hanson@econ.berkeley.edu (Robin Hanson) writes:
>The theoretical attraction is for a very nearly critical mass
>universe. The key observation is that the mass density relative
>to critical density diverges with time. If this parameter is near
>one, then it must have been very very near one when the universe
>was orders of magnitude younger than it is now. And if it is now
>almost exactly one now, then it will be far from one when the
>universe is a few orders of magnitude older than now, and thus
>we are living at the unusual time when this parameter goes from
>being near one to being far from one. Theorists don't have any
>ideas I know of for this coincidence, so they'd rather it wasn't
>there.
Barrow and Tipler mention on pages 494 and 500 of The Anthropic
Cosmological Principle a theory that all possible maximum sizes for
a closed universe are equally probable, implying that we should expect
omega to be infinitessimally close to one. (I don't know how this
theory handles the possibility of an open universe).
-- ------------------------------------------------------------------------ Peter McCluskey | caffeine O CH3 pcm@rahul.net | || | http://www.rahul.net/pcm | H3C C N | \ / \ / \ | N C C | || || C C---N // \ / O N | CH3Received on Sun Jan 18 20:36:34 1998
This archive was generated by hypermail 2.1.8 : Tue Mar 07 2006 - 14:45:29 PST