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.
Two Phase Formation of Massive Galaxies T.Naab, P. Johansson, R. Cen, K. Nagamine, R. Joung and J.P.O. PPPL:, 19 Dec 2012 ApJ.L.,658,710 (2007) ApJ.,697,
Supernova Cosmology Bruno Leibundgut European Southern Observatory.
1 16.1Evidence of the Big Bang 16.2The Big Bang 16.3Stellar Evolution 16.4Astronomical Objects 16.5Problems with the Big Bang 16.6The Age of the Universe.
History of the Universe - according to the standard big bang Radiaton dominated era Matter dominated era Decoupling - CMB emission Star and structure formation.
Cosmology Tim Arlen UCLA Physics Department Fall 2006 Image Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)
1.Introduction The standard cosmology is a successful framework for interpreting observations. In spite of this fact there were certain questions which.
It would appear that there is more matter in the universe, called dark matter, than we see. We believe this because The edges of galaxies are rotating.
Supernova cosmology The quest to measure the equation of state of dark energy Bruno Leibundgut European Southern Observatory.
Inflation
Physical Cosmology
Dark Matter and Energy
