Bounded variation

In mathematical analysis, a function of bounded variation, also known as a BV function, is a real-valued function whose total variation is bounded (finite): the graph of a function having this property is well behaved in a precise sense. For a continuous function of a single variable, being of bounded variation means that the distance along the direction of the y-axis, neglecting the contribution of motion along x-axis, traveled by a point moving along the graph has a finite value. For a continuous function of several variables, the meaning of the definition is the same, except for the fact that the continuous path to be considered cannot be the whole graph of the given function (which is a hypersurface in this case), but can be every intersection of the graph itself with a hyperplane (in the case of functions of two variables, a plane) parallel to a fixed x-axis and to the y-axis.

Functions of bounded variation are precisely those with respect to which one may find Riemann–Stieltjes integrals of all continuous functions.

Another characterization states that the functions of bounded variation on a compact interval are exactly those f which can be written as a difference g  h, where both g and h are bounded monotone.

In the case of several variables, a function f defined on an open subset Ω of ℝn is said to have bounded variation if its distributional derivative is a vector-valued finite Radon measure.

One of the most important aspects of functions of bounded variation is that they form an algebra of discontinuous functions whose first derivative exists almost everywhere: due to this fact, they can and frequently are used to define generalized solutions of nonlinear problems involving functionals, ordinary and partial differential equations in mathematics, physics and engineering. Considering the problem of multiplication of distributions or more generally the problem of defining general nonlinear operations on generalized functions, functions of bounded variation are the smallest algebra which has to be embedded in every space of generalized functions preserving the result of multiplication.

History

According to Boris Golubov, BV functions of a single variable were first introduced by Camille Jordan, in the paper (Jordan 1881) dealing with the convergence of Fourier series. The first successful step in the generalization of this concept to functions of several variables was due to Leonida Tonelli,[1] who introduced a class of continuous BV functions in 1926 (Cesari 1986, pp. 47–48), to extend his direct method for finding solutions to problems in the calculus of variations in more than one variable. Ten years after, in (Cesari 1936), Lamberto Cesari changed the continuity requirement in Tonelli's definition to a less restrictive integrability requirement, obtaining for the first time the class of functions of bounded variation of several variables in its full generality: as Jordan did before him, he applied the concept to resolve of a problem concerning the convergence of Fourier series, but for functions of two variables. After him, several authors applied BV functions to study Fourier series in several variables, geometric measure theory, calculus of variations, and mathematical physics. Renato Caccioppoli and Ennio de Giorgi used them to define measure of nonsmooth boundaries of sets (see the entry "Caccioppoli set" for further information). Olga Arsenievna Oleinik introduced her view of generalized solutions for nonlinear partial differential equations as functions from the space BV in the paper (Oleinik 1957), and was able to construct a generalized solution of bounded variation of a first order partial differential equation in the paper (Oleinik 1959): few years later, Edward D. Conway and Joel A. Smoller applied BV-functions to the study of a single nonlinear hyperbolic partial differential equation of first order in the paper (Conway & Smoller 1966), proving that the solution of the Cauchy problem for such equations is a function of bounded variation, provided the initial value belongs to the same class. Aizik Isaakovich Vol'pert developed extensively a calculus for BV functions: in the paper (Vol'pert 1967) he proved the chain rule for BV functions and in the book (Hudjaev & Vol'pert 1985) he, jointly with his pupil Sergei Ivanovich Hudjaev, explored extensively the properties of BV functions and their application. His chain rule formula was later extended by Luigi Ambrosio and Gianni Dal Maso in the paper (Ambrosio & Dal Maso 1990).

Formal definition

BV functions of one variable

Definition 1.1. The total variation[2] of a real-valued (or more generally complex-valued) function f, defined on an interval [a, b]⊂ℝ is the quantity

 V_a^b(f)=\sup_{P \in \mathcal{P}} \sum_{i=0}^{n_{P}-1} | f(x_{i+1})-f(x_i) |. \,

where the supremum is taken over the set  \scriptstyle \mathcal{P} =\left\{P=\{ x_0, \dots , x_{n_P}\}|P\text{ is a partition of } [a, b] \right\} of all partitions of the interval considered.

