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Polypolar coordination and symmetries
Computer Research and Modeling, 2010, v. 2, no. 4, pp. 329-341Views (last year): 1.The polypolar system of coordinates is formed by a family of a parametrized on a radius isofocal of kf-lemniscates. As well as the classical polar system of coordinates, it characterizes a point of a plane by a polypolar radius ρ and polypolar angle φ. For anyone connectedness a family isometric of curve ρ = const – lemniscates and family gradient of curves φ = const – are mutually orthogonal conjugate coordinate families. The singularities of polypolar coordination, its symmetry, and also curvilinear symmetries on multifocal lemniscates are considered.
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Wandering symmetries of the Lagrange's equations
Computer Research and Modeling, 2010, v. 2, no. 1, pp. 13-17Views (last year): 4.The dynamic process can be in equal degree adequately prototyped by a family of Lagrange's systems. Symmetry group ‘wanders’ on this family: systems are transformed from one into another. In this work we show that under determined condition the first integral can be obtained by a simple calculations on some of such groups. The main purpose of the work is to show usefulness of wandering symmetry concept. The considered example: flat motion of a charged particle in magnetic field in presence of viscous friction. With the help of three wandering symmetry first integral is calculated.
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Symmetries of the Hamilton–Jacobi equation
Computer Research and Modeling, 2012, v. 4, no. 2, pp. 253-265Views (last year): 1. Citations: 1 (RSCI).The notion of symmetry transformations of the Hamilton–Jacobi equation. For the group of symmetries is shown how to be associated with the Hamiltonian function coefficients of the infinitesimal operator of the group. The examples of calculation of the symmetries and examples calculations based on the full symmetry of the integrals.
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Integration the relativistic wave equations in Bianchi IX cosmology model
Computer Research and Modeling, 2016, v. 8, no. 3, pp. 433-443We consider integration Clein–Gordon and Dirac equations in Bianchi IX cosmology model. Using the noncommutative integration method we found the new exact solutions for Taub universe.
Noncommutative integration method for Bianchi IX model is based on the use of the special infinite-dimensional holomorphic representation of the rotation group, which is based on the nondegenerate orbit adjoint representation, and complex polarization of degenerate covector. The matrix elements of the representation of form a complete and orthogonal set and allow you to use the generalized Fourier transform. Casimir operator for rotation group under this transformation becomes constant. And the symmetry operators generated by the Killing vector fields in the linear differential operators of the first order from one dependent variable. Thus, the relativistic wave equation on the rotation group allow non-commutative reduction to ordinary differential equations. In contrast to the well-known method of separation of variables, noncommutative integration method takes into account the non-Abelian algebra of symmetry operators and provides solutions that carry information about the non-commutative symmetry of the task. Such solutions can be useful for measuring the vacuum quantum effects and the calculation of the Green’s functions by the splitting-point method.
The work for the Taub model compared the solutions obtained with the known, which are obtained by separation of variables. It is shown that the non-commutative solutions are expressed in terms of elementary functions, while the known solutions are defined by the Wigner function. And commutative reduced by the Klein–Gordon equation for Taub model coincides with the equation, reduced by separation of variables. A commutative reduced by the Dirac equation is equivalent to the reduced equation obtained by separation of variables.
Keywords: noncommutative integration, Bianchi IX.Views (last year): 5. -
Orbits in the two-body problem in terms of symmetries
Computer Research and Modeling, 2011, v. 3, no. 1, pp. 39-45For the two-body problem computed 12-parameter group symmetry transformations which translate the obvious solution — uniform motion of bodies in circular orbits with a common fixed center — a motion with arbitrary initial data.
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International Interdisciplinary Conference "Mathematics. Computing. Education"