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  2. Wave - Wikipedia

    en.wikipedia.org/wiki/Wave

    The analytical solution of SV-wave in a half-space indicates that the plane SV wave reflects back to the domain as a P and SV waves, leaving out special cases. The angle of the reflected SV wave is identical to the incidence wave, while the angle of the reflected P wave is greater than the SV wave.

  3. Electromagnetic radiation - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_radiation

    where v is the speed of the wave (c in a vacuum or less in other media), f is the frequency and λ is the wavelength. As waves cross boundaries between different media, their speeds change but their frequencies remain constant. Electromagnetic waves in free space must be solutions of Maxwell's electromagnetic wave equation. Two main classes of ...

  4. List of equations in wave theory - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in_wave...

    Position of a point in space, not necessarily a point on the wave profile or any line of propagation d, r: m [L] Wave profile displacement Along propagation direction, distance travelled (path length) by one wave from the source point r 0 to any point in space d (for longitudinal or transverse waves) L, d, r

  5. Wave equation - Wikipedia

    en.wikipedia.org/wiki/Wave_equation

    By comparison with vector wave equations, the scalar wave equation can be seen as a special case of the vector wave equations; in the Cartesian coordinate system, the scalar wave equation is the equation to be satisfied by each component (for each coordinate axis, such as the x component for the x axis) of a vector wave without sources of waves ...

  6. Relativistic wave equations - Wikipedia

    en.wikipedia.org/wiki/Relativistic_wave_equations

    The direct derivation of the Dirac-Pauli-Fierz equations using the Bargmann-Wigner operators is given in. [6] In 1941, Rarita and Schwinger focussed on spin- 3 ⁄ 2 particles and derived the Rarita–Schwinger equation , including a Lagrangian to generate it, and later generalized the equations analogous to spin n + 1 ⁄ 2 for integer n .

  7. De Broglie–Bohm theory - Wikipedia

    en.wikipedia.org/wiki/De_Broglie–Bohm_theory

    The evolution over time of the configuration of all particles is defined by a guiding equation. The evolution of the wave function over time is given by the Schrödinger equation. The theory is named after Louis de Broglie (1892–1987) and David Bohm (1917–1992).

  8. Wavelength - Wikipedia

    en.wikipedia.org/wiki/Wavelength

    A wave packet has an envelope that describes the overall amplitude of the wave; within the envelope, the distance between adjacent peaks or troughs is sometimes called a local wavelength. [21] [22] An example is shown in the figure. In general, the envelope of the wave packet moves at a speed different from the constituent waves. [23]

  9. Speed of light - Wikipedia

    en.wikipedia.org/wiki/Speed_of_Light

    The speed at which light waves propagate in vacuum is independent both of the motion of the wave source and of the inertial frame of reference of the observer. [ Note 5 ] This invariance of the speed of light was postulated by Einstein in 1905, [ 6 ] after being motivated by Maxwell's theory of electromagnetism and the lack of evidence for ...

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