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mathematics Mathematics is a field of study that discovers and organizes methods, Mathematical theory, theories and theorems that are developed and Mathematical proof, proved for the needs of empirical sciences and mathematics itself. There are many ar ...
, a Sobolev space is a
vector space In mathematics and physics, a vector space (also called a linear space) is a set (mathematics), set whose elements, often called vector (mathematics and physics), ''vectors'', can be added together and multiplied ("scaled") by numbers called sc ...
of functions equipped with a norm that is a combination of ''Lp''-norms of the function together with its derivatives up to a given order. The derivatives are understood in a suitable weak sense to make the space complete, i.e. a
Banach space In mathematics, more specifically in functional analysis, a Banach space (, ) is a complete normed vector space. Thus, a Banach space is a vector space with a metric that allows the computation of vector length and distance between vectors and ...
. Intuitively, a Sobolev space is a space of functions possessing sufficiently many derivatives for some application domain, such as
partial differential equation In mathematics, a partial differential equation (PDE) is an equation which involves a multivariable function and one or more of its partial derivatives. The function is often thought of as an "unknown" that solves the equation, similar to ho ...
s, and equipped with a norm that measures both the size and regularity of a function. Sobolev spaces are named after the Russian
mathematician A mathematician is someone who uses an extensive knowledge of mathematics in their work, typically to solve mathematical problems. Mathematicians are concerned with numbers, data, quantity, mathematical structure, structure, space, Mathematica ...
Sergei Sobolev. Their importance comes from the fact that weak solutions of some important partial differential equations exist in appropriate Sobolev spaces, even when there are no strong solutions in spaces of
continuous function In mathematics, a continuous function is a function such that a small variation of the argument induces a small variation of the value of the function. This implies there are no abrupt changes in value, known as '' discontinuities''. More preci ...
s with the
derivative In mathematics, the derivative is a fundamental tool that quantifies the sensitivity to change of a function's output with respect to its input. The derivative of a function of a single variable at a chosen input value, when it exists, is t ...
s understood in the classical sense.


Motivation

In this section and throughout the article \Omega is an
open subset In mathematics, an open set is a generalization of an open interval in the real line. In a metric space (a set with a distance defined between every two points), an open set is a set that, with every point in it, contains all points of the met ...
of \R^n. There are many criteria for smoothness of
mathematical function In mathematics, a function from a set (mathematics), set to a set assigns to each element of exactly one element of .; the words ''map'', ''mapping'', ''transformation'', ''correspondence'', and ''operator'' are sometimes used synonymously. ...
s. The most basic criterion may be that of continuity. A stronger notion of smoothness is that of differentiability (because functions that are differentiable are also continuous) and a yet stronger notion of smoothness is that the derivative also be continuous (these functions are said to be of class C^1 — see Differentiability classes). Differentiable functions are important in many areas, and in particular for differential equations. In the twentieth century, however, it was observed that the space C^1 (or C^2, etc.) was not exactly the right space to study solutions of differential equations. The Sobolev spaces are the modern replacement for these spaces in which to look for solutions of partial differential equations. Quantities or properties of the underlying model of the differential equation are usually expressed in terms of integral norms. A typical example is measuring the energy of a temperature or velocity distribution by an L^2-norm. It is therefore important to develop a tool for differentiating Lebesgue space functions. The
integration by parts In calculus, and more generally in mathematical analysis, integration by parts or partial integration is a process that finds the integral of a product of functions in terms of the integral of the product of their derivative and antiderivati ...
formula yields that for every u\in C^k(\Omega), where k is a
natural number In mathematics, the natural numbers are the numbers 0, 1, 2, 3, and so on, possibly excluding 0. Some start counting with 0, defining the natural numbers as the non-negative integers , while others start with 1, defining them as the positive in ...
, and for all infinitely differentiable functions with
compact support In mathematics, the support of a real-valued function f is the subset of the function domain of elements that are not mapped to zero. If the domain of f is a topological space, then the support of f is instead defined as the smallest closed ...
\varphi \in C_c^(\Omega), : \int_\Omega u\,D^\varphi\,dx=(-1)^\int_\Omega \varphi\, D^ u\,dx, where \alpha is a multi-index of order , \alpha, =k and we are using the notation: :D^f = \frac. The left-hand side of this equation still makes sense if we only assume u to be locally integrable. If there exists a locally integrable function v, such that : \int_\Omega u\,D^\varphi\;dx=(-1)^\int_\Omega \varphi \,v \;dx \qquad\text\varphi\in C_c^\infty(\Omega), then we call v the weak \alpha-th partial derivative of u. If there exists a weak \alpha-th partial derivative of u, then it is uniquely defined
almost everywhere In measure theory (a branch of mathematical analysis), a property holds almost everywhere if, in a technical sense, the set for which the property holds takes up nearly all possibilities. The notion of "almost everywhere" is a companion notion to ...
, and thus it is uniquely determined as an element of a Lebesgue space. On the other hand, if u\in C^k(\Omega), then the classical and the weak derivative coincide. Thus, if v is a weak \alpha-th partial derivative of u, we may denote it by D^\alpha u := v. For example, the function :u(x)=\begin 1+x & -1 is not continuous at zero, and not differentiable at −1, 0, or 1. Yet the function :v(x)=\begin 1 & -1 satisfies the definition for being the weak derivative of u(x), which then qualifies as being in the Sobolev space W^ (for any allowed p, see definition below). The Sobolev spaces W^(\Omega) combine the concepts of weak differentiability and Lebesgue norms.


