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Eternal inflation is a hypothetical inflationary universe model, which is itself an outgrowth or extension of the Big Bang theory. In theories of eternal inflation, the inflationary phase of the universe's expansion lasts forever in at least some regions of the universe. Because these regions expand exponentially rapidly, most of the volume of the universe at any given time is inflating. All models of eternal inflation produce a hypothetically infinite multiverse, typically a fractal. In 1983, Paul Steinhardt presented the first example of eternal inflation and Alexander Vilenkin showed that it is generic. Eternal inflation was found to be predicted by many different models of cosmic inflation. MIT professor Alan Guth proposed an inflation model involving a "false vacuum" phase with positive vacuum energy. Parts of the universe in that phase inflate, and only occasionally decay to lower-energy, non-inflating phases or the ground state. In chaotic inflation, proposed by physicist Andrei Linde, the peaks in the evolution of a scalar field (determining the energy of the vacuum) correspond to regions of rapid inflation which dominate. Chaotic inflation usually eternally inflates,〔 since the expansions of the inflationary peaks exhibit positive feedback and come to dominate the large-scale dynamics of the universe. Alan Guth's 2007 paper, "Eternal inflation and its implications",〔Guth, Alan; (Eternal inflation and its implications ) arXiv:hep-th/0702178〕 details what is now known on the subject, and demonstrates that this particular flavor of inflationary universe theory is relatively current, or is still considered viable, more than 20 years after its inception. 〔(【引用サイトリンク】 title=Many worlds interpretation )〕〔(【引用サイトリンク】url=http://pauli.physics.lsa.umich.edu/w/arch/som/sto2001/Guth/real/n001.htm )〕 ==Inflation and the multiverse== Both Linde and Guth believe that inflationary models of the early universe most likely lead to a multiverse but more proof is required. Polarization in the cosmic microwave background radiation suggests inflationary models for the early universe are more likely but confirmation is needed.〔 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Eternal inflation」の詳細全文を読む スポンサード リンク
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