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

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21#
發(fā)表于 2025-3-25 03:55:37 | 只看該作者
Trendüberwachung über Lebensdaueroduli space of a more fundamental, non-perturbative theory known as M-theory [376], and so no particular string theory is necessarily more fundamental since they are all related by duality symmetries (for a review see, e.g., Ref. [321]). Moreover, another point of this moduli space corresponds to el
22#
發(fā)表于 2025-3-25 11:32:56 | 只看該作者
23#
發(fā)表于 2025-3-25 12:37:37 | 只看該作者
,Einführung in die werteorientierte Führung, differential equations (ODE). Inhomogeneous cosmological models can also be studied, but since the evolution equations are autonomous partial differential equations (PDE) in this case the resulting state space is infinite-dimensional (i.e., a function space) , and the analysis is considerably more complicated.
24#
發(fā)表于 2025-3-25 18:17:21 | 只看該作者
Mehr Dinge zwischen Himmel und Erderedict steep exponential potentials [164] (i.e., .. > 2), effectively eliminating the possibility of power-law inflation. However, dimensionally reduced higher-dimensional theories also predict numerous scalar fields, and so it is of interest to study models with multiple scalar fields.
25#
發(fā)表于 2025-3-25 20:17:08 | 只看該作者
Introduction, differential equations (ODE). Inhomogeneous cosmological models can also be studied, but since the evolution equations are autonomous partial differential equations (PDE) in this case the resulting state space is infinite-dimensional (i.e., a function space) , and the analysis is considerably more complicated.
26#
發(fā)表于 2025-3-26 03:59:09 | 只看該作者
Multiple Scalar Fields,redict steep exponential potentials [164] (i.e., .. > 2), effectively eliminating the possibility of power-law inflation. However, dimensionally reduced higher-dimensional theories also predict numerous scalar fields, and so it is of interest to study models with multiple scalar fields.
27#
發(fā)表于 2025-3-26 06:58:42 | 只看該作者
Scalar Tensor Theories of Gravity,] and Brans and Dicke [60] and the most general scalar-tensor theories were formulated by Bergmann [40], Nordtvedt [289] and Wagoner [356] . The observational limits on scalar-tensor theories include solar system tests [2, 59, 64, 189] and cosmological tests such as Big Bang nucleosynthesis constraints [17, 322].
28#
發(fā)表于 2025-3-26 11:00:06 | 只看該作者
M-Theory, since they are all related by duality symmetries (for a review see, e.g., Ref. [321]). Moreover, another point of this moduli space corresponds to eleven-dimensional supergravity. This represents the low-energy limit of M-theory [337, 376] .
29#
發(fā)表于 2025-3-26 14:26:25 | 只看該作者
30#
發(fā)表于 2025-3-26 18:14:15 | 只看該作者
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