松紧带 发表于 2025-3-23 12:59:51
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.jealousy 发表于 2025-3-23 16:48:59
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.恶名声 发表于 2025-3-23 18:57:03
CISM International Centre for Mechanical Scienceshttp://image.papertrans.cn/n/image/667691.jpg付出 发表于 2025-3-24 00:37:33
http://reply.papertrans.cn/67/6677/667691/667691_14.pngKinetic 发表于 2025-3-24 03:41:31
http://reply.papertrans.cn/67/6677/667691/667691_15.pngmutineer 发表于 2025-3-24 09:31:48
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衣服 发表于 2025-3-24 11:58:47
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艰苦地移动 发表于 2025-3-24 18:13:32
http://reply.papertrans.cn/67/6677/667691/667691_18.pngmalapropism 发表于 2025-3-24 20:13:12
http://reply.papertrans.cn/67/6677/667691/667691_19.png安慰 发表于 2025-3-25 02:24:45
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