Bound Motion of Bodies and Paticles in the Rotating Systems

Details Bound Motion of Bodies and Paticles in the Rotating Systems Bound Motion of Bodies and Paticles in the Rotating Systems

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ijtp...46..848p&link_type=abstract

International Journal of Theoretical Physics, Volume 46, Issue 4, pp.848-859

Physics

Foucault Pendulum, Triangle Pendulum, Gyroscope, Rotating Galaxy, Lorentz Equation, Bargmann-Michel-Telegdi Equation

Scientific paper

The Lagrange theory of particle motion in the noninertial systems is applied to the Foucault pendulum, isosceles triangle pendulum and the general triangle pendulum swinging on the rotating Earth. As an analogue, planet orbiting in the rotating galaxy is considered as the giant galactic gyroscope. The Lorentz equation and the Bargmann-Michel-Telegdi equations are generalized for the rotation system. The knowledge of these equations is inevitable for the construction of LHC where each orbital proton “feels” the Coriolis force caused by the rotation of the Earth.

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