Sobolev spaces with integer ''k''


One-dimensional case

In the one-dimensional case the Sobolev space W^(\R) for 1 \le p \le \infty is defined as the subset of functions f in L^p(\R) such that f and its
weak derivative In mathematics, a weak derivative is a generalization of the concept of the derivative of a function (''strong derivative'') for functions not assumed differentiable, but only integrable, i.e., to lie in the L''p'' space L^1( ,b. The method o ...
s up to order k have a finite norm. As mentioned above, some care must be taken to define derivatives in the proper sense. In the one-dimensional problem it is enough to assume that the (k1)-th derivative f^ is differentiable almost everywhere and is equal almost everywhere to the
Lebesgue integral In mathematics, the integral of a non-negative Function (mathematics), function of a single variable can be regarded, in the simplest case, as the area between the Graph of a function, graph of that function and the axis. The Lebesgue integral, ...
of its derivative (this excludes irrelevant examples such as Cantor's function). With this definition, the Sobolev spaces admit a natural norm, :\, f\, _ = \left (\sum_^k \left \, f^ \right \, _p^p \right)^ = \left (\sum_^k \int \left , f^(t) \right , ^p\,dt \right )^. One can extend this to the case p = \infty , with the norm then defined using the
essential supremum In mathematics, the concepts of essential infimum and essential supremum are related to the notions of infimum and supremum, but adapted to measure theory and functional analysis, where one often deals with statements that are not valid for ''all' ...
by :\, f\, _ = \max_ \left \, f^ \right \, _\infty = \max_ \left(\text\, \sup_t \left , f^(t) \right , \right). Equipped with the norm \, \cdot\, _, W^ becomes a
Banach space In mathematics, more specifically in functional analysis, a Banach space (, ) is a complete normed vector space. Thus, a Banach space is a vector space with a metric that allows the computation of vector length and distance between vectors and ...
. It turns out that it is enough to take only the first and last in the sequence, i.e., the norm defined by :\left \, f^ \right \, _p + \, f\, _p is equivalent to the norm above (i.e. the induced topologies of the norms are the same).


