Hölder condition

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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. If α = 1, then the function satisfies a Lipschitz condition. If α = 0, then the function simply is bounded. The condition is named after Otto Hölder.

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 Ck(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 norms and seminorms 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 of the corresponding Hölder spaces:

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

which is continuous since, by definition of the Hölder norms, the inequality

|f|_{{0,\alpha ,\Omega }}\leq {\mathrm  {diam}}(\Omega )^{{\beta -\alpha }}|f|_{{0,\beta ,\Omega }}

holds for all f in C0,β(Ω). 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 C0,β(Ω). Thanks to the Ascoli-Arzelà theorem we can assume without loss of generality that unu uniformly, and we can also assume u = 0. Then

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

because of

{\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 }}}}|u_{n}(x)-u_{n}(y)|^{{1-{\frac  {\alpha }{\beta }}}}

we have:

|u_{n}(x)-u_{n}(y)|^{{1-{\frac  {\alpha }{\beta }}}}\leq \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 C0,α Hölder continuous.
  • The function f(x)={\sqrt  {x}} defined on [0, 1] is not Lipschitz continuous, but is C0,α Hölder continuous for α ≤ 1/2.
  • In the same manner, the function f(x) = xβ (with β ≤ 1) defined on [0, 1] serves as a prototypical example of a function that is C0,α Hölder continuous for 0 < α ≤ β, but not for α > β.
  • There are examples of uniformly continuous functions that are not αHölder 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.
  • For α > 1, any αHölder continuous function on [0, 1] is a constant.
  • The Cantor function is Hölder continuous for any exponent α ≤ 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 1/2Hölder continuous. It can be proved that when α > 1/2, the image of a αHölder continuous function from the unit interval to the square cannot fill the square.
  • A closed additive subgroup of an infinite dimensional Hilbert space H, connected by αHölder continuous arcs with α > 1/2, is a linear subspace. There are closed additive subgroups of H, not linear subspaces, connected by 1/2Hölder continuous arcs. An example is the additive subgroup L2(R, Z) of the Hilbert space L2(R, R).
  • Any αHölder 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
\|f-f_{k}\|_{{\infty ,X}}=O\left(k^{{-{\frac  {\alpha }{1-\alpha }}}}\right).
Conversely, any such sequence (fk) of Lipschitz functions converges to an αHölder continuous uniform limit f.
  • Any αHölder 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 larger such extension is:
f^{*}(x):=\inf _{{y\in X}}\left\{f(y)+C|x-y|^{\alpha }\right\}.
  • 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 ≤ ∞ then there exists a constant C, depending only on p and n, such that
\|u\|_{{C^{{0,\gamma }}({\mathbf  {R}}^{n})}}\leq C\|u\|_{{W^{{1,p}}({\mathbf  {R}}^{n})}}
for all uC1(Rn) ∩ Lp(Rn), where γ = 1 − (n/p). Thus if uW1, p(Rn), then u is in fact Hölder continuous of exponent γ, after possibly being redefined on a set of measure 0.
  • 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)}}|u(y)-u_{{x,r}}|^{2}dy\leq Cr^{{n+2\alpha }},
then u is Hölder continuous with exponent α.[1]
  • 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(u,x_{0},{\tfrac  {r}{2}})\leq \lambda w(u,x_{0},r)
for a fixed λ with 0 < λ < 1 and all sufficiently small values of r, then u is Hölder continuous.

Notes

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

References

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