After division by , the coefficients are and . At , and are analytic functions, so is a regular singular point. Its indicial equation is . There are no other finite singular points of a differential equation. At infinity the regular singular point criterion for a second-order equation would require , but ; hence infinity is an irregular singular point.
Substituting reduces the equation to , so
A linearly independent pair is and . Their Wronskian is . The second has a removable singularity at and value , whereas the first has a simple pole, agreeing with the two characteristic exponents at a regular singular point, . The integer difference does not require a logarithm. At infinity has an essential singularity, consistent with the irregular singular point; the existence of the simpler solution does not make infinity regular.
One possible open contour begins at along a ray with , avoids the essential singularity at the origin, and ends at infinity along a ray with . For example, when is real, it may leave the origin along the positive real axis, bend through the upper half-plane, and approach the negative real axis as . At its initial end, ; at its final end, . More generally, the terminal ray may be chosen with
so that is negative real. This contour satisfies the endpoint condition from part (a) and therefore produces a solution of the differential equation.
For
both and have a simple zero at zero. Hence has a simple pole, and its residue is
For , multiplication of the two Laurent series shows that all powers are even:
There are infinitely many negative powers, so zero is an essential singularity. There is no term, and therefore
Termwise integration of the exponential series gives
There are infinitely many negative Laurent coefficients, so zero is an essential singularity.
On a punctured neighborhood of the center, an essential singularity occurs exactly when infinitely many negative-power Laurent coefficients are nonzero. If all negative-power coefficients vanish, the singularity is removable; if finitely many are nonzero, the singularity is a pole. The punctured-neighborhood assumption matters: an annulus separated from its center cannot by itself classify the function there.
The exponential power series gives for . Hence all singular terms are
Infinitely many negative powers occur, so zero is an essential singularity.
Put . The identity gives a Laurent series containing a constant and only even negative powers . There is no coefficient, so
The singularity is an essential singularity, not a pole: infinitely many negative Laurent coefficients are nonzero. The residue is still defined as the coefficient of .
The Cauchy-Riemann equations are and . A holomorphic function is smooth, so equality of mixed partial derivatives gives
Thus its real and imaginary parts are harmonic functions.
An entire function is holomorphic at every finite point of the complex plane. The globally convergent power series for the exponential implies that and are entire. Their difference therefore gives
at every complex , proving that the hyperbolic sine is entire. For powers, the base case has derivative one everywhere. If is entire with derivative , the product rule gives everywhere. Induction proves that every positive integer power is entire.
A function has a pole of order at when it is holomorphic in a punctured neighbourhood and extends holomorphically to with . An isolated essential singularity is neither a removable singularity nor a pole; equivalently its Laurent series has infinitely many nonzero negative-power terms. In particular
has an essential singularity at zero.
For , the Laurent series about infinity is
To classify the point correctly, use . Then , and is holomorphic with value one at zero. Therefore
The pole at infinity is compatible with an essential singularity at the finite point zero. Negative powers of are regular powers of the local coordinate near infinity, so they do not make that point essential.
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.
For , singularities occur when , with . Each is a simple pole, since the substitution has nonzero derivative there:
More explicitly, , so and its residue is .
These poles accumulate at zero. Consequently . The removable/pole/essential classification for isolated singularities cannot be applied at that accumulation point; it is not an isolated essential singularity.
Multiply the exponential power series by the two prefactors:
Collecting powers yields the Laurent series
Its first terms are . Infinitely many negative-power coefficients are nonzero, so . The residue is the coefficient of :
The phrase "power series" here refers to a Laurent series; no ordinary Taylor series about an essential singularity exists.
For the first function, the complex exponential has no zeros, while the denominator has three distinct simple zeros. Thus there are . To examine infinity, substitute :
The factor has an essential singularity at zero, and multiplication by a nonzero finite-order factor cannot remove it. Therefore of the first function.
For the second function, has simple zeros at . At zero, its Taylor series gives
so . Every other is a double pole, since the numerator is nonzero there. There are no finite zeros, including after removal at zero.
