966 resultados para Stochastic Ordinary Differential Equations


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Differential equations are equations that involve an unknown function and derivatives. Euler's method are efficient methods to yield fairly accurate approximations of the actual solutions. By manipulating such methods, one can find ways to provide good approximations compared to the exact solution of parabolic partial differential equations and nonlinear parabolic differential equations.

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Schrödinger’s equation of a three-body system is a linear partial differential equation (PDE) defined on the 9-dimensional configuration space, ℝ9, naturally equipped with Jacobi’s kinematic metric and with translational and rotational symmetries. The natural invariance of Schrödinger’s equation with respect to the translational symmetry enables us to reduce the configuration space to that of a 6-dimensional one, while that of the rotational symmetry provides the quantum mechanical version of angular momentum conservation. However, the problem of maximizing the use of rotational invariance so as to enable us to reduce Schrödinger’s equation to corresponding PDEs solely defined on triangular parameters—i.e., at the level of ℝ6/SO(3)—has never been adequately treated. This article describes the results on the orbital geometry and the harmonic analysis of (SO(3),ℝ6) which enable us to obtain such a reduction of Schrödinger’s equation of three-body systems to PDEs solely defined on triangular parameters.

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Mode of access: Internet.

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"Only the material on elliptic equations will appear in these notes."

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Mode of access: Internet.

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Mimeographed.

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Bibliography: p. 165-170.

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Bibliography: p. 27-28.

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Supported in part by National Science Foundation under Grant No. U.S. NSF-GJ-328.

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Thesis - University of Illinois at Urbana-Champaign.

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Includes bibliographical references (20).

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Vita.

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Includes bibliographies (p. 11).

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Contiene: Vol. supplementary.

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Mode of access: Internet.