shrill 发表于 2025-3-28 18:37:26

Closed Models,lysis. In this Chapter we shall discuss the qualitative properties of the positive-curvature FRW models and the Kantowski-Sachs models with a barotropic fluid and a non-interacting scalar field with an exponential potential .

小隔间 发表于 2025-3-28 21:33:02

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巫婆 发表于 2025-3-28 23:31:46

Introduction,al cosmology involves the study of the early- and late- time behaviour of more general classes of cosmological models as well as the detailed investigation of special exact cosmological solutions with symmetries such as the spatially homogeneous and isotropic models with a Robertson-Walker (RW) geom

慢跑 发表于 2025-3-29 04:41:05

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津贴 发表于 2025-3-29 09:50:08

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Seminar 发表于 2025-3-29 12:58:28

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Entirety 发表于 2025-3-29 15:46:35

Multiple Scalar Fields,7] . There are a variety of inflationary models which include scalar fields , and in scalar field models with an exponential potential the universe inflates at a power-law rate, .(.) ∞ .., where . > 1 . As we have seen, all ever-expanding scalar field models with an exponential poten

defibrillator 发表于 2025-3-29 21:59:00

Scalar Tensor Theories of Gravity,string theory (see and references therein) . The first scalar-tensor theories to appear (with . = .. ) were due to Jordan , Fierz and Brans and Dicke and the most general scalar-tensor theories were formulated by Bergmann , Nordtvedt and Wagoner . The obser

osteocytes 发表于 2025-3-30 03:19:24

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set598 发表于 2025-3-30 05:22:42

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查看完整版本: Titlebook: Dynamical Systems and Cosmology; A. A. Coley Book 2003 Springer Science+Business Media Dordrecht 2003 Cosmology.EFE.Gravity.Potential.Rela