It is sometimes denoted by a delta with a bar: or .
Definition
Given n+1 data points
where the are assumed to be pairwise distinct, the forward divided differences are defined as:
To make the recursive process of computation clearer, the divided differences can be put in tabular form, where the columns correspond to the value of j above, and each entry in the table is computed from the difference of the entries to its immediate lower left and to its immediate upper left, divided by a difference of corresponding x-values:
Notation
Note that the divided difference depends on the values and , but the notation hides the dependency on the x-values. If the data points are given by a function f,
one sometimes writes the divided difference in the notation
Other notations for the divided difference of the function ƒ on the nodes x0,...,xn are:
Example
Divided differences for and the first few values of :
Thus, the table corresponding to these terms up to two columns has the following form:
The divided difference scheme can be put into an upper triangular matrix:
Then it holds
if is a scalar
This follows from the Leibniz rule. It means that multiplication of such matrices is commutative. Summarised, the matrices of divided difference schemes with respect to the same set of nodes x form a commutative ring.
Since is a triangular matrix, its eigenvalues are obviously .
Let be a Kronecker delta-like function, that is Obviously , thus is an eigenfunction of the pointwise function multiplication. That is is somehow an "eigenmatrix" of : . However, all columns of are multiples of each other, the matrix rank of is 1. So you can compose the matrix of all eigenvectors of from the -th column of each . Denote the matrix of eigenvectors with . Example The diagonalization of can be written as
Polynomials and power series
The matrix
contains the divided difference scheme for the identity function with respect to the nodes , thus contains the divided differences for the power function with exponent.
Consequently, you can obtain the divided differences for a polynomial function by applying to the matrix : If
and
then
This is known as Opitz' formula.
Now consider increasing the degree of to infinity, i.e. turn the Taylor polynomial into a Taylor series.
Let be a function which corresponds to a power series.
You can compute the divided difference scheme for by applying the corresponding matrix series to :
If
and
then
If and , the divided differences can be expressed as
where is the -th derivative of the function and is a certain B-spline of degree for the data points , given by the formula
This is a consequence of the Peano kernel theorem; it is called the Peano form of the divided differences and is the Peano kernel for the divided differences, all named after Giuseppe Peano.
Hermite–Genocchi formula
When is times continuously differentiable on a convex domain containing the nodes , including the confluent case of repeated nodes in arbitrary order (see §Generalization), the divided difference can be expressed as an integral over a -simplex :
where
is the -simplex.
When is analytic on a simply connected domain containing the nodes , including the confluent case of repeated nodes in arbitrary order (see §Generalization), the divided difference admits a contour integral representation via Cauchy's integral formula:
where is a positively oriented, simple closed contour in enclosing all the nodes .
When the data points are equidistantly distributed we get the special case called forward differences. They are easier to calculate than the more general divided differences.
Given n+1 data points
with
the forward differences are defined as:
whereas the backward differences are defined as:
Thus the forward difference table is written as:
whereas the backwards difference table is written as:
The relationship between divided differences and forward differences is
whereas for backward differences:[citation needed]
Explicit formula
When the data points are equispaced we can also derive an explicit formula for . For any fixed and such that ,
Proof. We prove this by induction on :
Base case: Let and . Then by definition , and
Induction step: Assume the above formula holds until and consider such that . By the recursive definition we have
We can use our inductive hypothesis on both members of the left side, and obtain
This can be rearranged as
where when . We obtain our thesis for by substituting the identity
Generalization
When some of the nodes coincide, the recursive definition of standard divided differences involves division by zero and can no longer be applied directly. In this confluent case, divided differences incorporate higher-order derivatives of the function . The resulting values are known as confluent divided differences or generalized divided differences. Conceptually, node confluence bridges discrete divided differences and continuous calculus, replacing finite differences with exact higher-order derivatives as nodes coalesce.
Let consist of nodes with arbitrary repetitions and order. Suppose there are distinct values among the nodes, with corresponding multiplicities such that . Let be a function that is times differentiable at for .
Confluent divided differences can be defined as the limit:
where are pairwise distinct nodes converging to , provided the limit exists.
In practice, any confluent divided difference with arbitrarily ordered repeated nodes can be computed by first permuting the node sequence so that identical nodes are adjacent, and then constructing the divided difference table with an additional higher-order derivative substitution rule.
Divided differences remain symmetric in in the confluent case, satisfying:
where is a permutation that reorders .
Consider the case where reorders such that identical nodes become contiguous:
In this case, the divided difference table is constructed using the standard recursive formula whenever the outer nodes are distinct. When evaluating divided differences on identical nodes , the calculation reduces to and coincides with a scaled higher-order derivative of :
All other entries in the divided difference table are then computed using the standard recursive rule.
Generalized case example
To evaluate a confluent divided difference with non-adjacent repeated nodes, such as , the node sequence is first permuted to group identical nodes contiguously:
The evaluation then proceeds by constructing the divided difference table:
Extracting and simplifying the rightmost entry from the resulting divided difference table yields:
Myron B. Allen; Eli L. Isaacson (1998). Numerical Analysis for Applied Science. John Wiley & Sons. Appendix A. ISBN978-1-118-03027-1.
Ron Goldman (2002). Pyramid Algorithms: A Dynamic Programming Approach to Curves and Surfaces for Geometric Modeling. Morgan Kaufmann. Chapter 4:Newton Interpolation and Difference Triangles. ISBN978-0-08-051547-2.