How probable is inflation

作者: S.W. Hawking , Don N. Page

DOI: 10.1016/0550-3213(88)90008-9

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摘要: … , the solution will exit from the stiff regime at large I xl and will undergo inflation before entering the dust regime. If this is so, we may write down an approximate solution valid throughout …

参考文章(8)
V.A. Belinsky, L.P. Grishchuk, I.M. Khalatnikov, Ya.B. Zeldovich, INFLATIONARY STAGES IN COSMOLOGICAL MODELS WITH A SCALAR FIELD Physics Letters B. ,vol. 155, pp. 232- 236 ,(1985) , 10.1016/0370-2693(85)90644-6
G.W. Gibbons, S.W. Hawking, J.M. Stewart, A natural measure on the set of all universes Nuclear Physics. ,vol. 281, pp. 736- 751 ,(1987) , 10.1016/0550-3213(87)90425-1
S.W. Hawking, The Quantum State of the Universe Nuclear Physics. ,vol. 239, pp. 257- 276 ,(1984) , 10.1016/0550-3213(84)90093-2
M. Henneaux, The Gibbs entropy production in general relativity Lettere Al Nuovo Cimento Series 2. ,vol. 38, pp. 609- 614 ,(1983) , 10.1007/BF02782751
A D Linde, The inflationary Universe Reports on Progress in Physics. ,vol. 47, pp. 925- 986 ,(1984) , 10.1088/0034-4885/47/8/002
D N Page, A fractal set of perpetually bouncing universe Classical and Quantum Gravity. ,vol. 1, pp. 417- 427 ,(1984) , 10.1088/0264-9381/1/4/015
S.W. Hawking, D.N. Page, Operator ordering and the flatness of the universe Nuclear Physics. ,vol. 264, pp. 185- 196 ,(1986) , 10.1016/0550-3213(86)90478-5
A.D. Linde, Chaotic inflation Physics Letters B. ,vol. 129, pp. 177- 181 ,(1983) , 10.1016/0370-2693(83)90837-7