cosmology from the Cosmic Microwave Background.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 10; February 12 2014.
1 Some key problems and key reactions in Nuclear Astrophysics Main issues: BBN: was the universe always the same? What’s in the core of Sun and other MS.