Manual Solution Fundamentals Cosmology Rich
The CMB and the SZ Effect Current Topics 2008 Dr. Katy Lancaster.
Cosmology Dr Katy Lancaster. Overview The Big Bang –Formation of the Universe –The Cosmic Microwave Background –The COBE experiment The Expanding Universe.
Cosmology from the Cosmic Microwave Background Katy Lancaster Astrophysics Group.
Dark energy and the CMB Robert Crittenden Work with S. Boughn, T. Giannantonio, L. Pogosian, N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto.
Dan Hooper Particle Astrophysics Center Fermi National Accelerator Laboratory [email protected] Ultrahigh Energy Cosmic Ray Nuclei and Neutrinos Aspen Workshop.
Cosmology topics, collaborations BOOMERanG, Cosmic Microwave Background LARES (LAser RElativity Satellite), General Relativity and extensions, Lense-Thirring.
USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS TO “FILL THE GAP” AT 1
Dark Energy Perturbations 李明哲 南京大学物理学院 2011.10.13 中国科技大学交叉学科理论研究中心 合肥.
On scales larger than few arcminutes, the millimeter sky is dominated by CMB temperature fluctuations. A significant fraction of these CMB photons encode.
The Pierre Auger Observatory & Ultra High Energy Cosmic Rays Nick Cowan UW Astronomy January 2006.
What have we learnt from WMAP? Robert Crittenden Institute of Cosmology and Gravitation, Portsmouth, UK.