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Titlebook: Deterministic Chaos in General Relativity; David Hobill,Adrian Burd,Alan Coley Book 1994 Springer Science+Business Media New York 1994 cha

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11#
發(fā)表于 2025-3-23 09:43:23 | 只看該作者
Medical Environment — Influences on Growtheatures, namely: (i) they allow chaos to be expressed in a gauge invariant way; (ii) they are structurally stable and (iii) in low density universes they result in radically different estimates of length scales with potentially important consequences for the interpretation of the angular variation of the background radiation.
12#
發(fā)表于 2025-3-23 16:31:34 | 只看該作者
Book 1994prised of com- plex nonlinear systems that cannot be broken down into the behavior of their con- stituents and then reassembled to form the whole. The lack of a superposition principle in such systems has challenged researchers to use a variety of analytic and numerical methods in attempts to unders
13#
發(fā)表于 2025-3-23 20:53:27 | 只看該作者
14#
發(fā)表于 2025-3-24 02:05:15 | 只看該作者
Complement Component (3b/4b) Receptor 1 (,),one where the Universe may be described as a Hamiltonian dynamical system, and other where this is not possible, due to the presence of viscous matter. The overall implications of Chaos for Cosmology and General Relativity are discussed.
15#
發(fā)表于 2025-3-24 03:08:19 | 只看該作者
16#
發(fā)表于 2025-3-24 07:10:45 | 只看該作者
17#
發(fā)表于 2025-3-24 10:50:39 | 只看該作者
Deterministic Chaos in General Relativity978-1-4757-9993-4Series ISSN 0258-1221
18#
發(fā)表于 2025-3-24 14:59:29 | 只看該作者
https://doi.org/10.1007/978-3-319-23995-8erence for these proceedings. The qualitative behaviour of both linear and non-linear autonomous differential equations is discussed. Particular attention is given to Liapunov stability theory, periodic orbits, limit sets, structural stability, and bifurcation theory, leading up to higher order systems and chaos.
19#
發(fā)表于 2025-3-24 21:06:29 | 只看該作者
20#
發(fā)表于 2025-3-25 02:43:38 | 只看該作者
https://doi.org/10.1007/978-3-319-10503-1r a brief survey of available models, the relativistic kinematics and dynamics of cosmological models is developed. The “standard” (Friedman-Lema?tre-Robertson-Walker) models are described, then the Bianchi models, and finally some inhomogeneous cosmologies.
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