1. “majority of its surfacearea is only about 10feet above sea level” The Nobel Prize in Physics 2011 Bob Nichol (ICG Portsmouth) 2. General Relativity Primer 3. Cosmology…

Establishing homogeneity of the universe in the shadow of dark energy Chris Clarkson Astrophysics, Cosmology & Gravity Centre, and, Department of Mathematics and Applied…

Slide 1Bin Wang Fudan University Shanghai Signature on the interaction between dark energy and dark matter Slide 2 COSMIC TRIANGLE Tightest Constraints: Low z: clusters(mass-to-light…

Slide 1 Neutrino Mass due to Quintessence and Accelerating Universe Gennady Y. Chitov Laurentian University, Canada Slide 2 Tyler August, Laurentian, Canada Tina Kahniashvili,…

Slide 1 seven sisters 20051 How I Stopped Worrying and Learned to Love the Universe Marilena LoVerde Columbia University Hubble Deep Field, NASA Slide 2 seven sisters 20052…

Slide 1 Rachel Bean : Beyond Einstein May 2004 An Overview of Dark Energy Rachel Bean Princeton University Slide 2 Rachel Bean : Beyond Einstein May 2004 The key dark energy…

Slide 1 Why the cosmological constant goes to zero, and why we see it now Slide 2 Quintessence C.Wetterich A.Hebecker, M.Doran, M.Lilley, J.Schwindt, C.Müller, G.Schäfer,…

The Hunting of the Dark Energy and On Beyond Lambda Eric Linder Cosmology Teach-In 26 June 2003 Cosmic Concordance Supernovae alone  Accelerating expansion  > 0…

From Dark Energy to Dark Force Luca Amendola INAF/Osservatorio Astronomico di Roma Outline Dark energy-dark matter interactions Non-linear observational effects of DE Modified…

Structure formation as an alternative to dark energy Syksy Räsänen University of Geneva Contents Brief overview of the observations The effect of clumpiness on the expansion…