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"For any reasonable value of Omega at the beginning of time, Einstein's equations show that it should almost be zero today. For Omega to be so close to 1 so many billions of years after the big bang would require a miracle. This is what is called in cosmology the finetuning problem. God, or some creator, had to "choose" the value of Omega to within fantastic accuracy for Omega to be about 0.1 today. For Omega to be between 0.1 and 10 today, it means that Omega had to be 1.00000000000000 one second after the big bang. In other words, at the beginning of time the value of Omega had to be "chosen" to equal the number 1 to within one part in a hundred trillion, which is difficult to comprehend."
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omega
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Michio Kaku |
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"Inflation is continuous and eternal, with big bangs happening all the time, with universes sprouting from other universes. In this picture, universes can "bud" off into other universes, creating a "multiverse." In this theory, spontaneous breaking may occur anywhere within our universe, allowing an entire universe to bud off our universe. It also means that our own universe might have budded from a previous universe. In the chaotic inflationary model, the multiverse is eternal, even if individual universes are not. Some universes may have a very large Omega, in which case they immediately vanish into a big crunch after their big bang. Some universes only have a tiny Omega and expand forever. Eventually, the multiverse becomes dominated by those universes that inflate by a huge amount. In retrospect, the idea of parallel universes is forced upon us."
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universe
omega
parallel-universes
multiverse
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Michio Kaku |