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Titlebook: Nonlinear Stability of Structures; Theory and Computati A. N. Kounadis,W. B. Kr?tzig Book 1995 CISM Udine 1995 chaos.dynamics.instability.n

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11#
發(fā)表于 2025-3-23 12:59:51 | 只看該作者
On the Stability and Bifurcation Phenomena Associated with Dynamical Systemsystems, and both static and dynamic bifurcations associated with such systems are explored analytically. Thus, Hopf and degenerate Hopf bifurcations, as well as bifurcations into quasi-periodic motions on invariant tori are analysed. A brief discussion concerning the analysis of non-autonomous systems is presented in the last chapter.
12#
發(fā)表于 2025-3-23 16:48:59 | 只看該作者
Applicationsected to high temperature gradients due to intense heating by the sun and cooling in the shadow. When the deformations of such structures are constrained, then buckling may occur which leads to local or global instabilities associated with large undesirable deflections.
13#
發(fā)表于 2025-3-23 18:57:03 | 只看該作者
CISM International Centre for Mechanical Scienceshttp://image.papertrans.cn/n/image/667691.jpg
14#
發(fā)表于 2025-3-24 00:37:33 | 只看該作者
15#
發(fā)表于 2025-3-24 03:41:31 | 只看該作者
16#
發(fā)表于 2025-3-24 09:31:48 | 只看該作者
ical equilibria of gas mixtures. It is based on a book by one of the authors, published in Czech by the Publishing House Academia in Prague. The rapid development of the topic during the two years since publication of the Czech edition has made it necessary to revise practically all the sections in
17#
發(fā)表于 2025-3-24 11:58:47 | 只看該作者
V. V. Bolotinical equilibria of gas mixtures. It is based on a book by one of the authors, published in Czech by the Publishing House Academia in Prague. The rapid development of the topic during the two years since publication of the Czech edition has made it necessary to revise practically all the sections in
18#
發(fā)表于 2025-3-24 18:13:32 | 只看該作者
19#
發(fā)表于 2025-3-24 20:13:12 | 只看該作者
20#
發(fā)表于 2025-3-25 02:24:45 | 只看該作者
K. Huseyinl evolution. In the following one should keep in mind that the stellar evolution results are influenced by the physics adopted in the models. In particular, two physical processes are important in determining the galactic chemical enrichment, the mass loss occurring during various phases of stellar
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