If f is differentiable and its derivative is Riemann-integrable, its total variation is the vertical component of the arc-length of its graph, that is to say,

 V_a^b(f) = \int _a^b |f'(x)|\,\mathrm{d}x.

Definition 1.2. A real-valued function  f on the real line is said to be of bounded variation (BV function) on a chosen interval [a, b]⊂ℝ if its total variation is finite, i.e.

 f \in BV([a,b]) \iff V_a^b(f) < +\infty

It can be proved that a real function ƒ is of bounded variation in [a,b] if and only if it can be written as the difference ƒ = ƒ1ƒ2 of two non-decreasing functions on [a,b]: this result is known as the Jordan decomposition of a function and it is related to the Jordan decomposition of a measure.

Through the Stieltjes integral, any function of bounded variation on a closed interval [a, b] defines a bounded linear functional on C([a, b]). In this special case,[3] the Riesz representation theorem states that every bounded linear functional arises uniquely in this way. The normalised positive functionals or probability measures correspond to positive non-decreasing lower semicontinuous functions. This point of view has been important in spectral theory,[4] in particular in its application to ordinary differential equations.

BV functions of several variables

Functions of bounded variation, BV functions, are functions whose distributional derivative is a finite[5] Radon measure. More precisely:

Definition 2.1. Let  \Omega be an open subset of ℝn. A function  u belonging to L^1(\Omega) is said of bounded variation (BV function), and written

 u\in BV(\Omega)

if there exists a finite vector Radon measure  \scriptstyle Du\in\mathcal M(\Omega,\mathbb{R}^n) such that the following equality holds


\int_\Omega u(x)\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x = - \int_\Omega \langle\boldsymbol{\phi}, Du(x)\rangle
\qquad \forall\boldsymbol{\phi}\in C_c^1(\Omega,\mathbb{R}^n)

that is, u defines a linear functional on the space  \scriptstyle C_c^1(\Omega,\mathbb{R}^n) of continuously differentiable vector functions  \scriptstyle\boldsymbol{\phi} of compact support contained in  \Omega : the vector measure Du represents therefore the distributional or weak gradient of u.

An equivalent definition is the following.

Definition 2.2. Given a function u belonging to L^1(\Omega), the total variation of u[2] in \Omega is defined as

 V(u,\Omega):=\sup\left\{\int_\Omega u(x)\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x\colon\boldsymbol{\phi}\in C_c^1(\Omega,\mathbb{R}^n),\ \Vert\boldsymbol{\phi}\Vert_{L^\infty(\Omega)}\le 1\right\}

where  \scriptstyle \Vert\;\Vert_{L^\infty(\Omega)} is the essential supremum norm. Sometimes, especially in the theory of Caccioppoli sets, the following notation is used

\int_\Omega\vert D u\vert = V(u,\Omega)

in order to emphasize that V(u,\Omega) is the total variation of the distributional / weak gradient of u. This notation reminds also that if u is of class C^1 (i.e. a continuous and differentiable function having continuous derivatives) then its variation is exactly the integral of the absolute value of its gradient.

The space of functions of bounded variation (BV functions) can then be defined as

 BV(\Omega)=\{ u\in L^1(\Omega)\colon V(u,\Omega)<+\infty\}

The two definitions are equivalent since if  \scriptstyle V(u,\Omega)<+\infty then

\left|\int_\Omega u(x)\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x \right |\leq V(u,\Omega)\Vert\boldsymbol{\phi}\Vert_{L^\infty(\Omega)}
\qquad \forall \boldsymbol{\phi}\in C_c^1(\Omega,\mathbb{R}^n)

therefore \scriptstyle \boldsymbol{\phi}\mapsto\,\int_\Omega u(x)\,\mathrm{div}\boldsymbol{\phi}(x)dx defines a continuous linear functional on the space \scriptstyle C_c^1(\Omega,\mathbb{R}^n). Since \scriptstyle C_c^1(\Omega,\mathbb{R}^n)
\subset C^0(\Omega,\mathbb{R}^n) as a linear subspace, this continuous linear functional can be extended continuously and linearily to the whole \scriptstyle C^0(\Omega,\mathbb{R}^n) by the Hahn–Banach theorem. Hence the continuous linear functional defines a Radon measure by the Riesz-Markov Theorem.

