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Everything about Wave Vector totally explained

A wave vector is a vector representation of a wave. The wave vector has magnitude indicating wavenumber (reciprocal of wavelength), and the direction of the vector indicates the direction of wave propagation. The wave vector is most useful for generalizing the equation of a single wave into a description of a family of waves. As long as the family of waves all travel in the same direction and with the same wavelength, a single wave vector is valid for the entire family. The most common case of a family of waves that meets these requirements is the plane wave, in which the family of waves is also coherent, for example all the waves have the same phase.
   For example, a common representation of a single wave at a single point in space is: » psi left(t ight) = A cos left(varphi + omega t ight)

where A is the amplitude, ω is the angular frequency, and φ is the starting phase of the wave (the independent variable t is time).
   In order to generalize the equation to all points in the one-dimensional space of the direction of propagation, we add in an additional phase offset term: » psi left(t, z ight) = A cos left(varphi + k z + omega t ight)

where k is the wavenumber (2π/λ) and the new independent variable z is the distance along the wave.
   Now, as long as we're dealing with a simple family of waves, with identical direction, wavelength, and phase (for example a plane wave), we can easily extend the formula by substituting the wave vector k for the wavenumber k, and the location in space vector r for the variable z: » psi left(t, ,

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