In mathematics, a differential operator is an operator defined as a function of the differentiation operator. It is helpful, as a matter of notation first, to consider differentiation as an abstract operation that accepts a function and returns another function (in the style of a higher-order function in computer science).
This article considers mainly linear differential operators, which are the most common type. However, non-linear differential operators also exist, such as the Schwarzian derivative.
Given a nonnegative integer m, an order-
m
P
l{F}1
l{F}2
\le m |
\alpha=(\alpha1,\alpha2, … ,\alphan)
|\alpha|=\alpha1+\alpha2+ … +\alphan
\alpha
a\alpha(x)
D\alpha
Thus for a function
f\inl{F}1
\le m |
The notation
D\alpha
The polynomial p obtained by replacing D by variables
\xi
\xi\alpha=
\alpha1 | |
\xi | |
1 |
…
\alphan | |
\xi | |
n |
.
\sigma(x,\xi)=\sum|\alpha|=a\alpha(x)\xi\alpha
More generally, let E and F be vector bundles over a manifold X. Then the linear operator
P:Cinfty(E)\toCinfty(F)
is a differential operator of order
k
Pu(x)=\sum|\alpha|P\alpha(x)
\partial\alphau | |
\partialx\alpha |
+lower-orderterms
where, for each multi-index α,
P\alpha(x):E\toF
The kth order coefficients of P transform as a symmetric tensor
\sigmaP:Sk(T*X) ⊗ E\toF
whose domain is the tensor product of the kth symmetric power of the cotangent bundle of X with E, and whose codomain is F. This symmetric tensor is known as the principal symbol (or just the symbol) of P.
The coordinate system xi permits a local trivialization of the cotangent bundle by the coordinate differentials dxi, which determine fiber coordinates ξi. In terms of a basis of frames eμ, fν of E and F, respectively, the differential operator P decomposes into components
(Pu)\nu=\sum\muP\nu\muu\mu
on each section u of E. Here Pνμ is the scalar differential operator defined by
P\nu\mu=\sum\alpha
| ||||
P | ||||
\nu\mu |
.
With this trivialization, the principal symbol can now be written
(\sigmaP(\xi)u)\nu=\sum|\alpha|=k\sum\mu
\alpha(x)\xi | |
P | |
\alpha |
u\mu.
In the cotangent space over a fixed point x of X, the symbol
\sigmaP
* | |
T | |
x |
X
\operatorname{Hom}(Ex,Fx)
A differential operator P and its symbol appear naturally in connection with the Fourier transform as follows. Let ƒ be a Schwartz function. Then by the inverse Fourier transform,
Pf(x)=
1 | |||||||
|
\int\limits | |
Rd |
ep(x,i\xi)\hat{f}(\xi)d\xi.
This exhibits P as a Fourier multiplier. A more general class of functions p(x,ξ) which satisfy at most polynomial growth conditions in ξ under which this integral is well-behaved comprises the pseudo-differential operators.
P
\theta\inT*X
\sigmaP(\theta,...,\theta)
Del defines the gradient, and is used to calculate the curl, divergence, and Laplacian of various objects.
The conceptual step of writing a differential operator as something free-standing is attributed to Louis François Antoine Arbogast in 1800.[1]
The most common differential operator is the action of taking the derivative. Common notations for taking the first derivative with respect to a variable x include:
{d\overdx}
D
Dx,
\partialx
When taking higher, nth order derivatives, the operator may be written:
{dn\overdxn}
Dn
n | |
D | |
x |
n | |
\partial | |
x |
The derivative of a function f of an argument x is sometimes given as either of the following:
[f(x)]'
f'(x).
The D notation's use and creation is credited to Oliver Heaviside, who considered differential operators of the form
n | |
\sum | |
k=0 |
ckDk
in his study of differential equations.
One of the most frequently seen differential operators is the Laplacian operator, defined by
\Delta=\nabla2=
n | |
\sum | |
k=1 |
\partial2 | ||||||||
|
.
Another differential operator is the Θ operator, or theta operator, defined by[2]
\Theta=z{d\overdz}.
This is sometimes also called the homogeneity operator, because its eigenfunctions are the monomials in z:
In n variables the homogeneity operator is given by
As in one variable, the eigenspaces of Θ are the spaces of homogeneous functions. (Euler's homogeneous function theorem)
In writing, following common mathematical convention, the argument of a differential operator is usually placed on the right side of the operator itself. Sometimes an alternative notation is used: The result of applying the operator to the function on the left side of the operator and on the right side of the operator, and the difference obtained when applying the differential operator to the functions on both sides, are denoted by arrows as follows:
f\overleftarrow{\partialx}g=g ⋅ \partialxf
f\overrightarrow{\partialx}g=f ⋅ \partialxg
f\overleftrightarrow{\partialx}g=f ⋅ \partialxg-g ⋅ \partialxf.