Locally BV functions

If the function space of locally integrable functions, i.e. functions belonging to \scriptstyle L^1_{loc}(\Omega), is considered in the preceding definitions 1.2, 2.1 and 2.2 instead of the one of globally integrable functions, then the function space defined is that of functions of locally bounded variation. Precisely, developing this idea for definition 2.2, a local variation is defined as follows,

 V(u,U):=\sup\left\{\int_\Omega u(x)\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x\colon\boldsymbol{\phi}\in C_c^1(U,\mathbb{R}^n),\ \Vert\boldsymbol{\phi}\Vert_{L^\infty(\Omega)}\le 1\right\}

for every set \scriptstyle U\in\mathcal{O}_c(\Omega), having defined \scriptstyle \mathcal{O}_c(\Omega) as the set of all precompact open subsets of \Omega with respect to the standard topology of finite-dimensional vector spaces, and correspondingly the class of functions of locally bounded variation is defined as

BV_{loc}(\Omega)=\{ u\in L^1_{loc}(\Omega)\colon V(u,U)<+\infty\; \forall U\in\mathcal{O}_c(\Omega)\}

Notation

There are basically two distinct conventions for the notation of spaces of functions of locally or globally bounded variation, and unfortunately they are quite similar: the first one, which is the one adopted in this entry, is used for example in references Giusti (1984) (partially), Hudjaev & Vol'pert (1985) (partially), Giaquinta, Modica & Souček (1998) and is the following one

The second one, which is adopted in references Vol'pert (1967) and Maz'ya (1985) (partially), is the following:

Basic properties

Only the properties common to functions of one variable and to functions of several variables will be considered in the following, and proofs will be carried on only for functions of several variables since the proof for the case of one variable is a straightforward adaptation of the several variables case: also, in each section it will be stated if the property is shared also by functions of locally bounded variation or not. References (Giusti 1984, pp. 7–9), (Hudjaev & Vol'pert 1985) and (Màlek et al. 1996) are extensively used.

BV functions have only jump-type or removable discontinuities

In the case of one variable, the assertion is clear: for each point x_0 in the interval [a , b]⊂ℝ of definition of the function u, either one of the following two assertions is true

 \lim_{x\rightarrow x_{0^-}}\!\!\!u(x) = \!\!\!\lim_{x\rightarrow x_{0^+}}\!\!\!u(x)
 \lim_{x\rightarrow x_{0^-}}\!\!\!u(x) \neq \!\!\!\lim_{x\rightarrow x_{0^+}}\!\!\!u(x)

while both limits exist and are finite. In the case of functions of several variables, there are some premises to understand: first of all, there is a continuum of directions along which it is possible to approach a given point x_0 belonging to the domain \Omega⊂ℝn. It is necessary to make precise a suitable concept of limit: choosing a unit vector \scriptstyle{\boldsymbol{\hat{a}}}\in\mathbb{R}^n it is possible to divide \Omega in two sets

\Omega_{({\boldsymbol{\hat{a}}},\boldsymbol{x}_0)} = \Omega \cap \{\boldsymbol{x}\in\mathbb{R}^n|\langle\boldsymbol{x}-\boldsymbol{x}_0,{\boldsymbol{\hat{a}}}\rangle>0\} \qquad
\Omega_{(-{\boldsymbol{\hat{a}}},\boldsymbol{x}_0)} = \Omega \cap \{\boldsymbol{x}\in\mathbb{R}^n|\langle\boldsymbol{x}-\boldsymbol{x}_0,-{\boldsymbol{\hat{a}}}\rangle>0\}

