2010
DOI: 10.2478/s11534-010-0004-1
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Magnetohydrodynamic flows as Newtonian-type gravitational motions

Abstract: Abstract:We study the motion of a magnetised, highly conductive fluid within the framework of Newtonian gravity. Our analysis examines whether and under what conditions magnetohydrodynamic flows can be represented as hydrodynamic ones and then as Newtonian-type gravitational motions. In the latter case we define a generalised effective density and an effective Poisson-type potential, which include the magnetic input and determine the dynamics of the magnetised system. Introducing the dynamical equivalence of t… Show more

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Cited by 2 publications
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“…Furthermore, in the stellar and galactic levels, the notion of the repulsive gravity, predicted in the dynamical-equivalence approach, can be used to tackle problems like the formation of the (stellar and galactic) winds, and, in the case of magnetohydrodynamic flows, of the (stellar and galactic) jets [15] .…”
Section: Applicationsmentioning
confidence: 99%
“…Furthermore, in the stellar and galactic levels, the notion of the repulsive gravity, predicted in the dynamical-equivalence approach, can be used to tackle problems like the formation of the (stellar and galactic) winds, and, in the case of magnetohydrodynamic flows, of the (stellar and galactic) jets [15] .…”
Section: Applicationsmentioning
confidence: 99%