Explosive 发表于 2025-3-23 11:51:09

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致词 发表于 2025-3-23 17:31:02

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卷发 发表于 2025-3-23 22:00:38

https://doi.org/10.1007/978-3-662-62542-2nd Coley and references therein). Exact spatially homogeneous solutions were first displayed in early papers ; however, it was not until after 1985 that many of them were recognized by Wainwright and Rosquist and Jantzen as being selfsimilar. The complete set of self-simil

松果 发表于 2025-3-23 23:17:10

,Einführung in die werteorientierte Führung,-interacting scalar field with an exponential potential in the class of Bianchi type B models (except for the exceptional case Bianchi VI.), using the Hewitt and Wainwright formalism . In particular, we shall study the generality of the scaling solutions. We define the governing equations

GEON 发表于 2025-3-24 03:14:42

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临时抱佛脚 发表于 2025-3-24 06:30:54

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的阐明 发表于 2025-3-24 14:26:27

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减少 发表于 2025-3-24 15:31:22

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arbovirus 发表于 2025-3-24 20:57:32

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担心 发表于 2025-3-25 00:21:30

Trendüberwachung über Lebensdauer determine (among other things) whether models evolve from a low-curvature regime and thereby test the self-consistency of the low-energy effective string cosmology paradigm. In particular, we consider the class of “isotropic curvature” models , which are spatially homogeneous but contain
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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