Georg Raffelt, Max-Planck-Institut für Physik, München, Germany Neutrino Physics & Astrophysics, 17-21 Sept 2008, Beijing, China Geheimnis der dunklen.
New Developments and Perspectives in General Relativity and Cosmology Thesis Dennis Smoot University of Illinois Chicago, IL.
Cosmological Parameters and the WMAP data Antony Lewis CfA, Harvard / CITA, Toronto Standard assumptions – what are the parameters?
IS IT POSSIBLE TO OBSERVATIONALLY DISTINGUISH ADIABATIC QUARTESSENCE FROM CDM? Luca Amendola 1, Martin Makler 2, Ribamar R. R. Reis 3 and Ioav Waga 3 1.
The Big Bang Theory: Origin & Evolution of the Universe.
Stellar Physics 10 lectures, exploring the development of cosmology, and some of the key ideas of Big Bang theory Access PPT slides at .
Dr Martin Hendry University of Glasgow. Why are we here?…. The period of inflation in the very early Universe was invoked to explain some apparent fine.
Seeing Dark Energy (or the cosmological constant which is the simplest form of DE) Professor Bob Nichol (ICG, Portsmouth)
IIB on K3 £ T 2 /Z 2 orientifold + flux and D3/D7: a supergravity view-point Dr. Mario Trigiante (Politecnico di Torino)
Communicating Astronomy with the Public 2005 The Nuts and Bolts of a Good News Story Cheryl Gundy and Lynn Barranger STScI Office of Public Outreach.
Gerard t Hooft Spinoza Institute, Utrecht University Utrecht University and.
Scientific Arguments: Fine-Tuning and the Big Bang Professor Rob Koons Philosophy – UT [email protected] robkoons.net Unpublished Papers.