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{{distinguish|Ornstein–Uhlenbeck process}}


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In [[mathematics]], the '''Ornstein–Uhlenbeck operator''' is a generalization of the [[Laplace operator]] to an infinite-dimensional setting. The Ornstein–Uhlenbeck operator plays a significant role in the [[Malliavin calculus]].
 
==Introduction: the finite-dimensional picture==
 
===The Laplacian===
 
Consider the [[gradient]] operator &nabla; acting on scalar functions ''f''&nbsp;:&nbsp;'''R'''<sup>''n''</sup>&nbsp;&rarr;&nbsp;'''R'''; the gradient of a scalar function is a [[vector field]] ''v''&nbsp;=&nbsp;&nabla;''f''&nbsp;:&nbsp;'''R'''<sup>''n''</sup>&nbsp;&rarr;&nbsp;'''R'''<sup>''n''</sup>. The [[divergence]] operator div, acting on vector fields to produce scalar fields, is the [[adjoint operator]] to &nabla;. The Laplace operator &Delta; is then the [[function composition|composition]] of the divergence and gradient operators:
 
:<math>\Delta = \mathrm{div} \circ \nabla</math>,
 
acting on scalar functions to produce scalar functions. Note that ''A''&nbsp;=&nbsp;&minus;&Delta; is a positive operator, whereas &Delta; is a [[dissipative operator]].
 
Using [[spectral theory]], one can define a [[square root]] (1&nbsp;&minus;&nbsp;&Delta;)<sup>1/2</sup> for the operator (1&nbsp;&minus;&nbsp;&Delta;). This square root satisfies the following relation involving the [[Sobolev space|Sobolev ''H''<sup>1</sup>-norm]] and [[Lp space|''L''<sup>2</sup>-norm]] for suitable scalar functions ''f'':
 
:<math>\big\| f \big\|_{H^{1}}^{2} = \big\| (1 - \Delta)^{1/2} f \big\|_{L^{2}}^{2}.</math>
 
===The Ornstein–Uhlenbeck operator===
 
Often, when working on '''R'''<sup>''n''</sup>, one works with respect to [[Lebesgue measure]], which has many nice properties. However, remember that the aim is to work in ''infinite''-dimensional spaces, and it is a fact that [[there is no infinite-dimensional Lebesgue measure]]. Instead, if one is studying some [[separable space|separable]] [[Banach space]] ''E'', what does make sense is a notion of [[Gaussian measure]];  in particular, the [[abstract Wiener space]] construction makes sense.
 
To get some intuition about what can be expected in the infinite-dimensional setting, consider standard Gaussian measure ''&gamma;''<sup>''n''</sup> on '''R'''<sup>''n''</sup>:  for Borel subsets ''A'' of '''R'''<sup>''n''</sup>,
 
:<math>\gamma^{n} (A) := \int_{A} (2 \pi)^{-n/2} \exp ( - | x |^{2} / 2) \, \mathrm{d} x.</math>
 
This makes ('''R'''<sup>''n''</sup>,&nbsp;''B''('''R'''<sup>''n''</sup>),&nbsp;''&gamma;''<sup>''n''</sup>) into a [[probability space]];  '''E''' will denote [[expected value|expectation]] with respect to ''&gamma;''<sup>''n''</sup>.
 
The '''gradient operator''' &nabla; acts on a (differentiable) function ''&phi;''&nbsp;:&nbsp;'''R'''<sup>''n''</sup>&nbsp;&rarr;&nbsp;'''R''' to give a [[vector field]] &nabla;''&phi;''&nbsp;:&nbsp;'''R'''<sup>''n''</sup>&nbsp;&rarr;&nbsp;'''R'''<sup>''n''</sup>
 
The '''divergence operator''' ''&delta;'' (to be more precise, ''&delta;''<sub>''n''</sup>, since it depends on the dimension) is now defined to be the [[adjoint operator|adjoint]] of &nabla; in the [[Hilbert space]] sense, in the Hilbert space ''L''<sup>2</sup>('''R'''<sup>''n''</sup>,&nbsp;''B''('''R'''<sup>''n''</sup>),&nbsp;''&gamma;''<sup>''n''</sup>;&nbsp;'''R'''). In other words, ''&delta;'' acts on a vector field ''v''&nbsp;:&nbsp;'''R'''<sup>''n''</sup>&nbsp;&rarr;&nbsp;'''R'''<sup>''n''</sup> to give a scalar function ''&delta;v''&nbsp;:&nbsp;'''R'''<sup>''n''</sup>&nbsp;&rarr;&nbsp;'''R''', and satisfies the formula
 
