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{{distinguish|Ornstein–Uhlenbeck process}} | |||
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'' : '''R'''<sup>''n''</sup> → '''R'''; the gradient of a scalar function is a [[vector field]] ''v'' = ∇''f'' : '''R'''<sup>''n''</sup> → '''R'''<sup>''n''</sup>. The [[divergence]] operator div, acting on vector fields to produce scalar fields, is the [[adjoint operator]] to ∇. The Laplace operator Δ 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'' = −Δ is a positive operator, whereas Δ is a [[dissipative operator]]. | |||
Using [[spectral theory]], one can define a [[square root]] (1 − Δ)<sup>1/2</sup> for the operator (1 − Δ). 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 ''γ''<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>, ''B''('''R'''<sup>''n''</sup>), ''γ''<sup>''n''</sup>) into a [[probability space]]; '''E''' will denote [[expected value|expectation]] with respect to ''γ''<sup>''n''</sup>. | |||
The '''gradient operator''' ∇ acts on a (differentiable) function ''φ'' : '''R'''<sup>''n''</sup> → '''R''' to give a [[vector field]] ∇''φ'' : '''R'''<sup>''n''</sup> → '''R'''<sup>''n''</sup>. | |||
The '''divergence operator''' ''δ'' (to be more precise, ''δ''<sub>''n''</sup>, since it depends on the dimension) is now defined to be the [[adjoint operator|adjoint]] of ∇ in the [[Hilbert space]] sense, in the Hilbert space ''L''<sup>2</sup>('''R'''<sup>''n''</sup>, ''B''('''R'''<sup>''n''</sup>), ''γ''<sup>''n''</sup>; '''R'''). In other words, ''δ'' acts on a vector field ''v'' : '''R'''<sup>''n''</sup> → '''R'''<sup>''n''</sup> to give a scalar function ''δv'' : '''R'''<sup>''n''</sup> → '''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 ''δ'' acts on a vector field ''v'' with components ''v''<sup>''i''</sup>, ''i'' = 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 “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, ''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 Δ 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 ''γ''. Let D denote the [[Malliavin derivative]]. The Malliavin derivative D is an [[unbounded operator]] from ''L''<sup>2</sup>(''E'', ''γ''; '''R''') into ''L''<sup>2</sup>(''E'', ''γ''; ''H'') – in some sense, it measures “how random” a function on ''E'' is. The domain of D is not the whole of ''L''<sup>2</sup>(''E'', ''γ''; '''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, ''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 | |||
:<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 ''δ''. | |||
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 = 1–79 | |||
| 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, 7–11 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
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:
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:
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,
This makes (Rn, B(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 field ∇φ : 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(Rn, B(Rn), γn; R). In other words, δ acts on a vector field v : Rn → Rn to give a scalar function δv : Rn → R, and satisfies the formula
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:
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
with the useful formula that for any f and g smooth enough for all the terms to make sense,
The Ornstein–Uhlenbeck operator L is related to the usual Laplacian Δ by
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(E, γ; R) into L2(E, γ; H) – in some sense, it measures “how random” a function on E is. The domain of D is not the whole of L2(E, γ; R), but is a dense linear subspace, the Watanabe-Sobolev space, often denoted by (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
for all F in and v in the domain of δ.
Then the Ornstein–Uhlenbeck operator for E is the operator L defined by
References
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