Then for each point x_0 belonging to the domain \scriptstyle\Omega\in\mathbb{R}^n of the BV function u, only one of the following two assertions is true

 \lim_{\overset{\boldsymbol{x}\rightarrow \boldsymbol{x}_0}{\boldsymbol{x}\in\Omega_{({\boldsymbol{\hat{a}}},\boldsymbol{x}_0)}}}\!\!\!\!\!\!u(\boldsymbol{x}) = \!\!\!\!\!\!\!\lim_{\overset{\boldsymbol{x}\rightarrow \boldsymbol{x}_0}{\boldsymbol{x}\in\Omega_{(-{\boldsymbol{\hat{a}}},\boldsymbol{x}_0)}}}\!\!\!\!\!\!\!u(\boldsymbol{x})
  \lim_{\overset{\boldsymbol{x}\rightarrow \boldsymbol{x}_0}{\boldsymbol{x}\in\Omega_{({\boldsymbol{\hat{a}}},\boldsymbol{x}_0)}}}\!\!\!\!\!\!u(\boldsymbol{x}) \neq \!\!\!\!\!\!\!\lim_{\overset{\boldsymbol{x}\rightarrow \boldsymbol{x}_0}{\boldsymbol{x}\in\Omega_{(-{\boldsymbol{\hat{a}}},\boldsymbol{x}_0)}}}\!\!\!\!\!\!\!u(\boldsymbol{x})

or x_0 belongs to a subset of \Omega having zero n-1-dimensional Hausdorff measure. The quantities

\lim_{\overset{\boldsymbol{x}\rightarrow \boldsymbol{x}_0}{\boldsymbol{x}\in\Omega_{({\boldsymbol{\hat{a}}},\boldsymbol{x}_0)}}}\!\!\!\!\!\!u(\boldsymbol{x})=u_{\boldsymbol{\hat a}}(\boldsymbol{x}_0) \qquad \lim_{\overset{\boldsymbol{x}\rightarrow \boldsymbol{x}_0}{\boldsymbol{x}\in\Omega_{(-{\boldsymbol{\hat{a}}},\boldsymbol{x}_0)}}}\!\!\!\!\!\!\!u(\boldsymbol{x})=u_{-\boldsymbol{\hat a}}(\boldsymbol{x}_0)

are called approximate limits of the BV function u at the point x_0.

V(·, Ω) is lower semi-continuous on BV(Ω)

The functional \scriptstyle V(\cdot,\Omega):BV(\Omega)\rightarrow \mathbb{R}^+ is lower semi-continuous: to see this, choose a Cauchy sequence of BV-functions \scriptstyle\{u_n\}_{n\in\mathbb{N}} converging to \scriptstyle u\in L^1_\text{loc}(\Omega). Then, since all the functions of the sequence and their limit function are integrable and by the definition of lower limit

\liminf_{n\rightarrow\infty}V(u_n,\Omega) \geq \liminf_{n\rightarrow\infty} \int_\Omega u_n(x)\,\mathrm{div}\, \boldsymbol{\phi}\, \mathrm{d}x \geq \int_\Omega \lim_{n\rightarrow\infty} u_n(x)\,\mathrm{div}\, \boldsymbol{\phi}\, \mathrm{d}x = \int_\Omega u(x)\,\mathrm{div}\boldsymbol{\phi}\, \mathrm{d}x \qquad\forall\boldsymbol{\phi}\in C_c^1(\Omega,\mathbb{R}^n),\quad\Vert\boldsymbol{\phi}\Vert_{L^\infty(\Omega)}\leq 1

Now considering the supremum on the set of functions \scriptstyle\boldsymbol{\phi}\in C_c^1(\Omega,\mathbb{R}^n) such that \scriptstyle \Vert\boldsymbol{\phi}\Vert_{L^\infty(\Omega)}\leq 1 then the following inequality holds true

\liminf_{n\rightarrow\infty}V(u_n,\Omega)\geq V(u,\Omega)

which is exactly the definition of lower semicontinuity.

