{"title":"洛伦兹系统的标度性质与耗散南布力学","authors":"M. Axenides, E. Floratos","doi":"10.1142/9789814602136_0002","DOIUrl":null,"url":null,"abstract":"In the framework of Nambu Mechanics, we have recently argued that Non-Hamiltonian Chaotic Flows in $ R^{3} $, are dissipation induced deformations, of integrable volume preserving flows, specified by pairs of Intersecting Surfaces in $R^{3}$. In the present work we focus our attention to the Lorenz system with a linear dissipative sector in its phase space dynamics. In this case the Intersecting Surfaces are Quadratic. We parametrize its dissipation strength through a continuous control parameter $\\epsilon$, acting homogeneously over the whole 3-dim. phase space. In the extended $\\epsilon$-Lorenz system we find a scaling relation between the dissipation strength $ \\epsilon $ and Reynolds number parameter r . It results from the scale covariance, we impose on the Lorenz equations under arbitrary rescalings of all its dynamical coordinates. Its integrable limit, ($ \\epsilon = 0 $, \\ fixed r), which is described in terms of intersecting Quadratic Nambu \"Hamiltonians\" Surfaces, gets mapped on the infinite value limit of the Reynolds number parameter (r $\\rightarrow \\infty,\\ \\epsilon= 1$). In effect weak dissipation, through small $\\epsilon$ values, generates and controls the well explored Route to Chaos in the large r-value regime. The non-dissipative $\\epsilon=0 $ integrable limit is therefore the gateway to Chaos for the Lorenz system.","PeriodicalId":166772,"journal":{"name":"arXiv: Chaotic Dynamics","volume":"391 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2012-05-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Scaling Properties of the Lorenz System and Dissipative Nambu Mechanics\",\"authors\":\"M. Axenides, E. Floratos\",\"doi\":\"10.1142/9789814602136_0002\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In the framework of Nambu Mechanics, we have recently argued that Non-Hamiltonian Chaotic Flows in $ R^{3} $, are dissipation induced deformations, of integrable volume preserving flows, specified by pairs of Intersecting Surfaces in $R^{3}$. In the present work we focus our attention to the Lorenz system with a linear dissipative sector in its phase space dynamics. In this case the Intersecting Surfaces are Quadratic. We parametrize its dissipation strength through a continuous control parameter $\\\\epsilon$, acting homogeneously over the whole 3-dim. phase space. In the extended $\\\\epsilon$-Lorenz system we find a scaling relation between the dissipation strength $ \\\\epsilon $ and Reynolds number parameter r . It results from the scale covariance, we impose on the Lorenz equations under arbitrary rescalings of all its dynamical coordinates. Its integrable limit, ($ \\\\epsilon = 0 $, \\\\ fixed r), which is described in terms of intersecting Quadratic Nambu \\\"Hamiltonians\\\" Surfaces, gets mapped on the infinite value limit of the Reynolds number parameter (r $\\\\rightarrow \\\\infty,\\\\ \\\\epsilon= 1$). In effect weak dissipation, through small $\\\\epsilon$ values, generates and controls the well explored Route to Chaos in the large r-value regime. The non-dissipative $\\\\epsilon=0 $ integrable limit is therefore the gateway to Chaos for the Lorenz system.\",\"PeriodicalId\":166772,\"journal\":{\"name\":\"arXiv: Chaotic Dynamics\",\"volume\":\"391 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2012-05-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv: Chaotic Dynamics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1142/9789814602136_0002\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Chaotic Dynamics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1142/9789814602136_0002","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Scaling Properties of the Lorenz System and Dissipative Nambu Mechanics
In the framework of Nambu Mechanics, we have recently argued that Non-Hamiltonian Chaotic Flows in $ R^{3} $, are dissipation induced deformations, of integrable volume preserving flows, specified by pairs of Intersecting Surfaces in $R^{3}$. In the present work we focus our attention to the Lorenz system with a linear dissipative sector in its phase space dynamics. In this case the Intersecting Surfaces are Quadratic. We parametrize its dissipation strength through a continuous control parameter $\epsilon$, acting homogeneously over the whole 3-dim. phase space. In the extended $\epsilon$-Lorenz system we find a scaling relation between the dissipation strength $ \epsilon $ and Reynolds number parameter r . It results from the scale covariance, we impose on the Lorenz equations under arbitrary rescalings of all its dynamical coordinates. Its integrable limit, ($ \epsilon = 0 $, \ fixed r), which is described in terms of intersecting Quadratic Nambu "Hamiltonians" Surfaces, gets mapped on the infinite value limit of the Reynolds number parameter (r $\rightarrow \infty,\ \epsilon= 1$). In effect weak dissipation, through small $\epsilon$ values, generates and controls the well explored Route to Chaos in the large r-value regime. The non-dissipative $\epsilon=0 $ integrable limit is therefore the gateway to Chaos for the Lorenz system.