2010
DOI: 10.1007/jhep04(2010)036
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Strange attractors in dissipative Nambu mechanics: classical and quantum aspects

Abstract: We extend the framework of Nambu-Hamiltonian Mechanics to include dissipation in R 3 phase space. We demonstrate that it accommodates the phase space dynamics of low dimensional dissipative systems such as the much studied Lorenz and Rössler Strange attractors, as well as the more recent constructions of Chen and Leipnik-Newton. The rotational, volume preserving part of the flow preserves in time a family of two intersecting surfaces, the so called Nambu Hamiltonians. They foliate the entire phase space and ar… Show more

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Cited by 10 publications
(19 citation statements)
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“…By fixing r in the -Lorenz system and taking the limit → 0 we recover the nondissipative Lorenz system of eq.(1.4). It is integrable and describes the motion of a particle in an one dimensional anharmonic potential [1]( or the pendulum). We can still rescale this sytem by choosing λ = 1 √ r and we discover the infinite r limit of the full Lorenz system, which has been studied in detail in ref.…”
Section: Some Remarks Are In Odermentioning
confidence: 99%
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“…By fixing r in the -Lorenz system and taking the limit → 0 we recover the nondissipative Lorenz system of eq.(1.4). It is integrable and describes the motion of a particle in an one dimensional anharmonic potential [1]( or the pendulum). We can still rescale this sytem by choosing λ = 1 √ r and we discover the infinite r limit of the full Lorenz system, which has been studied in detail in ref.…”
Section: Some Remarks Are In Odermentioning
confidence: 99%
“…We choose to work with the Cylinder intersecting with a Paraboloid as the two Nambu "Hamiltonians" among the whole set of SL(2,R) geometries [1].…”
Section: Figure 2: Lorenz ζ Dissipation Parametermentioning
confidence: 99%
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“…Névir and Blender [22] developed a Nambu representation of the nondissipative parts of the classical Lorenz-63 [12] model for X 1 , Y 2 , and Z 1 (see also [1,24,3] and [25] for a classification). With the conservation laws for H and C the Lorenz equations are in terms of x = (X 1 , Y 2 , Z 1 )…”
Section: Nambu Structurementioning
confidence: 99%