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In [[mathematics]], '''Bochner spaces''' are a generalization of the concept of [[Lp space|''L<sup>p</sup>'' spaces]] to functions whose values lie in a [[Banach space]] which is not necessarily the space R or C of real or complex numbers. | |||
The space ''L<sup>p</sup>(X)'' consists of (equivalence classes of) all [[Bochner measurable]] functions ''f'' with values in the Banach space ''X'' whose [[norm (mathematics)|norm]] ''||f||<sub>X</sub>'' lies in the standard ''L<sup>p</sup>'' space. Thus, if ''X'' is the set of complex numbers, it is the standard Lebesgue ''L<sup>p</sup>'' space. | |||
Almost all standard results on ''L<sup>p</sup>'' spaces do hold on Bochner spaces too; in particular, the Bochner spaces ''L<sup>p</sup>(X)'' are Banach spaces for <math>1\le p\le \infty</math>. | |||
==Background== | |||
Bochner spaces are named for the [[Poland|Polish]]-[[United States|American]] [[mathematician]] [[Salomon Bochner]]. | |||
==Applications== | |||
Bochner spaces are often used in the [[functional analysis]] approach to the study of [[partial differential equation]]s that depend on time, e.g. the [[heat equation]]: if the temperature <math>g(t,x)</math> is a scalar function of time and space, one can write <math>(f(t))(x):=g(t,x)</math> to make ''f'' a family ''f(t)'' (parametrized by time) of functions of space, possibly in some Bochner space. | |||
==Definition== | |||
Given a [[measure space]] (''T'', Σ, ''μ''), a [[Banach space]] (''X'', || · ||<sub>''X''</sub>) and 1 ≤ ''p'' ≤ +∞, the '''Bochner space''' ''L''<sup>''p''</sup>(''T''; ''X'') is defined to be the [[Kolmogorov quotient]] (by equality [[almost everywhere]]) of the space of all [[Bochner measurable]] functions ''u'' : ''T'' → ''X'' such that the corresponding norm is finite: | |||
:<math>\| u \|_{L^{p} (T; X)} := \left( \int_{T} \| u(t) \|_{X}^{p} \, \mathrm{d} \mu (t) \right)^{1/p} < + \infty \mbox{ for } 1 \leq p < \infty,</math> | |||
:<math>\| u \|_{L^{\infty} (T; X)} := \mathrm{ess\,sup}_{t \in T} \| u(t) \|_{X} < + \infty.</math> | |||
In other words, as is usual in the study of ''L''<sup>''p''</sup> spaces, ''L''<sup>''p''</sup>(''T''; ''X'') is a space of [[equivalence class]]es of functions, where two functions are defined to be equivalent if they are equal everywhere except upon a ''μ''-[[measure zero]] subset of ''T''. As is also usual in the study of such spaces, it is usual to [[abuse of notation|abuse notation]] and speak of a "function" in ''L''<sup>''p''</sup>(''T''; ''X'') rather than an equivalence class (which would be more technically correct). | |||
==Application to PDE theory== | |||
Very often, the space ''T'' is an [[Interval (mathematics)|interval]] of time over which we wish to solve some partial differential equation, and ''μ'' will be one-dimensional [[Lebesgue measure]]. The idea is to regard a function of time and space as a collection of functions of space, this collection being parametrized by time. For example, in the solution of the heat equation on a region Ω in '''R'''<sup>''n''</sup> and an interval of time [0, ''T''], one seeks solutions | |||
:<math>u \in L^{2} \left( [0, T]; H_{0}^{1} (\Omega) \right)</math> | |||
with time derivative | |||
:<math>\frac{\partial u}{\partial t} \in L^{2} \left( [0, T]; H^{- 1} (\Omega) \right).</math> | |||
Here <math>H_{0}^{1} (\Omega)</math> denotes the [[Sobolev space|Sobolev]] [[Hilbert space]] of once-[[weak derivative|weakly differentiable]] functions with first weak derivative in ''L''²(Ω) that vanish at the [[boundary (topology)|boundary]] of Ω (in the sense of trace, or, equivalently, are limits of smooth functions with [[compact space|compact]] [[support (mathematics)|support]] in Ω); <math>H^{-1} (\Omega)</math> denotes the [[dual space]] of <math>H_{0}^{1} (\Omega)</math>. | |||
(The "[[partial derivative]]" with respect to time ''t'' above is actually a [[total derivative]], since the use of Bochner spaces removes the space-dependence.) | |||
==References== | |||
* {{cite book | last=Evans | first=Lawrence C. | title=Partial differential equations | location=Providence, RI | publisher=American Mathematical Society | year=1998 | isbn=0-8218-0772-2}} | |||
==See also== | |||
*[[Vector-valued functions]] | |||
{{Functional Analysis}} | |||
[[Category:Functional analysis]] | |||
[[Category:Partial differential equations]] | |||
[[Category:Sobolev spaces]] |
Latest revision as of 22:17, 1 February 2014
In mathematics, Bochner spaces are a generalization of the concept of Lp spaces to functions whose values lie in a Banach space which is not necessarily the space R or C of real or complex numbers.
The space Lp(X) consists of (equivalence classes of) all Bochner measurable functions f with values in the Banach space X whose norm ||f||X lies in the standard Lp space. Thus, if X is the set of complex numbers, it is the standard Lebesgue Lp space.
Almost all standard results on Lp spaces do hold on Bochner spaces too; in particular, the Bochner spaces Lp(X) are Banach spaces for .
Background
Bochner spaces are named for the Polish-American mathematician Salomon Bochner.
Applications
Bochner spaces are often used in the functional analysis approach to the study of partial differential equations that depend on time, e.g. the heat equation: if the temperature is a scalar function of time and space, one can write to make f a family f(t) (parametrized by time) of functions of space, possibly in some Bochner space.
Definition
Given a measure space (T, Σ, μ), a Banach space (X, || · ||X) and 1 ≤ p ≤ +∞, the Bochner space Lp(T; X) is defined to be the Kolmogorov quotient (by equality almost everywhere) of the space of all Bochner measurable functions u : T → X such that the corresponding norm is finite:
In other words, as is usual in the study of Lp spaces, Lp(T; X) is a space of equivalence classes of functions, where two functions are defined to be equivalent if they are equal everywhere except upon a μ-measure zero subset of T. As is also usual in the study of such spaces, it is usual to abuse notation and speak of a "function" in Lp(T; X) rather than an equivalence class (which would be more technically correct).
Application to PDE theory
Very often, the space T is an interval of time over which we wish to solve some partial differential equation, and μ will be one-dimensional Lebesgue measure. The idea is to regard a function of time and space as a collection of functions of space, this collection being parametrized by time. For example, in the solution of the heat equation on a region Ω in Rn and an interval of time [0, T], one seeks solutions
with time derivative
Here denotes the Sobolev Hilbert space of once-weakly differentiable functions with first weak derivative in L²(Ω) that vanish at the boundary of Ω (in the sense of trace, or, equivalently, are limits of smooth functions with compact support in Ω); denotes the dual space of .
(The "partial derivative" with respect to time t above is actually a total derivative, since the use of Bochner spaces removes the space-dependence.)
References
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