James Rich Solutions of Fundamentals of Cosmology 123 Solutions Chapter 1 1.1 If Ω M = Ω T = 1, then Ω M (a) = Ω T (a) = 1 for all a(t ). Structure formation never ceases…

Slide 1The CMB and the SZ Effect Current Topics 2008 Dr. Katy Lancaster Slide 2 Course Content Introduction - The Cosmic Microwave Background - The Sunyaev Zeldovich Effect…

Slide 1Cosmology Dr Katy Lancaster Slide 2 Overview The Big Bang –Formation of the Universe –The Cosmic Microwave Background –The COBE experiment The Expanding Universe…

Slide 1Cosmology from the Cosmic Microwave Background Katy Lancaster Astrophysics Group Slide 2 Who am I? Postdoc in the Physics department working with Professor Mark Birkinshaw…

Slide 1Dark energy and the CMB Robert Crittenden Work with S. Boughn, T. Giannantonio, L. Pogosian, N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto Slide 2 Why use…

Slide 1 Dan Hooper Particle Astrophysics Center Fermi National Accelerator Laboratory [email protected] Ultrahigh Energy Cosmic Ray Nuclei and Neutrinos Aspen Workshop on…

Slide 1 Cosmology topics, collaborations BOOMERanG, Cosmic Microwave Background LARES (LAser RElativity Satellite), General Relativity and extensions, Lense-Thirring Landau…

Slide 1 USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS TO “FILL THE GAP” AT 1 MORPHOLOGICAL CLASSIFICATION OF RADIO GALAXIES FR IFR II LOW POWERHIGH POWER Fanaroff…

Slide 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 Slide 2 Outline Importance of cosmological…

Slide 1 On scales larger than few arcminutes, the millimeter sky is dominated by CMB temperature fluctuations. A significant fraction of these CMB photons encode a wealth…