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Thursday, 22 March 2007, 13:00 in P8445B
Prof. Ira Wasserman (Cornell)
The neutron star in 1930 -- and today (special colloquium)
The neutron had not yet been discovered in 1930, but it might have been. To understand neutron stars simply it is fun to ask how much could have been predicted about their properties if it had. After using this fictional device to introduce neutron stars, we will fast forward to today, where some of the issues remain the same as we could have deduced in 1930, but others are more subtle -- and potentially revealing about high density nuclear physics.
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Modified by Andrei Frolov <frolov@sfu.ca> on 2023-11-01