Abstract
Generalized Jacobi's equation is derived by introducing the friction force into the equations of motion of mass points constituting the system.
The exact solution of the equation of virial oscillations of celestial bodies written for non-conservative systems is obtained using non-linear time scale in the course of the change of variables for a particular friction force law.
The nature of the undamped virial oscillations of celestial bodies is though to be related to the system unstability near the state determined by the virial theorem. Thus, the friction force changes its sign near the unstable equilibrium state and due to dissipation of energy during evolution of the system the undamped virial oscillations can be described as self-exited oscillations.
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References
Bogolubov, N. N. and Mitropolsky, Yu. A.: 1974,Asymptotic Methods in the Theory of Nonlinear Oscillations, Nauka, Moscow.
Lightman, A. P. and Shapiro, S. L.: 1978,Rev. Mod. Phys. 50, 437.
Ferronsky, V. I., Denisik, S. A., and Ferronsky, S. V.: 1978,Celest. Mech. 18, 113.
Ferronsky, V. I., Denisik, S. A., and Ferronsky, S. V.: 1979,Celest. Mech. 20, 143.
Ferronsky, V. I., Denisik, S. A., and Ferronsky, S. V.: 1981,Celest. Mech. 23, 243.
Ferronsky, V. I., Denisik, S. A., and Ferronsky, S. V.: 1982,Celest. Mech. 27, 285.
Ferronsky, V. I., Denisik, S. A., and Ferronsky, S. V.: 1984,Celest. Mech. (in press).
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Ferronsky, V.I., Denisik, S.A. & Ferronsky, S.V. Virial oscillations of celestial bodies III. The solution of the evolutionary problem in non-newtonian time scale. Celestial Mechanics 32, 173–183 (1984). https://doi.org/10.1007/BF01231124
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DOI: https://doi.org/10.1007/BF01231124