At infinity the double poles accumulate. Equivalently, after , the function has double poles at tending to zero. Hence . The removable/pole/essential trichotomy for isolated singularities does not apply there; calling this an isolated essential singularity would be incorrect.
Write the Laurent series about as . The isolated singularity is:
These cases exhaust the possible principal parts. The residue is
For the first example, gives
Thus zero is a double pole, with residue zero. For the other example,
so the ratio is . Its singularity is removable, with extended value zero and residue zero. The numerator's zero has higher order than the denominator's, so there is no pole.
For , the denominator vanishes exactly when . Thus set
Each denominator zero is simple, since
Every is purely imaginary and nonzero. The identity for real shows , so there is no cancellation. Each is consequently a simple pole, with residue .
These poles accumulate at zero. Therefore
In particular, zero has no punctured neighbourhood on which the function is holomorphic, so it cannot be classified as a removable singularity, a pole, or an isolated essential singularity. There are no other finite singularities.
The expression is , which is holomorphic for every . At zero,
has infinitely many nonzero negative-power terms, so it has an essential singularity. Multiplication by the nonvanishing entire function preserves that classification: if had a removable singularity or a pole, multiplying by would give the same type for , a contradiction. Hence
We prove the Casorati-Weierstrass theorem by contradiction. Fix an allowed . If the stated image were not a dense set in , there would be a disc disjoint from it. Hence
The holomorphic function is bounded by on that punctured disc. By the permitted Riemann removable singularity theorem, it extends to a holomorphic function on the full disc.
If , then is holomorphic near and agrees with away from . This makes a removable singularity of .
If , then is not identically zero, since is nowhere zero away from . Its Taylor series therefore has a finite first nonzero coefficient: otherwise the identity theorem would make it identically zero. Write with and . Then
has a pole of order at , since multiplying by gives the nonzero limit .
Both cases contradict an essential singularity. Thus
Let . It is holomorphic and nowhere zero on a punctured neighbourhood of , and the chain rule gives
If had a pole of order , part (c) would imply . But the derivative of a holomorphic function on a punctured disc has residue zero. Indeed, write its Laurent series
Termwise differentiation is valid on every smaller closed annulus. The only possible term comes from and has coefficient zero. Thus
a contradiction. Therefore . This proves an exponential has no isolated pole, including when has an essential singularity; no choice of a holomorphic logarithm on the entire punctured disc was assumed.
For , is holomorphic at every finite nonzero point. At zero its Laurent series has infinitely many negative powers, so zero is an essential singularity. If the Riemann sphere is included, has a pole of order at , so infinity is a pole of order .
The apparent singularity at zero cancels: the Taylor series of the sine gives
Thus zero is a removable singularity, with extension . At , the other terms are holomorphic, whereas has a simple pole. Therefore
There are no other finite singularities. If “all” includes the point at infinity on the Riemann sphere, it is an essential singularity: has infinitely many negative powers in its Laurent series at .
Singularities. The complex exponential factors as . The second factor has an essential singularity at zero, and multiplication by the nonvanishing holomorphic function does not remove it. There are no other finite singularities. On the Riemann sphere, infinity is also an essential singularity, since .
Symmetry and integral formula. The identity and uniqueness of the Laurent series on give for every integer . The Laurent coefficient formula, on the positively oriented unit circle, gives
The imaginary part vanishes by the substitution . Hence
Polynomial contour integral. For an integer and integer , the binomial theorem gives . The residue theorem selects , that is . Therefore the correct complete statement is
The printed nonnegative-integer condition alone misses . For example satisfies that condition, but the integral is zero and the displayed factorial is undefined.
Explicit coefficients. Both Taylor series in
converge absolutely and uniformly on every compact annulus away from zero, so their product can be regrouped. For , put and . For arbitrary integer , use the already proved symmetry:
Here is a modified Bessel function. The printed series is directly meaningful for ; for negative the absolute values, or an appropriately shifted lower summation limit, are essential.