Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!mnetor!seismo!columbia!rutgers!uwvax!uwmacc!uwmcsd1!uwmeecs!litow From: litow@uwmeecs.UUCP (Dr. B. Litow) Newsgroups: sci.physics Subject: Re: Size of the Universe Message-ID: <440@uwmeecs.UUCP> Date: Wed, 15-Oct-86 07:44:57 EDT Article-I.D.: uwmeecs.440 Posted: Wed Oct 15 07:44:57 1986 Date-Received: Wed, 15-Oct-86 20:23:08 EDT References: <5845@decwrl.DEC.COM> <1322@utastro.UUCP> <1733@cvl.UUCP> Organization: U of Wi-Milwaukee, Dept of EE and CS Lines: 26 > From one of Ethan Vishniac's postings: > > > The flatness problem makes everyone uncomfortable... > > The mention of hyperspherical models made me wonder how we know that > the universe really is as extensive as the distance computed from > highly red-shifted objects suggests. > In particular, how do we know that the univers is not (relatively) > small with a topology that permits closed geodesics. > In this case, highly red-shifted light has just looped the loop > a couple of times, which would allow the entire universe to be in > communication. > This would have interesting consequences. For instance, certain > object would represent earlier stages of our own galaxy if we knew > where to look. > I have never heard this notion discussed. > Does anyone know what (if anything) eliminates such a model?? > Please reply to the net. > > > Randal Nelson I don't know much about this but a starting point for references might be "The Large Scale Structure of Spacetime" by Hawking & Ellis *** REPLACE THIS LINE WITH YOUR MESSAGE ***