From the Foucault pendulum to the galactical gyroscope and LHC

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dc.creatorPardy, Miroslav
dc.date2006-01-17
dc.date.accessioned2026-07-07T06:57:00Z
dc.date.available2026-07-07T06:57:00Z
dc.descriptionWe consider the Foucault pendulum, isosceles triangle pendulum and the general triangle pendulum rotating on the Earth. As an analogue, planet orbiting in the rotating galaxy is considered as the giant galactical gyroscope. The Lorentz and the Bargman-Michel-Telegdi equations are generalized for the rotating system. These equations are inevitable for LHC where orbital photons "feels" the Coriolis force caused by the rotation ofthe Earth.
dc.description10 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0601365
dc.identifierhttp://arxiv.org/abs/astro-ph/0601365
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/106810
dc.subjectAstrophysics
dc.titleFrom the Foucault pendulum to the galactical gyroscope and LHC
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