BV(Ω) is a Banach space

By definition BV(\Omega) is a subset of L^1(\Omega), while linearity follows from the linearity properties of the defining integral i.e.

\begin{align}
\int_\Omega [u(x)+v(x)]\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x & =
\int_\Omega u(x)\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x +\int_\Omega v(x)\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x = \\
& =- \int_\Omega \langle\boldsymbol{\phi}(x), Du(x)\rangle- \int_\Omega \langle \boldsymbol{\phi}(x), Dv(x)\rangle
                                               =- \int_\Omega \langle \boldsymbol{\phi}(x), [Du(x)+Dv(x)]\rangle
\end{align}

for all \scriptstyle\phi\in C_c^1(\Omega,\mathbb{R}^n) therefore \scriptstyle u+v\in BV(\Omega)for all \scriptstyle u,v\in BV(\Omega), and


\int_\Omega c\cdot u(x)\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x =
c\!\int_\Omega u(x)\,\mathrm{div}\boldsymbol{\phi}(x)\mathrm{d}x =
-c\! \int_\Omega \langle \boldsymbol{\phi}(x), Du(x)\rangle

for all \scriptstyle c\in\mathbb{R}, therefore \scriptstyle cu\in BV(\Omega) for all \scriptstyle u\in BV(\Omega), and all \scriptstyle c\in\mathbb{R}. The proved vector space properties imply that BV(\Omega) is a vector subspace of L^1(\Omega). Consider now the function \scriptstyle\|\;\|_{BV}:BV(\Omega)\rightarrow\mathbb{R}^+ defined as

\| u \|_{BV} := \| u \|_{L^1} + V(u,\Omega)

where \scriptstyle\| \; \|_{L^1} is the usual L^1(\Omega) norm: it is easy to prove that this is a norm on BV(\Omega). To see that BV(\Omega) is complete respect to it, i.e. it is a Banach space, consider a Cauchy sequence \scriptstyle\{u_n\}_{n\in\mathbb{N}} in BV(\Omega). By definition it is also a Cauchy sequence in L^1(\Omega) and therefore has a limit u in L^1(\Omega): since u_n is bounded in BV(\Omega) for each n, then \scriptstyle \Vert u \Vert_{BV} < +\infty by lower semicontinuity of the variation \scriptstyle V(\cdot,\Omega), therefore u is a BV function. Finally, again by lower semicontinuity, choosing an arbitrary small positive number \scriptstyle\varepsilon

\Vert u_j - u_k \Vert_{BV}<\varepsilon\quad\forall j,k\geq N\in\mathbb{N} \quad\Rightarrow\quad V(u_k-u,\Omega)\leq \liminf_{j\rightarrow +\infty} V(u_k-u_j,\Omega)\leq\varepsilon

BV(Ω) is not separable

To see this, it is sufficient to consider the following example belonging to the space BV([0,1]):[6] for each 0<α<1 define

\chi_\alpha=\chi_{[\alpha,1]}=
\begin{cases} 0 & \mbox{if } x \notin\; [\alpha,1] \\ 
              1 & \mbox{if } x \in [\alpha,1]
\end{cases}

as the characteristic function of the left-closed interval [\alpha,1]. Then, choosing α,β[0,1] such that αβ the following relation holds true:

\Vert \chi_\alpha - \chi_\beta \Vert_{BV}=2+|\alpha-\beta|

Now, in order to prove that every dense subset of BV(]0,1[) cannot be countable, it is sufficient to see that for every α[0,1] it is possible to construct the balls

B_\alpha=\left\{\psi\in BV([0,1]);\Vert \chi_\alpha - \psi \Vert_{BV}\leq 1\right\}

Obviously those balls are pairwise disjoint, and also are an indexed family of sets whose index set is [0,1]. This implies that this family has the cardinality of the continuum: now, since any dense subset of BV([0,1]) must have at least a point inside each member of this family, its cardinality is at least that of the continuum and therefore cannot a be countable subset.[7] This example can be obviously extended to higher dimensions, and since it involves only local properties, it implies that the same property is true also for BV_{loc}.

