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  2. Polar motion - Wikipedia

    en.wikipedia.org/wiki/Polar_motion

    This is the so-called polar motion. [8] Observations show that the figure axis exhibits an annual wobble forced by surface mass displacement via atmospheric and/or ocean dynamics, while the free nutation is much larger than the Euler period and of the order of 435 to 445 sidereal days. This observed free nutation is called Chandler wobble.

  3. Vicsek model - Wikipedia

    en.wikipedia.org/wiki/Vicsek_model

    The Vicsek model is a mathematical model used to describe active matter. One motivation of the study of active matter by physicists is the rich phenomenology associated to this field. Collective motion and swarming are among the most studied phenomena.

  4. Polariton - Wikipedia

    en.wikipedia.org/wiki/Polariton

    A polariton is the result of the combination of a photon with a polar excitation in a material. The following are types of polaritons: Phonon polaritons result from coupling of an infrared photon with an optical phonon; Exciton polaritons result from coupling of visible light with an exciton [12]

  5. Schrödinger equation - Wikipedia

    en.wikipedia.org/wiki/Schrödinger_equation

    The motion of the electron is of principal interest here, so the equivalent one-body problem is the motion of the electron using the reduced mass. The Schrödinger equation for a hydrogen atom can be solved by separation of variables. [24] In this case, spherical polar coordinates are the most convenient.

  6. Toroidal moment - Wikipedia

    en.wikipedia.org/wiki/Toroidal_moment

    In condensed matter magnetic toroidal order can be induced by different mechanisms: [7] Order of localized spins breaking spatial inversion and time reversal. The resulting toroidal moment is described by a sum of cross products of the spins S i of the magnetic ions and their positions r i within the magnetic unit cell: [8] T = Σ i r i × S i

  7. International Earth Rotation and Reference Systems Service

    en.wikipedia.org/wiki/International_Earth...

    The IERS was established in its present form in 1987 by the International Astronomical Union and the International Union of Geodesy and Geophysics, replacing the earlier International Polar Motion Service (IPMS) and the Earth rotation section of the Bureau International de l'Heure (BIH). The service began operation on January 1, 1988.

  8. Geodesics in general relativity - Wikipedia

    en.wikipedia.org/wiki/Geodesics_in_general...

    This formulation of the geodesic equation of motion can be useful for computer calculations and to compare General Relativity with Newtonian Gravity. [1] It is straightforward to derive this form of the geodesic equation of motion from the form which uses proper time as a parameter using the chain rule. Notice that both sides of this last ...

  9. Maxwell's equations in curved spacetime - Wikipedia

    en.wikipedia.org/wiki/Maxwell's_equations_in...

    When working in the presence of bulk matter, distinguishing between free and bound electric charges may facilitate analysis. When the distinction is made, they are called the macroscopic Maxwell's equations. Without this distinction, they are sometimes called the "microscopic" Maxwell's equations for contrast.