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19 February 2004
The
cosmic microwave background gives us a detailed picture of the Universe
before atoms, stars and galaxies some 14 billion years ago. Encoded
in its tiny variations in intensity are information about the past,
present and future of the Universe. It also provides one of the strongest
pieces of evidence for the big bang cosmology. This lecture will discuss
contemporary cosmological theory, especially in relation to the findings
of the Wilkinson Microwave Anisotropy Probe. The implications of current
cosmological theory for religious thought will also be discussed.
Keynote speaker:
Coverage:
Listen to Dr. Turner
Listen to Reverend Smith-Moran
Read the Summary
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