Chain rule for BV functions

Chain rules for nonsmooth functions are very important in mathematics and mathematical physics since there are several important physical models whose behavior is described by functions or functionals with a very limited degree of smoothness.The following version is proved in the paper (Vol'pert 1967, p. 248): all partial derivatives must be intended in a generalized sense. i.e. as generalized derivatives

Theorem. Let \scriptstyle f:\mathbb{R}^p\rightarrow\mathbb{R} be a function of class C^1 (i.e. a continuous and differentiable function having continuous derivatives) and let \scriptstyle\boldsymbol{u}(\boldsymbol{x})=(u_1(\boldsymbol{x}),\ldots,u_p(\boldsymbol{x})) be a function in BV(\Omega) with  \Omega being an open subset of  \scriptstyle\mathbb{R}^n . Then \scriptstyle f\circ\boldsymbol{u}(\boldsymbol{x})=f(\boldsymbol{u}(\boldsymbol{x}))\in BV(\Omega) and

\frac{\partial f(\boldsymbol{u}(\boldsymbol{x}))}{\partial x_i}=\sum_{k=1}^p\frac{\partial\bar{f}(\boldsymbol{u}(\boldsymbol{x}))}{\partial u_k}\frac{\partial{u_k(\boldsymbol{x})}}{\partial x_i}
\qquad\forall i=1,\ldots,n

where \scriptstyle\bar f(\boldsymbol{u}(\boldsymbol{x})) is the mean value of the function at the point \scriptstyle x \in\Omega, defined as

\bar f(\boldsymbol{u}(\boldsymbol{x}))=\int_0^1 f\left(\boldsymbol{u}_{\boldsymbol{\hat a}}(\boldsymbol{x})t + \boldsymbol{u}_{-\boldsymbol{\hat a}}(\boldsymbol{x})(1-t)\right)dt

A more general chain rule formula for Lipschitz continuous functions \scriptstyle f:\mathbb{R}^p\rightarrow\mathbb{R}^s has been found by Luigi Ambrosio and Gianni Dal Maso and is published in the paper (Ambrosio & Dal Maso 1990). However, even this formula has very important direct consequences: choosing \scriptstyle f(u)=v(\boldsymbol{x})u(\boldsymbol{x}), where \scriptstyle v(\boldsymbol{x}) is also a BV function, the preceding formula gives the Leibniz rule for BV functions

\frac{\partial v(\boldsymbol{x})u(\boldsymbol{x})}{\partial x_i} = {\bar u(\boldsymbol{x})}\frac{\partial v(\boldsymbol{x})}{\partial x_i} +
{\bar v(\boldsymbol{x})}\frac{\partial u(\boldsymbol{x})}{\partial x_i}

This implies that the product of two functions of bounded variation is again a function of bounded variation, therefore BV(\Omega) is an algebra.

BV(Ω) is a Banach algebra

This property follows directly from the fact that BV(\Omega) is a Banach space and also an associative algebra: this implies that if \{v_n\} and \{u_n\} are Cauchy sequences of BV functions converging respectively to functions v and u in BV(\Omega), then

\begin{matrix}
  vu_n\xrightarrow[n\to\infty]{} vu \\
  v_nu\xrightarrow[n\to\infty]{} vu
        \end{matrix}\quad\Longleftrightarrow
\quad vu\in BV(\Omega)

therefore the ordinary product of functions is continuous in BV(\Omega) respect to each argument, making this function space a Banach algebra.