The case

Sobolev spaces with are especially important because of their connection with
Fourier series A Fourier series () is an Series expansion, expansion of a periodic function into a sum of trigonometric functions. The Fourier series is an example of a trigonometric series. By expressing a function as a sum of sines and cosines, many problems ...
and because they form a
Hilbert space In mathematics, a Hilbert space is a real number, real or complex number, complex inner product space that is also a complete metric space with respect to the metric induced by the inner product. It generalizes the notion of Euclidean space. The ...
. A special notation has arisen to cover this case, since the space is a Hilbert space: :H^k = W^. The space H^k can be defined naturally in terms of
Fourier series A Fourier series () is an Series expansion, expansion of a periodic function into a sum of trigonometric functions. The Fourier series is an example of a trigonometric series. By expressing a function as a sum of sines and cosines, many problems ...
whose coefficients decay sufficiently rapidly, namely, :H^k(\mathbb) = \Big \, where \widehat is the Fourier series of f, and \mathbb denotes the 1-torus. As above, one can use the equivalent norm :\, f\, ^2_=\sum_^\infty \left (1 + , n, ^ \right )^k \left , \widehat(n) \right , ^2. Both representations follow easily from Parseval's theorem and the fact that differentiation is equivalent to multiplying the Fourier coefficient by in. Furthermore, the space H^k admits an
inner product In mathematics, an inner product space (or, rarely, a Hausdorff pre-Hilbert space) is a real vector space or a complex vector space with an operation called an inner product. The inner product of two vectors in the space is a scalar, ofte ...
, like the space H^0 = L^2. In fact, the H^k inner product is defined in terms of the L^2 inner product: :\langle u,v\rangle_ = \sum_^k \left \langle D^i u,D^i v \right \rangle_. The space H^k becomes a Hilbert space with this inner product.


Other examples

In one dimension, some other Sobolev spaces permit a simpler description. For example, W^(0,1) is the space of absolutely continuous functions on (or rather, equivalence classes of functions that are equal almost everywhere to such), while W^(I) is the space of bounded Lipschitz functions on , for every interval . However, these properties are lost or not as simple for functions of more than one variable. All spaces W^ are (normed)
algebra Algebra is a branch of mathematics that deals with abstract systems, known as algebraic structures, and the manipulation of expressions within those systems. It is a generalization of arithmetic that introduces variables and algebraic ope ...
s, i.e. the product of two elements is once again a function of this Sobolev space, which is not the case for p<\infty. (E.g., functions behaving like , ''x'', −1/3 at the origin are in L^2, but the product of two such functions is not in L^2).


Multidimensional case

The transition to multiple dimensions brings more difficulties, starting from the very definition. The requirement that f^ be the integral of f^ does not generalize, and the simplest solution is to consider derivatives in the sense of distribution theory. A formal definition now follows. Let k \in \N, 1 \leqslant p \leqslant \infty. The Sobolev space W^(\Omega) is defined to be the set of all functions f on \Omega such that for every multi-index \alpha with , \alpha, \leqslant k, the mixed
partial derivative In mathematics, a partial derivative of a function of several variables is its derivative with respect to one of those variables, with the others held constant (as opposed to the total derivative, in which all variables are allowed to vary). P ...
:f^ = \frac exists in the weak sense and is in L^p(\Omega), i.e. :\left \, f^ \right \, _ < \infty. That is, the Sobolev space W^(\Omega) is defined as :W^(\Omega) = \left \. The
natural number In mathematics, the natural numbers are the numbers 0, 1, 2, 3, and so on, possibly excluding 0. Some start counting with 0, defining the natural numbers as the non-negative integers , while others start with 1, defining them as the positive in ...
k is called the order of the Sobolev space W^(\Omega). There are several choices for a norm for W^(\Omega). The following two are common and are equivalent in the sense of equivalence of norms: :\, u \, _ := \begin \left( \sum_ \left \, D^u \right \, _^p \right)^ & 1 \leqslant p < \infty; \\ \max_ \left \, D^u \right \, _ & p = \infty; \end and :\, u \, '_ := \begin \sum_ \left \, D^u \right \, _ & 1 \leqslant p < \infty; \\ \sum_ \left \, D^u \right \, _ & p = \infty. \end With respect to either of these norms, W^(\Omega) is a Banach space. For p<\infty, W^(\Omega) is also a
separable space In mathematics, a topological space is called separable if it contains a countable, dense subset; that is, there exists a sequence ( x_n )_^ of elements of the space such that every nonempty open subset of the space contains at least one elemen ...
. It is conventional to denote W^(\Omega) by H^k(\Omega) for it is a
Hilbert space In mathematics, a Hilbert space is a real number, real or complex number, complex inner product space that is also a complete metric space with respect to the metric induced by the inner product. It generalizes the notion of Euclidean space. The ...
with the norm \, \cdot \, _.


