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, such that

|f(x)-f(y)|\leq C\|x-y\|^{\alpha }

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 satisfying the condition with α > 1 is constant. If α = 1, then the function satisfies a Lipschitz condition. If α > 0, the condition implies the function is continuous. If α = 0, the function need not be continuous, but it is bounded. The condition is named after Otto Hölder.

We have the following chain of inclusions for functions over a compact subset 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 kth partial derivatives are Hölder continuous with exponent α, where 0 < α ≤ 1. This is a locally convex topological vector space. If the Hölder coefficient

|f|_{C^{0,\alpha }}=\sup _{x\neq y\in \Omega }{\frac {|f(x)-f(y)|}{|x-y|^{\alpha }}},

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 space $C^{k,\alpha }({\overline {\Omega }})$ can be assigned the norm

\|f\|_{C^{k,\alpha }}=\|f\|_{C^{k}}+\max _{|\beta |=k}\left|D^{\beta }f\right|_{C^{0,\alpha }}

where β ranges over multi-indices and

\|f\|_{C^{k}}=\max _{|\beta |\leq k}\sup _{x\in \Omega }\left|D^{\beta }f(x)\right|.

These seminorms and norms are often denoted simply $|f|_{0,\alpha }$ and $\|f\|_{k,\alpha }$ or also $|f|_{0,\alpha ,\Omega }\;$ and $\|f\|_{k,\alpha ,\Omega }$ in order to stress the dependence on the domain of f. If Ω is open and bounded, then $C^{k,\alpha }({\overline {\Omega }})$ is a Banach space with respect to the norm $\|\cdot \|_{C^{k,\alpha }}$ .

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:

C^{0,\beta }(\Omega )\to C^{0,\alpha }(\Omega ),

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

\forall f\in C^{0,\beta }(\Omega ):\qquad |f|_{0,\alpha ,\Omega }\leq \mathrm {diam} (\Omega )^{\beta -\alpha }|f|_{0,\beta ,\Omega }.

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 (u_n) be a bounded sequence in C^0,β(Ω). Thanks to the Ascoli-Arzelà theorem we can assume without loss of generality that u_n → u uniformly, and we can also assume u = 0. Then

|u_{n}-u|_{0,\alpha }=|u_{n}|_{0,\alpha }\to 0,

because

{\frac {|u_{n}(x)-u_{n}(y)|}{|x-y|^{\alpha }}}=\left({\frac {|u_{n}(x)-u_{n}(y)|}{|x-y|^{\beta }}}\right)^{\frac {\alpha }{\beta }}\left|u_{n}(x)-u_{n}(y)\right|^{1-{\frac {\alpha }{\beta }}}\leq |u_{n}|_{0,\beta }^{\frac {\alpha }{\beta }}\left(2\|u_{n}\|_{\infty }\right)^{1-{\frac {\alpha }{\beta }}}=o(1).

Examples

If 0 < α ≤ β ≤ 1 then all $C^{0,\beta }({\overline {\Omega }})$ Hölder continuous functions on a bounded set Ω are also $C^{0,\alpha }({\overline {\Omega }})$ 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 $[0,\infty )$ , 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:

f(x)=\sum _{n=0}^{\infty }a^{n}\cos \left(b^{n}\pi x\right),

where

0<a<1,b

is an integer,

b\geq 2

and

ab>1+{\tfrac {3\pi }{2}},

is α-Hölder continuous with

\alpha =-{\frac {\log(a)}{\log(b)}}.

^[1]

The Cantor function is Hölder continuous for any exponent $\alpha \leq {\tfrac {\log 2}{\log 3}},$ 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 $\alpha >{\tfrac {1}{2}}$ 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 $\alpha <{\tfrac {1}{2}}.$

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

u_{x,r}={\frac {1}{|B_{r}|}}\int _{B_{r}(x)}u(y)dy

and u satisfies

\int _{B_{r}(x)}\left|u(y)-u_{x,r}\right|^{2}dy\leq Cr^{n+2\alpha },

then 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

w(u,x_{0},r)=\sup _{B_{r}(x_{0})}u-\inf _{B_{r}(x_{0})}u

for some function u(x) satisfies

w\left(u,x_{0},{\tfrac {r}{2}}\right)\leq \lambda w\left(u,x_{0},r\right)

for a fixed λ with 0 < λ < 1 and all sufficiently small values of 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 $n<p\leq \infty$ then there exists a constant C, depending only on p and n, such that:

\forall u\in C^{1}(\mathbf {R} ^{n})\cap L^{p}(\mathbf {R} ^{n}):\qquad \|u\|_{C^{0,\gamma }(\mathbf {R} ^{n})}\leq C\|u\|_{W^{1,p}(\mathbf {R} ^{n})},

where

\gamma =1-{\tfrac {n}{p}}.

Thus if u ∈ W^{1, p}(Rⁿ), 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 L²(R, Z) of the Hilbert space L²(R, R).

Any α–Hölder continuous function f on a metric space X admits a Lipschitz approximation by means of a sequence of functions (f_k) such that f_k is k-Lipschitz and

\|f-f_{k}\|_{\infty ,X}=O\left(k^{-{\frac {\alpha }{1-\alpha }}}\right).

Conversely, any such sequence (f_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:

f^{*}(x):=\inf _{y\in X}\left\{f(y)+C|x-y|^{\alpha }\right\}.

The image of any α–Hölder function has Hausdorff dimension at most ${\tfrac {1}{\alpha }}.$

The space $C^{0,\alpha }(\Omega ),0<\alpha \leq 1$ is not separable.

The embedding $C^{0,\beta }(\Omega )\subset C^{0,\alpha }(\Omega ),0<\alpha <\beta \leq 1$ is not dense.

Notes

↑ Hardy, G. H. “Weierstrass's Non-Differentiable Function.” Transactions of the American Mathematical Society, vol. 17, no. 3, 1916, pp. 301–325. JSTOR, JSTOR, www.jstor.org/stable/1989005.
↑ See, for example, Han and Lin, Chapter 3, Section 1. This result was originally due to Sergio Campanato.

References

Lawrence C. Evans (1998). Partial Differential Equations. American Mathematical Society, Providence. ISBN 0-8218-0772-2.
Gilbarg, D.; Trudinger, Neil (1983). Elliptic Partial Differential Equations of Second Order. New York: Springer. ISBN 3-540-41160-7. .
Han, Qing; Lin, Fanghua (1997). Elliptic Partial Differential Equations. New York: Courant Institute of Mathematical Sciences. ISBN 0-9658703-0-8. OCLC 38168365 MR 1669352

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[1] Hardy, G. H. “Weierstrass's Non-Differentiable Function.” Transactions of the American Mathematical Society, vol. 17, no. 3, 1916, pp. 301–325. JSTOR, JSTOR, www.jstor.org/stable/1989005.

[2] See, for example, Han and Lin, Chapter 3, Section 1. This result was originally due to Sergio Campanato.