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NASA NTRS ยท 19760043169

Lagrangian density for collisional plasma

Abstract

For the purpose of deriving appropriate Lagrangians for plasma equations that include effects of energy loss, the paper examines the inverse problem of the calculus of variations for systems of first- and second-order quasi-linear partial differential equations. This results in convenient forms of the sufficient conditions under which the given differential equations are Euler-Lagrange equations of a Lagrangian. These conditions are then applied to determine the necessary transformation that converts equations, apparently not already in it, into Euler-Lagrange form. The appropriate Lagrangian for a warm collisional plasma is obtained, and the Lagrangian is derived for a resistive transmission line.

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BibTeXRIS

Peng, Y.-K. M.. 1976-02-01. Lagrangian density for collisional plasma. https://ntrs.nasa.gov/citations/19760043169

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