See also: Hermitian adjoint. Given a linear differential operator
T
T*
\langle ⋅ , ⋅ \rangle
In the functional space of square-integrable functions on a real interval, the scalar product is defined by
where the line over f(x) denotes the complex conjugate of f(x). If one moreover adds the condition that f or g vanishes as
x\toa
x\tob
This formula does not explicitly depend on the definition of the scalar product. It is therefore sometimes chosen as a definition of the adjoint operator. When
T*
A (formally) self-adjoint operator is an operator equal to its own (formal) adjoint.
If Ω is a domain in Rn, and P a differential operator on Ω, then the adjoint of P is defined in L2(Ω) by duality in the analogous manner:
\langlef,P*
g\rangle | |
L2(\Omega) |
=\langlePf,
g\rangle | |
L2(\Omega) |
for all smooth L2 functions f, g. Since smooth functions are dense in L2, this defines the adjoint on a dense subset of L2: P* is a densely defined operator.
The Sturm - Liouville operator is a well-known example of a formal self-adjoint operator. This second-order linear differential operator L can be written in the form
Lu=-(pu')'+qu=-(pu''+p'u')+qu=-pu''-p'u'+qu=(-p)D2u+(-p')Du+(q)u.
This property can be proven using the formal adjoint definition above.[3]
This operator is central to Sturm–Liouville theory where the eigenfunctions (analogues to eigenvectors) of this operator are considered.
Differentiation is linear, i.e.
D(f+g)=(Df)+(Dg),
D(af)=a(Df),
where f and g are functions, and a is a constant.
Any polynomial in D with function coefficients is also a differential operator. We may also compose differential operators by the rule
(D1\circD2)(f)=D1(D2(f)).
Some care is then required: firstly any function coefficients in the operator D2 must be differentiable as many times as the application of D1 requires. To get a ring of such operators we must assume derivatives of all orders of the coefficients used. Secondly, this ring will not be commutative: an operator gD isn't the same in general as Dg. For example we have the relation basic in quantum mechanics:
Dx-xD=1.
The subring of operators that are polynomials in D with constant coefficients is, by contrast, commutative. It can be characterised another way: it consists of the translation-invariant operators.
The differential operators also obey the shift theorem.
See main article: Weyl algebra.
If R is a ring, let
R\langleD,X\rangle
R\langleD,X\rangle/I
XaDbmodI
Differential modules over
R[X]
R\langleD,X\rangle/I
If R is a ring, let
R\langleD1,\ldots,Dn,X1,\ldots,Xn\rangle
D1,\ldots,Dn,X1,\ldots,Xn
(DiXj-XjDi)-\deltai,j, DiDj-DjDi, XiXj-XjXi
1\lei,j\len,
\delta
This is a simple ring.Every element can be written in a unique way as a R-linear combination of monomials of the form
In differential geometry and algebraic geometry it is often convenient to have a coordinate-independent description of differential operators between two vector bundles. Let E and F be two vector bundles over a differentiable manifold M. An R-linear mapping of sections is said to be a kth-order linear differential operator if it factors through the jet bundle Jk(E).In other words, there exists a linear mapping of vector bundles
iP:Jk(E)\toF
such that
P=iP\circjk
where is the prolongation that associates to any section of E its k-jet.
This just means that for a given section s of E, the value of P(s) at a point x ∈ M is fully determined by the kth-order infinitesimal behavior of s in x. In particular this implies that P(s)(x) is determined by the germ of s in x, which is expressed by saying that differential operators are local. A foundational result is the Peetre theorem showing that the converse is also true: any (linear) local operator is differential.
An equivalent, but purely algebraic description of linear differential operators is as follows: an R-linear map P is a kth-order linear differential operator, if for any k + 1 smooth functions
f0,\ldots,fk\inCinfty(M)
[fk,[fk-1,[ … [f0,P] … ]]=0.
Here the bracket
[f,P]:\Gamma(E)\to\Gamma(F)
[f,P](s)=P(f ⋅ s)-f ⋅ P(s).
This characterization of linear differential operators shows that they are particular mappings between modules over a commutative algebra, allowing the concept to be seen as a part of commutative algebra.
A differential operator of infinite order is (roughly) a differential operator whose total symbol is a power series instead of a polynomial.
A differential operator acting on two functions
D(g,f)
A microdifferential operator is a type of operator on an open subset of a cotangent bundle, as opposed to an open subset of a manifold. It is obtained by extending the notion of a differential operator to the cotangent bundle.
\begin{align} L*u&{}=(-1)2D2[(-p)u]+(-1)1D[(-p')u]+(-1)0(qu)\\ &{}=-D2(pu)+D(p'u)+qu\\ &{}=-(pu)''+(p'u)'+qu\\ &{}=-p''u-2p'u'-pu''+p''u+p'u'+qu\\ &{}=-p'u'-pu''+qu\\ &{}=-(pu')'+qu\\ &{}=Lu \end{align}