Generalizations and extensions

Weighted BV functions

It is possible to generalize the above notion of total variation so that different variations are weighted differently. More precisely, let \scriptstyle \varphi : [0, +\infty)\longrightarrow [0, +\infty) be any increasing function such that \scriptstyle \varphi(0) = \varphi(0+) =\lim_{x\rightarrow 0_+}\varphi(x) = 0 (the weight function) and let \scriptstyle f: [0, T]\longrightarrow X be a function from the interval [0 , T]⊂ℝ taking values in a normed vector space X. Then the \scriptstyle \boldsymbol\varphi-variation of f over [0, T] is defined as

\mathop{\varphi\mbox{-Var}}_{[0, T]} (f) := \sup \sum_{j = 0}^{k} \varphi \left( | f(t_{j + 1}) - f(t_{j}) |_{X} \right),

where, as usual, the supremum is taken over all finite partitions of the interval [0, T], i.e. all the finite sets of real numbers t_i such that

0 = t_{0} < t_{1} < \ldots < t_{k} = T.

The original notion of variation considered above is the special case of \scriptstyle \varphi-variation for which the weight function is the identity function: therefore an integrable function f is said to be a weighted BV function (of weight \scriptstyle\varphi) if and only if its \scriptstyle \varphi-variation is finite.

f\in BV_\varphi([0, T];X)\iff \mathop{\varphi\mbox{-Var}}_{[0, T]} (f) <+\infty

The space \scriptstyle BV_\varphi([0, T];X) is a topological vector space with respect to the norm

\| f \|_{BV_\varphi} := \| f \|_{\infty} + \mathop{\varphi \mbox{-Var}}_{[0, T]} (f),

where \scriptstyle\| f \|_{\infty} denotes the usual supremum norm of f. Weighted BV functions were introduced and studied in full generality by Władysław Orlicz and Julian Musielak in the paper Musielak & Orlicz 1959: Laurence Chisholm Young studied earlier the case \scriptstyle\varphi(x)=x^p where p is a positive integer.

SBV functions

SBV functions i.e. Special functions of Bounded Variation were introduced by Luigi Ambrosio and Ennio de Giorgi in the paper (Ambrosio & De Giorgi 1988), dealing with free discontinuity variational problems: given an open subset  \Omega of ℝn, the space SBV(\Omega) is a proper linear subspace of BV(\Omega), since the weak gradient of each function belonging to it consists precisely of the sum of an n-dimensional support and an n-1-dimensional support measure and no intermediate-dimensional terms, as seen in the following definition.

Definition. Given a locally integrable function u, then \scriptstyle u\in {S\!BV}(\Omega) if and only if

1. There exist two Borel functions f and g of domain \Omega and codomainn such that

 \int_\Omega\vert f\vert dH^n+ \int_\Omega\vert g\vert dH^{n-1}<+\infty.

2. For all of continuously differentiable vector functions  \scriptstyle\phi of compact support contained in  \Omega , i.e. for all  \scriptstyle \phi \in
C_c^1(\Omega,\mathbb{R}^n) the following formula is true:

 \int_\Omega u\mbox{div} \phi dH^n = \int_\Omega \langle \phi, f\rangle dH^n +\int_\Omega \langle \phi, g\rangle dH^{n-1}.

where H^\alpha is the \alpha-dimensional Hausdorff measure.

Details on the properties of SBV functions can be found in works cited in the bibliography section: particularly the paper (De Giorgi 1992) contains a useful bibliography.

bv sequences

As particular examples of Banach spaces, Dunford & Schwartz (1958, Chapter IV) consider spaces of sequences of bounded variation, in addition to the spaces of functions of bounded variation. The total variation of a sequence x=(xi) of real or complex numbers is defined by

TV(x) = \sum_{i=1}^\infty |x_{i+1}-x_i|.

The space of all sequences of finite total variation is denoted by bv. The norm on bv is given by

\|x\|_{bv} = |x_1| + TV(x) = |x_1| +  \sum_{i=1}^\infty |x_{i+1}-x_i|.

With this norm, the space bv is a Banach space.