Approximation by smooth functions

It is rather hard to work with Sobolev spaces relying only on their definition. It is therefore interesting to know that by the Meyers–Serrin theorem a function u \in W^(\Omega) can be approximated by smooth functions. This fact often allows us to translate properties of smooth functions to Sobolev functions. If p is finite and \Omega is open, then there exists for any u \in W^(\Omega) an approximating sequence of functions u_m \in C^(\Omega) such that: : \left \, u_m - u \right \, _ \to 0. If \Omega has Lipschitz boundary, we may even assume that the u_m are the restriction of smooth functions with compact support on all of \R^n.


Examples

In higher dimensions, it is no longer true that, for example, W^ contains only continuous functions. For example, , x, ^ \in W^(\mathbb^3) where \mathbb^3 is the
unit ball Unit may refer to: General measurement * Unit of measurement, a definite magnitude of a physical quantity, defined and adopted by convention or by law **International System of Units (SI), modern form of the metric system **English units, histo ...
in three dimensions. For k > n/p, the space W^(\Omega) will contain only continuous functions, but for which k this is already true depends both on p and on the dimension. For example, as can be easily checked using
spherical polar coordinates In mathematics, a spherical coordinate system specifies a given point in three-dimensional space by using a distance and two angles as its three coordinates. These are * the radial distance along the line connecting the point to a fixed point ...
for the function f : \mathbb^n \to \R \cup \ defined on the ''n''-dimensional unit ball we have: :f(x) = , x , ^ \in W^(\mathbb^n) \Longleftrightarrow \alpha < \tfrac - k. Intuitively, the blow-up of ''f'' at 0 "counts for less" when ''n'' is large since the unit ball has "more outside and less inside" in higher dimensions.


Absolutely continuous on lines (ACL) characterization of Sobolev functions

Let 1\leqslant p \leqslant \infty. If a function is in W^(\Omega), then, possibly after modifying the function on a set of measure zero, the restriction to almost every line parallel to the coordinate directions in \R^n is
absolutely continuous In calculus and real analysis, absolute continuity is a smoothness property of functions that is stronger than continuity and uniform continuity. The notion of absolute continuity allows one to obtain generalizations of the relationship betwe ...
; what's more, the classical derivative along the lines that are parallel to the coordinate directions are in L^p(\Omega). Conversely, if the restriction of f to almost every line parallel to the coordinate directions is absolutely continuous, then the pointwise gradient \nabla f exists
almost everywhere In measure theory (a branch of mathematical analysis), a property holds almost everywhere if, in a technical sense, the set for which the property holds takes up nearly all possibilities. The notion of "almost everywhere" is a companion notion to ...
, and f is in W^(\Omega) provided f, , \nabla f, \in L^p(\Omega). In particular, in this case the weak partial derivatives of f and pointwise partial derivatives of f agree almost everywhere. The ACL characterization of the Sobolev spaces was established by Otto M. Nikodym (
1933 Events January * January 11 – Australian aviator Sir Charles Kingsford Smith makes the first commercial flight between Australia and New Zealand. * January 17 – The United States Congress votes in favour of Philippines independen ...
); see . A stronger result holds when p>n. A function in W^(\Omega) is, after modifying on a set of measure zero,
Hölder continuous Hölder: * ''Hölder, Hoelder'' as surname * Hölder condition * Hölder's inequality In mathematical analysis, Hölder's inequality, named after Otto Hölder, is a fundamental inequality (mathematics), inequality between Lebesgue integration, in ...
of exponent \gamma = 1 - \tfrac, by Morrey's inequality. In particular, if p=\infty and \Omega has Lipschitz boundary, then the function is
Lipschitz continuous In mathematical analysis, Lipschitz continuity, named after Germany, German mathematician Rudolf Lipschitz, is a strong form of uniform continuity for function (mathematics), functions. Intuitively, a Lipschitz continuous function is limited in h ...
.


