Physics
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pthph..81.1037n&link_type=abstract
Progress of Theoretical Physics, Vol. 81, No. 5, pp. 1037-1056
Physics
29
Scientific paper
We investigate the stationary solution of the modified Fokker-Planck equation which governs the global dynamics of the inflation. Contrary to the original FP equation which is for a Hubble horizon size region, we found that the normalizable stationary solution can exist for modified Fokker-Planck equation which is for many Hubble horizon size regions. For a chaotic inflationary model with the potential lambda phi(2n) , we get initial distribution of classical universes using this solution, and discussed the physical meaning of it. Especially for n = 2, this distribution obeys power-law and classical universes which, created from the Planck energy region, make the fractal structure. In other cases n !=q 2, creation of large classical universes is strongly suppressed.
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