Mathieu function

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In mathematics, the Mathieu functions are solutions to the Mathieu differential equation, which is

The Mathieu functions are used in treating problems involving parametric resonance, vibrating elliptical drumheads, and gravitational waves in general relativity, among other applications. They were introduced by Emile Mathieu in 1868 in the context of the second problem.

Floquet solution

According to Floquet's theorem, for fixed values of a,q, Mathieu's equation admits a complex valued solution of form

 

where   is a complex number, the Mathieu exponent, and P is a complex valued function which is periodic with period  . However, P is in general not sinusoidal. In the example plotted below,   (real part, red; imaginary part; green):

 

Mathieu sine and cosine

For fixed a,q, the Mathieu cosine   is a function of   defined as the unique solution of the Mathieu equation which

  1. takes the value  ,
  2. is an even function, or equivalently  .

Similarly, the Mathieu sine   is the unique solution which

  1. takes the value  ,
  2. is an odd function, or equivalently  .

These are closely related to the Floquet solution:

 
 

For small values of q, these functions do resemble sine and cosine near the origin. In the example plotted below (same values of a,q as above), the Mathieu cosine is plotted in red and cosine in green:

File:MathieuCosine example.gif

For this example, the McLaurin series is

 

Periodic solutions

For countably many special values of a, called characteristic values, the Mathieu equation admits solutions which are periodic with period  . The characteristic values of the Mathiue cosine, sine functions respectively are written  , where n in N. Here are the first few periodic Mathieu cosine functions:

 

Here,   (red) is sinusoidal, but none of the others are. For example,   (green) is too flat near the origin to be sinusoidal.

Symbolic computation engines

Various special functions related to the Mathieu functions are implemented in Maple and Mathematica.

References

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