Functions vanishing at the boundary

The Sobolev space W^(\Omega) is also denoted by H^1\!(\Omega). It is a Hilbert space, with an important subspace H^1_0\!(\Omega) defined to be the closure of the infinitely differentiable functions compactly supported in \Omega in H^1\!(\Omega). The Sobolev norm defined above reduces here to :\, f\, _ = \left ( \int_\Omega \! , f, ^2 \!+\! , \nabla\! f, ^2 \right)^. When \Omega has a regular boundary, H^1_0\!(\Omega) can be described as the space of functions in H^1\!(\Omega) that vanish at the boundary, in the sense of traces ( see below). When n=1, if \Omega = (a,b) is a bounded interval, then H^1_0(a,b) consists of continuous functions on ,b/math> of the form :f(x) = \int_a^x f'(t) \, \mathrmt, \qquad x \in , b/math> where the generalized derivative f' is in L^2(a,b) and has 0 integral, so that f(b) = f(a) = 0. When \Omega is bounded, the Poincaré inequality states that there is a constant C= C(\Omega) such that: :\int_\Omega , f, ^2 \leqslant C^2 \int_\Omega , \nabla f, ^2, \qquad f \in H^1_0(\Omega). When \Omega is bounded, the injection from H^1_0\!(\Omega) to L^2\!(\Omega), is
compact Compact as used in politics may refer broadly to a pact or treaty; in more specific cases it may refer to: * Interstate compact, a type of agreement used by U.S. states * Blood compact, an ancient ritual of the Philippines * Compact government, a t ...
. This fact plays a role in the study of the Dirichlet problem, and in the fact that there exists an
orthonormal basis In mathematics, particularly linear algebra, an orthonormal basis for an inner product space V with finite Dimension (linear algebra), dimension is a Basis (linear algebra), basis for V whose vectors are orthonormal, that is, they are all unit vec ...
of L^2(\Omega) consisting of eigenvectors of the
Laplace operator In mathematics, the Laplace operator or Laplacian is a differential operator given by the divergence of the gradient of a Scalar field, scalar function on Euclidean space. It is usually denoted by the symbols \nabla\cdot\nabla, \nabla^2 (where \ ...
(with Dirichlet boundary condition).


Traces

Sobolev spaces are often considered when investigating partial differential equations. It is essential to consider boundary values of Sobolev functions. If u\in C(\Omega), those boundary values are described by the restriction u, _. However, it is not clear how to describe values at the boundary for u\in W^(\Omega), as the ''n''-dimensional measure of the boundary is zero. The following theorem resolves the problem: ''Tu'' is called the trace of ''u''. Roughly speaking, this theorem extends the restriction operator to the Sobolev space W^(\Omega) for well-behaved Ω. Note that the trace operator ''T'' is in general not surjective, but for 1 < ''p'' < ∞ it maps continuously onto the Sobolev–Slobodeckij space W^(\partial\Omega). Intuitively, taking the trace costs 1/''p'' of a derivative. The functions ''u'' in ''W''1,p(Ω) with zero trace, i.e. ''Tu'' = 0, can be characterized by the equality : W_0^(\Omega)= \left \, where : W_0^(\Omega):= \left \. In other words, for Ω bounded with Lipschitz boundary, trace-zero functions in W^(\Omega) can be approximated by smooth functions with compact support.


Sobolev spaces with non-integer ''k''


Bessel potential spaces

For a natural number ''k'' and one can show (by using Fourier multipliers) that the space W^(\R^n) can equivalently be defined as : W^(\R^n) = H^(\R^n) := \Big \, with the norm :\, f\, _ := \left\, \mathcal^ \Big \xi, ^2\big)^ \mathcalf \Big\right\, _. This motivates Sobolev spaces with non-integer order since in the above definition we can replace ''k'' by any real number ''s''. The resulting spaces :H^(\R^n) := \left \ are called Bessel potential spaces (named after
Friedrich Bessel Friedrich Wilhelm Bessel (; 22 July 1784 – 17 March 1846) was a German astronomer, mathematician, physicist, and geodesy, geodesist. He was the first astronomer who determined reliable values for the distance from the Sun to another star by th ...
). They are Banach spaces in general and Hilbert spaces in the special case ''p'' = 2. For s \geq 0, H^(\Omega) is the set of restrictions of functions from H^(\R^n) to Ω equipped with the norm :\, f\, _ := \inf \left \ . Again, ''Hs,p''(Ω) is a Banach space and in the case ''p'' = 2 a Hilbert space. Using extension theorems for Sobolev spaces, it can be shown that also ''Wk,p''(Ω) = ''Hk,p''(Ω) holds in the sense of equivalent norms, if Ω is domain with uniform ''Ck''-boundary, ''k'' a natural number and . By the
embedding In mathematics, an embedding (or imbedding) is one instance of some mathematical structure contained within another instance, such as a group (mathematics), group that is a subgroup. When some object X is said to be embedded in another object Y ...
s : H^(\R^n) \hookrightarrow H^(\R^n) \hookrightarrow H^(\R^n) \hookrightarrow H^(\R^n), \quad k \leqslant s \leqslant s' \leqslant k+1 the Bessel potential spaces H^(\R^n) form a continuous scale between the Sobolev spaces W^(\R^n). From an abstract point of view, the Bessel potential spaces occur as complex
interpolation space In the mathematics, mathematical field of numerical analysis, interpolation is a type of estimation, a method of constructing (finding) new data points based on the range of a discrete set of known data points. In engineering and science, one ...
s of Sobolev spaces, i.e. in the sense of equivalent norms it holds that : \left W^(\R^n), W^(\R^n) \right \theta = H^(\R^n), where: :1 \leqslant p \leqslant \infty, \ 0 < \theta < 1, \ s= (1-\theta)k + \theta (k+1)= k+\theta.