:<math>\mathbb{E} \big[ \nabla f \cdot v \big] = \mathbb{E} \big[ f \delta v \big].</math>
 
On the left, the product is the pointwise Euclidean [[dot product]] of two vector fields;  on the right, it is just the pointwise multiplication of two functions. Using [[integration by parts]], one can check that ''&delta;'' acts on a vector field ''v'' with components ''v''<sup>''i''</sup>, ''i''&nbsp;=&nbsp;1, ..., ''n'', as follows:
 
:<math>\delta v (x) = \sum_{i = 1}^{n} \left( x_{i} v^{i} (x) - \frac{\partial v^{i}}{\partial x_{i}} (x) \right).</math>
 
The change of notation from &ldquo;div&rdquo; to &ldquo;''&delta;''&rdquo; is for two reasons:  first, ''&delta;'' is the notation used in infinite dimensions (the Malliavin calculus);  secondly, ''&delta;'' is really the ''negative'' of the usual divergence.
 
The (finite-dimensional) '''Ornstein–Uhlenbeck operator''' ''L'' (or, to be more precise, ''L''<sub>''m''</sub>) is defined by
 
:<math>L := - \delta \circ \nabla,</math>
 
with the useful formula that for any ''f'' and ''g'' smooth enough for all the terms to make sense,
 
:<math>\delta ( f \nabla g) = - \nabla f \cdot \nabla g - f L g.</math>
 
The Ornstein–Uhlenbeck operator ''L'' is related to the usual Laplacian &Delta; by
 
:<math>L f (x) = \Delta f (x) - x \cdot \nabla f (x).</math>
 
==The Ornstein–Uhlenbeck operator for a separable Banach space==
 
Consider now an [[abstract Wiener space]] ''E'' with Cameron-Martin Hilbert space ''H'' and Wiener measure ''&gamma;''. Let D denote the [[Malliavin derivative]]. The Malliavin derivative D is an [[unbounded operator]] from ''L''<sup>2</sup>(''E'',&nbsp;''&gamma;'';&nbsp;'''R''') into ''L''<sup>2</sup>(''E'',&nbsp;''&gamma;'';&nbsp;''H'') &ndash; in some sense, it measures &ldquo;how random&rdquo; a function on ''E'' is. The domain of D is not the whole of ''L''<sup>2</sup>(''E'',&nbsp;''&gamma;'';&nbsp;'''R'''), but is a [[dense set|dense]] [[linear subspace]], the Watanabe-Sobolev space, often denoted by <math>\mathbb{D}^{1,2}</math> (once differentiable in the sense of Malliavin, with derivative in ''L''<sup>2</sup>).
 
Again, ''&delta;'' is defined to be the adjoint of the gradient operator (in this case, the Malliavin derivative is playing the role of the gradient operator). The operator ''&delta;'' is also known the [[Skorokhod integral]], which is an anticipating [[stochastic integral]];  it is this set-up that gives rise to the slogan &ldquo;stochastic integrals are divergences&rdquo;. ''&delta;'' satisfies the identity
 
:<math>\mathbb{E} \big[ \langle \mathrm{D} F, v \rangle_{H} \big] = \mathbb{E} \big[ F \delta v \big]</math>
 
for all ''F'' in <math>\mathbb{D}^{1,2}</math> and ''v'' in the domain of ''&delta;''.
 
Then the '''Ornstein–Uhlenbeck operator''' for ''E'' is the operator ''L'' defined by
 
:<math>L := - \delta \circ \mathrm{D}.</math>
 
==References==
 
* {{cite book
| last = Ocone
| first = Daniel L.
| chapter = A guide to the stochastic calculus of variations
| title = Stochastic analysis and related topics (Silivri, 1986)
| series = Lecture Notes in Math. 1316
| pages = 1&ndash;79
| publisher = Springer
| location = Berlin
| year = 1988
}} {{MathSciNet|id=953793}}
* {{cite web
| last = Sanz-Solé
| first = Marta
| title = Applications of Malliavin Calculus to Stochastic Partial Differential Equations (Lectures given at Imperial College London, 7&ndash;11 July 2008)
| year = 2008
| url = http://www.ma.ic.ac.uk/~dcrisan/lecturenotes-london.pdf
| accessdate = 2008-07-09
}}
 
{{DEFAULTSORT:Ornstein-Uhlenbeck operator}}
[[Category:Operator theory]]
[[Category:Stochastic calculus]]

Revision as of 04:40, 31 January 2014

Template:Distinguish

In mathematics, the Ornstein–Uhlenbeck operator is a generalization of the Laplace operator to an infinite-dimensional setting. The Ornstein–Uhlenbeck operator plays a significant role in the Malliavin calculus.

