Swinburne, Ross, And the Cosmological Argument
THE BIG BANG HOW CLOSE CAN WE COME? Michael Dine May, 2003.
Visualization Project Seeing and Hearing the CMB.
Young And Hot Big Bang
3A03 – GR and Cosmology Ralph Pudritz Dept. of Physics & Astronomy McMaster University.
The Cosmic Near-Infrared Background: Remnant light form early stars Journal Club talk 3.12.2010 A. B. Fry Ferdinand & Komatsu 2006 (F&K06) also Ferdinand.
3K background radiation by Roman Werpachowski and Peter Holrick.
ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations.
Cosmic Microwave Background & Primordial Gravitational Waves Jun-Qing Xia Key Laboratory of Particle Astrophysics, IHEP Planck Member CHEP, PKU, April.
1 The Life History of Galaxies and Black Holes Elaine Sadler, School of Physics, University of Sydney The life history of ‘normal’ galaxies Black holes.
Cosmology. The Cosmological Principle On the largest scales, the universe is roughly homogeneous (same at all places) and isotropic (same in all directions).
The Big Bang: Fact or Fiction?