The total variation itself defines a norm on a certain subspace of bv, denoted by bv0, consisting of sequences x = (xi) for which

\lim_{n\to\infty} x_n =0.

The norm on bv0 is denoted

\|x\|_{bv_0} = TV(x) = \sum_{i=1}^\infty |x_{i+1}-x_i|.

With respect to this norm bv0 becomes a Banach space as well.

Measures of bounded variation

A signed (or complex) measure \mu on a measurable space (X,\Sigma) is said to be of bounded variation if its total variation \scriptstyle\Vert \mu\Vert=|\mu|(X) is bounded: see Halmos (1950, p. 123), Kolmogorov & Fomin (1969, p. 346) or the entry "Total variation" for further details.

Examples

The function f(x)=sin(1/x) is not of bounded variation on the interval  [0,2 / \pi] .

The function

f(x) = \begin{cases} 0, & \mbox{if }x =0 \\ \sin(1/x), & \mbox{if } x \neq 0 \end{cases}

is not of bounded variation on the interval  [0, 2/\pi]

The function f(x)=x sin(1/x) is not of bounded variation on the interval  [0,2 / \pi] .

While it is harder to see, the continuous function

f(x) = \begin{cases} 0, & \mbox{if }x =0 \\ x \sin(1/x), & \mbox{if } x \neq 0 \end{cases}

is not of bounded variation on the interval  [0, 2/\pi] either.

The function f(x)=x2 sin(1/x) is of bounded variation on the interval  [0,2 / \pi] .

At the same time, the function

f(x) = \begin{cases} 0, & \mbox{if }x =0 \\ x^2 \sin(1/x), & \mbox{if } x \neq 0 \end{cases}

is of bounded variation on the interval  [0,2/\pi]. However, all three functions are of bounded variation on each interval [a,b] with a>0.

The Sobolev space  W^{1,1}(\Omega) is a proper subset of  BV(\Omega). In fact, for each  u in  W^{1,1}(\Omega) it is possible to choose a measure  \scriptstyle \mu:=\nabla u \mathcal L (where  \scriptstyle\mathcal L is the Lebesgue measure on \Omega) such that the equality

 \int u\mathrm{div}\phi = -\int \phi\, d\mu = -\int \phi \nabla u \qquad \forall \phi\in C_c^1

holds, since it is nothing more than the definition of weak derivative, and hence holds true. One can easily find an example of a BV function which is not W^{1,1}: in dimension one, any step function with a non-trivial jump will do.

Applications

Mathematics

Functions of bounded variation have been studied in connection with the set of discontinuities of functions and differentiability of real functions, and the following results are well-known. If f is a real function of bounded variation on an interval [a,b] then

For real functions of several real variables

Physics and engineering

The ability of BV functions to deal with discontinuities has made their use widespread in the applied sciences: solutions of problems in mechanics, physics, chemical kinetics are very often representable by functions of bounded variation. The book (Hudjaev & Vol'pert 1985) details a very ample set of mathematical physics applications of BV functions. Also there is some modern application which deserves a brief description.

See also

Notes

  1. Tonelli introduced what is now called after him Tonelli plane variation: for an analysis of this concept and its relations to other generalizations, see the entry "Total variation".
  2. 1 2 See the entry "Total variation" for further details and more information.
  3. See for example Kolmogorov & Fomin (1969, pp. 374–376).
  4. For a general reference on this topic, see Riesz & Szőkefalvi-Nagy (1990)
  5. In this context, "finite" means that its value is never infinite, i.e. it is a finite measure.
  6. The example is taken from Giaquinta, Modica & Souček (1998, p. 331): see also (Kannan & Krueger 1996, example 9.4.1, p. 237).
  7. The same argument is used by Kolmogorov & Fomin (1969, example 7, pp. 48–49), in order to prove the non separability of the space of bounded sequences, and also Kannan & Krueger (1996, example 9.4.1, p. 237).

References

Research works

Historical references

External links

Theory

Other

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