For a holomorphic function with , the chain rule gives
Writing and equating real parts and imaginary parts,
For , division by gives the Cauchy-Riemann equations in polar coordinates:
The restriction reflects the coordinate singularity at the origin; the Cartesian equations have no such restriction.
Insert the specified real part into the polar Cauchy-Riemann equations. The first gives , and integration with respect to gives
The second equation then requires , so . The remaining imaginary additive constant is fixed by . Thus
The resulting polynomial is holomorphic at the origin too, consistently extending the calculation made in polar coordinates with .
Using the exponential form of the complex cosine, is equivalent to . Thus the zeros are exactly
At each point , so the cosine has a simple zero. Cubing it gives
The order of a zero of a holomorphic function is therefore three at every zero. There are no finite singularities because this is an entire function.
To classify infinity, examine at . The identity shows that its Laurent series contains the nonzero negative-power coefficients
There are infinitely many terms in the principal part, the criterion for an essential singularity. Therefore This is also the general characterization of a nonpolynomial entire function at infinity.
If , factor out and use the geometric series:
Thus
The radius of convergence is the distance to the nearest singularity, the simple pole at . The case must be treated separately: the function is , has no Taylor series about zero and is already its own Laurent series on .
For , multiply the absolutely convergent Taylor series of the sine by the geometric series:
The product is odd, so all even coefficients vanish. Collecting the coefficient of gives
For example, the first terms are . The denominator vanishes at , and the numerator is nonzero there, so these are genuine simple poles. Therefore is the radius of convergence.

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