Introduction: the finite-dimensional picture

The Laplacian

Consider the gradient operator ∇ acting on scalar functions f : Rn → R; the gradient of a scalar function is a vector field v = ∇f : Rn → Rn. The divergence operator div, acting on vector fields to produce scalar fields, is the adjoint operator to ∇. The Laplace operator Δ is then the composition of the divergence and gradient operators:

Δ=div,

acting on scalar functions to produce scalar functions. Note that A = −Δ is a positive operator, whereas Δ is a dissipative operator.

Using spectral theory, one can define a square root (1 − Δ)1/2 for the operator (1 − Δ). This square root satisfies the following relation involving the Sobolev H1-norm and L2-norm for suitable scalar functions f:

fH12=(1Δ)1/2fL22.

The Ornstein–Uhlenbeck operator

Often, when working on Rn, one works with respect to Lebesgue measure, which has many nice properties. However, remember that the aim is to work in infinite-dimensional spaces, and it is a fact that there is no infinite-dimensional Lebesgue measure. Instead, if one is studying some separable Banach space E, what does make sense is a notion of Gaussian measure; in particular, the abstract Wiener space construction makes sense.

To get some intuition about what can be expected in the infinite-dimensional setting, consider standard Gaussian measure γn on Rn: for Borel subsets A of Rn,

γn(A):=A(2π)n/2exp(|x|2/2)dx.

This makes (RnB(Rn), γn) into a probability space; E will denote expectation with respect to γn.

The gradient operator ∇ acts on a (differentiable) function φ : Rn → R to give a vector fieldφ : Rn → Rn.

The divergence operator δ (to be more precise, δn, since it depends on the dimension) is now defined to be the adjoint of ∇ in the Hilbert space sense, in the Hilbert space L2(RnB(Rn), γnR). In other words, δ acts on a vector field v : Rn → Rn to give a scalar function δv : Rn → R, and satisfies the formula

𝔼[fv]=𝔼[fδv].

On the left, the product is the pointwise Euclidean dot product of two vector fields; on the right, it is just the pointwise multiplication of two functions. Using integration by parts, one can check that δ acts on a vector field v with components vi, i = 1, ..., n, as follows:

δv(x)=i=1n(xivi(x)vixi(x)).

The change of notation from “div” to “δ” is for two reasons: first, δ is the notation used in infinite dimensions (the Malliavin calculus); secondly, δ is really the negative of the usual divergence.

The (finite-dimensional) Ornstein–Uhlenbeck operator L (or, to be more precise, Lm) is defined by

L:=δ,

with the useful formula that for any f and g smooth enough for all the terms to make sense,

δ(fg)=fgfLg.

The Ornstein–Uhlenbeck operator L is related to the usual Laplacian Δ by

Lf(x)=Δf(x)xf(x).

The Ornstein–Uhlenbeck operator for a separable Banach space

Consider now an abstract Wiener space E with Cameron-Martin Hilbert space H and Wiener measure γ. Let D denote the Malliavin derivative. The Malliavin derivative D is an unbounded operator from L2(EγR) into L2(EγH) – in some sense, it measures “how random” a function on E is. The domain of D is not the whole of L2(EγR), but is a dense linear subspace, the Watanabe-Sobolev space, often denoted by 𝔻1,2 (once differentiable in the sense of Malliavin, with derivative in L2).

Again, δ is defined to be the adjoint of the gradient operator (in this case, the Malliavin derivative is playing the role of the gradient operator). The operator δ is also known the Skorokhod integral, which is an anticipating stochastic integral; it is this set-up that gives rise to the slogan “stochastic integrals are divergences”. δ satisfies the identity

𝔼[DF,vH]=𝔼[Fδv]

for all F in 𝔻1,2 and v in the domain of δ.

Then the Ornstein–Uhlenbeck operator for E is the operator L defined by

L:=δD.

References