# Hölder condition

# Hölder condition

In mathematics, a real or complex-valued function *f* on *d*-dimensional Euclidean space satisfies a **Hölder condition**, or is **Hölder continuous**, when there are nonnegative real constants *C*, α>0, such that

for all *x* and *y* in the domain of *f*. More generally, the condition can be formulated for functions between any two metric spaces. The number α is called the *exponent* of the Hölder condition. A function on an interval satisfying the condition with α > 1 is constant. If α = 1, then the function satisfies a Lipschitz condition. For any α > 0, the condition implies the function is uniformly continuous. The condition is named after Otto Hölder.

We have the following chain of strict inclusions for functions over a **closed and bounded non-trivial interval** of the real line

- **Continuously differentiable** ⊂ **Lipschitz continuous** ⊂

**α-Hölder continuous**⊂ **uniformly continuous** = **continuous**

where 0 < α ≤ 1.

Hölder spaces

Hölder spaces consisting of functions satisfying a Hölder condition are basic in areas of functional analysis relevant to solving partial differential equations, and in dynamical systems. The Hölder space *C**k*,α(Ω), where Ω is an open subset of some Euclidean space and *k* ≥ 0 an integer, consists of those functions on Ω having continuous derivatives up to order *k* and such that the *k*th partial derivatives are Hölder continuous with exponent α, where 0 < α ≤ 1. This is a locally convex topological vector space. If the Hölder coefficient

is finite, then the function *f* is said to be *(uniformly) Hölder continuous with exponent α in Ω.* In this case, the Hölder coefficient serves as a seminorm. If the Hölder coefficient is merely bounded on compact subsets of Ω, then the function *f* is said to be *locally Hölder continuous with exponent α in Ω.*

`If the function`

*f*and its derivatives up to order*k*are bounded on the closure of Ω, then the Hölder spacecan be assigned the normwhere β ranges over multi-indices and

`These seminorms and norms are often denoted simplyandor alsoandin order to stress the dependence on the domain of`

*f*. If Ω is open and bounded, thenis aBanach spacewith respect to the norm.Compact embedding of Hölder spaces

Let Ω be a bounded subset of some Euclidean space (or more generally, any totally bounded metric space) and let 0 < α < β ≤ 1 two Hölder exponents. Then, there is an obvious inclusion map of the corresponding Hölder spaces:

which is continuous since, by definition of the Hölder norms, we have:

Moreover, this inclusion is compact, meaning that bounded sets in the ‖ · ‖0,β norm are relatively compact in the ‖ · ‖0,α norm. This is a direct consequence of the Ascoli-Arzelà theorem. Indeed, let (*un*) be a bounded sequence in *C*0,β(Ω). Thanks to the Ascoli-Arzelà theorem we can assume without loss of generality that *un* → *u* uniformly, and we can also assume *u* = 0. Then

because

Examples

If 0 < α ≤ β ≤ 1 then all Hölder continuous functions on a

*bounded set*Ω are also Hölder continuous. This also includes β = 1 and therefore all Lipschitz continuous functions on a bounded set are also*C*0,α Hölder continuous.

The function

*f*(*x*) =*x*β (with β ≤ 1) defined on [0, 1] serves as a prototypical example of a function that is*C*0,α Hölder continuous for 0 < α ≤ β, but not for α > β. Further, if we defined*f*analogously on , it would be*C*0,α Hölder continuous only for α = β.

For α > 1, any α–Hölder continuous function on [0, 1] (or any interval) is a constant.

There are examples of uniformly continuous functions that are not α–Hölder continuous for any α. For instance, the function defined on [0, 1/2] by

*f*(0) = 0 and by*f*(*x*) = 1/log(*x*) otherwise is continuous, and therefore uniformly continuous by the Heine-Cantor theorem. It does not satisfy a Hölder condition of any order, however.

The Weierstrass function defined by:

^{[1]}

The Cantor function is Hölder continuous for any exponent and for no larger one. In the former case, the inequality of the definition holds with the constant

*C*:= 2.

Peano curves from [0, 1] onto the square [0, 1]2 can be constructed to be 1/2–Hölder continuous. It can be proved that when the image of a α–Hölder continuous function from the unit interval to the square cannot fill the square.

Sample paths of Brownian motion are almost surely everywhere locally α-Hölder for every

Functions which are locally integrable and whose integrals satisfy an appropriate growth condition are also Hölder continuous. For example, if we let

*u*satisfies

*u*is Hölder continuous with exponent α.

^{[2]}

Functions whose

*oscillation*decay at a fixed rate with respect to distance are Hölder continuous with an exponent that is determined by the rate of decay. For instance, if

*u*(

*x*) satisfies

*r*, then

*u*is Hölder continuous.

Functions in Sobolev space can be embedded into the appropriate Hölder space via Morrey's inequality if the spatial dimension is less than the exponent of the Sobolev space. To be precise, if then there exists a constant

*C*, depending only on*p*and*n*, such that:

*u*∈

*W*

^{1, p}(

**R**

^{n}), then

*u*is in fact Hölder continuous of exponent γ, after possibly being redefined on a set of measure 0.

Properties

A closed additive subgroup of an infinite dimensional Hilbert space

*H*, connected by α–Hölder continuous arcs with α > 1/2, is a linear subspace. There are closed additive subgroups of*H*, not linear subspaces, connected by 1/2–Hölder continuous arcs. An example is the additive subgroup*L*2(**R**,**Z**) of the Hilbert space*L*2(**R**,**R**).

Any α–Hölder continuous function

*f*on a metric space*X*admits a Lipschitz approximation by means of a sequence of functions (*fk*) such that*fk*is*k*-Lipschitz and

_{k}*) of Lipschitz functions converges to an α–Hölder continuous uniform limit

*f*.

Any α–Hölder function

*f*on a subset*X*of a normed space*E*admits a uniformly continuous extension to the whole space, which is Hölder continuous with the same constant*C*and the same exponent α. The largest such extension is:

The image of any α–Hölder function has Hausdorff dimension at most

The space is not separable.

The embedding is not dense.