Eric2006 - Well, my memory was close - but here is the standard big bang model explanation - which sounds reasonable for any model starting with a superdense superhot state and cooling and expanding:<br /><br />"A few hundred thousand years later [after the big bang] the temperature had fallen to about 3,000K [from above 10 trillionK {K=degrees Kelvin}right after the big bang]. Protons became able to capture and hold on to electrons to form atoms of neutral hydrogen, because the radiation was no longer energetic enough to separate (ionize) them. Most of the electrons were quickly mopped up, and it became possible for photons to travel vast distances without being absorbed or suffering collisions. During this stage, known as the 'decoupling' of matter and radiation, the universe became transparent." - [bracketts mine] - "The World of Science," by Andromeda Oxford Ltd. (distributed by Britannica) 1991, Volume 8, pages 110-111.<br /><br />Note that while page 111 indicates a few hundred thousand years after the big bang for becoming transparent, the caption on the illustration on page 110 states:<br /><br />"The graph shows how the temperature of matter and radiation declined from well over 10^12K to about 3,000K in the first 100,000 years or so. At this stage (the 'decoupling' of matter from radiation) space became transparent." - Ibid., p. 110<br /><br />OK, that is obviously an estimate, since in the first 100,000 years is less than a few hundred thousand years.<br /><br />The point I was making is that FTL inflation may well have occurred very early after the big bang, long before this decoupling. Therefore, some matter may still be beyond our universe's light. <br /><br />If said matter is expanding FTL, then it would be forever beyond the light of our universe.