Sobolev–Slobodeckij spaces

Another approach to define fractional order Sobolev spaces arises from the idea to generalize the
Hölder condition In mathematics, a real or complex-valued function on -dimensional Euclidean space satisfies a Hölder condition, or is Hölder continuous, when there are real constants , , such that , f(x) - f(y) , \leq C\, x - y\, ^ for all and in the do ...
to the ''Lp''-setting. For 1 \leqslant p < \infty, \theta \in (0, 1) and f \in L^p(\Omega), the Slobodeckij seminorm (roughly analogous to the Hölder seminorm) is defined by : :=\left(\int_ \int_ \frac \; dx \; dy \right )^. Let be not an integer and set \theta = s - \lfloor s \rfloor \in (0,1). Using the same idea as for the Hölder spaces, the Sobolev–Slobodeckij space W^(\Omega) is defined as :W^(\Omega) := \left\. It is a Banach space for the norm :\, f \, _ := \, f\, _ + \sup_ ^\alpha f. If \Omega is suitably regular in the sense that there exist certain extension operators, then also the Sobolev–Slobodeckij spaces form a scale of Banach spaces, i.e. one has the continuous injections or
embedding In mathematics, an embedding (or imbedding) is one instance of some mathematical structure contained within another instance, such as a group (mathematics), group that is a subgroup. When some object X is said to be embedded in another object Y ...
s : W^(\Omega) \hookrightarrow W^(\Omega) \hookrightarrow W^(\Omega) \hookrightarrow W^(\Omega), \quad k \leqslant s \leqslant s' \leqslant k+1. There are examples of irregular Ω such that W^(\Omega) is not even a vector subspace of W^(\Omega) for 0 < ''s'' < 1 (see Example 9.1 of ) From an abstract point of view, the spaces W^(\Omega) coincide with the real
interpolation space In the mathematics, mathematical field of numerical analysis, interpolation is a type of estimation, a method of constructing (finding) new data points based on the range of a discrete set of known data points. In engineering and science, one ...
s of Sobolev spaces, i.e. in the sense of equivalent norms the following holds: : W^(\Omega) = \left (W^(\Omega), W^(\Omega) \right)_ , \quad k \in \N, s \in (k, k+1), \theta = s - \lfloor s \rfloor . Sobolev–Slobodeckij spaces play an important role in the study of traces of Sobolev functions. They are special cases of Besov spaces. The constant arising in the characterization of the fractional Sobolev space W^(\Omega) can be characterized through the Bourgain-Brezis-Mironescu formula: : \lim_ \; (1 - s) \int_ \int_ \frac \; dx \; dy = \frac \int_ \vert \nabla f\vert^p; and the condition : \limsup_\; (1 - s) \int_ \int_ \frac \; dx \; dy < \infty characterizes those functions of L^p (\Omega) that are in the first-order Sobolev space W^ (\Omega).


Extension operators

If \Omega is a domain whose boundary is not too poorly behaved (e.g., if its boundary is a manifold, or satisfies the more permissive " cone condition") then there is an operator ''A'' mapping functions of \Omega to functions of \R^n such that: # ''Au''(''x'') = ''u''(''x'') for almost every ''x'' in \Omega and # A : W^(\Omega) \to W^(\R^n) is continuous for any 1 ≤ ''p'' ≤ ∞ and integer ''k''. We will call such an operator ''A'' an extension operator for \Omega.


