Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!mnetor!seismo!lll-crg!lll-lcc!qantel!hplabs!pyramid!ucat!pesnta!amd!amdcad!amdimage!prls!philabs!pwa-b!mmintl!franka From: franka@mmintl.UUCP (Frank Adams) Newsgroups: net.arch Subject: Re: VERY LARGE main memories: crypt Message-ID: <1820@mmintl.UUCP> Date: Thu, 18-Sep-86 17:59:23 EDT Article-I.D.: mmintl.1820 Posted: Thu Sep 18 17:59:23 1986 Date-Received: Sun, 21-Sep-86 22:06:48 EDT References: <1178@bu-cs.bu-cs.BU.EDU> <1087@ihwpt.UUCP> <553@astroatc.UUCP> <1124@tekig5.UUCP> <1126@tekig5.UUCP> <645@faron.UUCP> Reply-To: franka@mmintl.UUCP (Frank Adams) Organization: Multimate International, E. Hartford, CT Lines: 19 In article <645@faron.UUCP> bs@faron.UUCP writes: > The point of all this is that the known mass can be >used to get an estimate on the number of atoms in the universe. It is >something like 10^78 or 10^79. There are therefore at least that number >of electrons. This assumes that most of the mass in the universe is in the form of ordinary matter -- protons, neutrons, and electrons. This assumption is very much in question these days. Proposed alternatives include everything from neutrinos to topological singularities left over from shortly after the big bang. The visible matter in the universe is about an order of magnitude less than amount needed to close the universe. This is a better lower bound on the number of electrons -- it seems unlikely that stars contain any significant quantity of such exotic mass. Frank Adams ihnp4!philabs!pwa-b!mmintl!franka Multimate International 52 Oakland Ave North E. Hartford, CT 06108