Pie eyed
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- Jun 26, 2007
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- #126
Here's one for you all;
The Horizon problem
Why is the Universe, almost but not quite, homogeneous on the very largest distance scales. Is it the result of an inflationary epoch - a period of rapid expansion in very early history of the universe which flattened out, or could of flattened out homogeneities? If so what called this inflation?
The "Big Bounce" theory, a variant of the "Big Crunch" postulates that at the point in time when the incredibly rapidly contracting universe reaches the point where gravity reverses it's effect and becomes repellant rather than it's more familiar attractant self, massive vibrations would be caused which theoretically should be evident in the background radiation of any resultant universe....much like the uneven homogeneities you mention.
Still just another of the many theories floating around.
Just as a point of interest of the more than 600 most current papers on the subject the last 100 or so focus on the "Bid Bounce" version of events.
At the moment it is the most popular amongst those in the field as far as interest and speculation go.
You have to remember that the variations on the Big Bang are dealing with a period of time in the Plankt Era, where Newtonian physics appear to break down, around 10^24 of a second,which is so short as to be almost un-fathomable to most people.





