A function f ( z ) {\displaystyle f(z)} defined on the complex plane is said to be of exponential type if there exist real-valued constants M {\displaystyle M} and τ {\displaystyle \tau } such that
in the limit of r → ∞ {\displaystyle r\to \infty } . Here, the complex variable z {\displaystyle z} was written as z = r e i θ {\displaystyle z=re^{i\theta }} to emphasize that the limit must hold in all directions θ {\displaystyle \theta } . Letting τ {\displaystyle \tau } stand for the infimum of all such τ {\displaystyle \tau } , one then says that the function f {\displaystyle f} is of exponential type τ {\displaystyle \tau } .
For example, let f ( z ) = sin ( π z ) {\displaystyle f(z)=\sin(\pi z)} . Then one says that sin ( π z ) {\displaystyle \sin(\pi z)} is of exponential type π {\displaystyle \pi } , since π {\displaystyle \pi } is the smallest number that bounds the growth of sin ( π z ) {\displaystyle \sin(\pi z)} along the imaginary axis. So, for this example, Carlson's theorem cannot apply, as it requires functions of exponential type less than π {\displaystyle \pi } . Similarly, the Euler–Maclaurin formula cannot be applied either, as it, too, expresses a theorem ultimately anchored in the theory of finite differences.
A holomorphic function F ( z ) {\displaystyle F(z)} is said to be of exponential type σ > 0 {\displaystyle \sigma >0} if for every ε > 0 {\displaystyle \varepsilon >0} there exists a real-valued constant A ε {\displaystyle A_{\varepsilon }} such that
for | z | → ∞ {\displaystyle |z|\to \infty } where z ∈ C {\displaystyle z\in \mathbb {C} } . We say F ( z ) {\displaystyle F(z)} is of exponential type if F ( z ) {\displaystyle F(z)} is of exponential type σ {\displaystyle \sigma } for some σ > 0 {\displaystyle \sigma >0} . The number
is the exponential type of F ( z ) {\displaystyle F(z)} . The limit superior here means the limit of the supremum of the ratio outside a given radius as the radius goes to infinity. This is also the limit superior of the maximum of the ratio at a given radius as the radius goes to infinity. The limit superior may exist even if the maximum at radius r {\displaystyle r} does not have a limit as r {\displaystyle r} goes to infinity. For example, for the function
the value of
at r = 10 n ! − 1 {\displaystyle r=10^{n!-1}} is dominated by the n − 1 st {\displaystyle n-1^{\text{st}}} term so we have the asymptotic expressions:
and this goes to zero as n {\displaystyle n} goes to infinity,1 but F ( z ) {\displaystyle F(z)} is nevertheless of exponential type 1, as can be seen by looking at the points z = 10 n ! {\displaystyle z=10^{n!}} .
Stein (1957) has given a generalization of exponential type for entire functions of several complex variables. Suppose K {\displaystyle K} is a convex, compact, and symmetric subset of R n {\displaystyle \mathbb {R} ^{n}} . It is known that for every such K {\displaystyle K} there is an associated norm ‖ ⋅ ‖ K {\displaystyle \|\cdot \|_{K}} with the property that
In other words, K {\displaystyle K} is the unit ball in R n {\displaystyle \mathbb {R} ^{n}} with respect to ‖ ⋅ ‖ K {\displaystyle \|\cdot \|_{K}} . The set
is called the polar set and is also a convex, compact, and symmetric subset of R n {\displaystyle \mathbb {R} ^{n}} . Furthermore, we can write
We extend ‖ ⋅ ‖ K {\displaystyle \|\cdot \|_{K}} from R n {\displaystyle \mathbb {R} ^{n}} to C n {\displaystyle \mathbb {C} ^{n}} by
An entire function F ( z ) {\displaystyle F(z)} of n {\displaystyle n} -complex variables is said to be of exponential type with respect to K {\displaystyle K} if for every ε > 0 {\displaystyle \varepsilon >0} there exists a real-valued constant A ε {\displaystyle A_{\varepsilon }} such that
for all z ∈ C n {\displaystyle z\in \mathbb {C} ^{n}} .
Collections of functions of exponential type τ {\displaystyle \tau } can form a complete uniform space, namely a Fréchet space, by the topology induced by the countable family of norms
In fact, even ( max | z | = r log log | F ( z ) | ) / ( log r ) {\displaystyle (\max _{|z|=r}\log \log |F(z)|)/(\log r)} goes to zero at r = 10 n ! − 1 {\displaystyle r=10^{n!-1}} as n {\displaystyle n} goes to infinity. ↩