Case of ''p'' = 2

Extension operators are the most natural way to define H^s(\Omega) for non-integer ''s'' (we cannot work directly on \Omega since taking Fourier transform is a global operation). We define H^s(\Omega) by saying that u \in H^s(\Omega) if and only if Au \in H^s(\R^n). Equivalently, complex interpolation yields the same H^s(\Omega) spaces so long as \Omega has an extension operator. If \Omega does not have an extension operator, complex interpolation is the only way to obtain the H^s(\Omega) spaces. As a result, the interpolation inequality still holds.


Extension by zero

Like above, we define H^s_0(\Omega) to be the closure in H^s(\Omega) of the space C^\infty_c(\Omega) of infinitely differentiable compactly supported functions. Given the definition of a trace, above, we may state the following If u\in H^s_0(\Omega) we may define its extension by zero \tilde u \in L^2(\R^n) in the natural way, namely :\tilde u(x)= \begin u(x) & x \in \Omega \\ 0 & \text \end For its extension by zero, :Ef := \begin f & \textrm \ \Omega, \\ 0 & \textrm \end is an element of L^p(\R^n). Furthermore, : \, Ef \, _= \, f \, _. In the case of the Sobolev space ''W''1,p(Ω) for , extending a function ''u'' by zero will not necessarily yield an element of W^(\R^n). But if Ω is bounded with Lipschitz boundary (e.g. ∂Ω is ''C''1), then for any bounded open set O such that Ω⊂⊂O (i.e. Ω is compactly contained in O), there exists a bounded linear operator : E: W^(\Omega)\to W^(\R^n), such that for each u\in W^(\Omega): Eu = u a.e. on Ω, ''Eu'' has compact support within O, and there exists a constant ''C'' depending only on ''p'', Ω, O and the dimension ''n'', such that :\, Eu \, _\leqslant C \, u\, _. We call Eu an extension of u to \R^n.


Sobolev embeddings

It is a natural question to ask if a Sobolev function is continuous or even continuously differentiable. Roughly speaking, sufficiently many weak derivatives (i.e. large ''k'') result in a classical derivative. This idea is generalized and made precise in the Sobolev embedding theorem. Write W^ for the Sobolev space of some compact
Riemannian manifold In differential geometry, a Riemannian manifold is a geometric space on which many geometric notions such as distance, angles, length, volume, and curvature are defined. Euclidean space, the N-sphere, n-sphere, hyperbolic space, and smooth surf ...
of dimension ''n''. Here ''k'' can be any real number, and 1 ≤ ''p'' ≤ ∞. (For ''p'' = ∞ the Sobolev space W^ is defined to be the Hölder space ''C''''n'',α where ''k'' = ''n'' + α and 0 < α ≤ 1.) The Sobolev embedding theorem states that if k \geqslant m and k - \tfrac \geqslant m - \tfrac then :W^\subseteq W^ and the embedding is continuous. Moreover, if k > m and k - \tfrac > m - \tfrac then the embedding is completely continuous (this is sometimes called Kondrachov's theorem or the Rellich–Kondrachov theorem). Functions in W^ have all derivatives of order less than ''m'' continuous, so in particular this gives conditions on Sobolev spaces for various derivatives to be continuous. Informally these embeddings say that to convert an ''Lp'' estimate to a boundedness estimate costs 1/''p'' derivatives per dimension. There are similar variations of the embedding theorem for non-compact manifolds such as \R^n . Sobolev embeddings on \R^n that are not compact often have a related, but weaker, property of cocompactness.


See also

* Sobolev mapping * Souček space * Besov space * Triebel–Lizorkin space


Notes


References

* . * . * * * * *. *. *. *. *. *. *; translation of Mat. Sb., 4 (1938) pp. 471–497. *. *. *. *.


External links


Eleonora Di Nezza, Giampiero Palatucci, Enrico Valdinoci (2011). "Hitchhiker's guide to the fractional Sobolev spaces".
{{DEFAULTSORT:Sobolev Space Fourier analysis Fractional calculus Function spaces