Divided_differences

In mathematics, divided differences is an algorithm, historically used for computing tables of logarithms and trigonometric functions.^{[citation needed]} Charles Babbage's difference engine, an early mechanical calculator, was designed to use this algorithm in its operation.^[1]

Divided differences is a recursive division process. Given a sequence of data points ${\displaystyle (x_{0},y_{0}),\ldots ,(x_{n},y_{n})}$, the method calculates the coefficients of the interpolation polynomial of these points in the Newton form.

Given n + 1 data points $${\displaystyle (x_{0},y_{0}),\ldots ,(x_{n},y_{n})}$$ where the ${\displaystyle x_{k}$ are assumed to be pairwise distinct, the forward divided differences are defined as: $${\displaystyle {\begin{aligned}{\mathopen {[}y_{k}]&:=y_{k},&&k\in \{0,\ldots ,n\}\\{\mathopen {[}y_{k},\ldots ,y_{k+j}]&:={\frac {[y_{k+1},\ldots ,y_{k+j}]-[y_{k},\ldots ,y_{k+j-1}]}{x_{k+j}-x_{k},&&k\in \{0,\ldots ,n-j\},\ j\in \{1,\ldots ,n\}.\end{aligned}$$

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: $${\displaystyle {\begin{matrix}x_{0}&y_{0}=[y_{0}]&&&\\&&[y_{0},y_{1}]&&\\x_{1}&y_{1}=[y_{1}]&&[y_{0},y_{1},y_{2}]&\\&&[y_{1},y_{2}]&&[y_{0},y_{1},y_{2},y_{3}]\\x_{2}&y_{2}=[y_{2}]&&[y_{1},y_{2},y_{3}]&\\&&[y_{2},y_{3}]&&\\x_{3}&y_{3}=[y_{3}]&&&\\\end{matrix}$$

Note that the divided difference ${\displaystyle [y_{k},\ldots ,y_{k+j}]}$ depends on the values ${\displaystyle x_{k},\ldots ,x_{k+j}$ and ${\displaystyle y_{k},\ldots ,y_{k+j}$, but the notation hides the dependency on the x-values. If the data points are given by a function f, $${\displaystyle (x_{0},y_{0}),\ldots ,(x_{k},y_{n})=(x_{0},f(x_{0})),\ldots ,(x_{n},f(x_{n}))}$$ one sometimes writes the divided difference in the notation $${\displaystyle f[x_{k},\ldots ,x_{k+j}]\ {\stackrel {\text{def}{=}\ [f(x_{k}),\ldots ,f(x_{k+j})]=[y_{k},\ldots ,y_{k+j}].}$$Other notations for the divided difference of the function ƒ on the nodes x₀, ..., x_n are: $${\displaystyle f[x_{k},\ldots ,x_{k+j}]={\mathopen {[}x_{0},\ldots ,x_{n}]f={\mathopen {[}x_{0},\ldots ,x_{n};f]=D[x_{0},\ldots ,x_{n}]f.}$$

Divided differences for ${\displaystyle k=0}$ and the first few values of ${\displaystyle j}$: $${\displaystyle {\begin{aligned}{\mathopen {[}y_{0}]&=y_{0}\\{\mathopen {[}y_{0},y_{1}]&={\frac {y_{1}-y_{0}{x_{1}-x_{0}\\{\mathopen {[}y_{0},y_{1},y_{2}]&={\frac {\mathopen {[}y_{1},y_{2}]-{\mathopen {[}y_{0},y_{1}]}{x_{2}-x_{0}={\frac {\frac {y_{2}-y_{1}{x_{2}-x_{1}-{\frac {y_{1}-y_{0}{x_{1}-x_{0}{x_{2}-x_{0}={\frac {y_{2}-y_{1}{(x_{2}-x_{1})(x_{2}-x_{0})}-{\frac {y_{1}-y_{0}{(x_{1}-x_{0})(x_{2}-x_{0})}\\{\mathopen {[}y_{0},y_{1},y_{2},y_{3}]&={\frac {\mathopen {[}y_{1},y_{2},y_{3}]-{\mathopen {[}y_{0},y_{1},y_{2}]}{x_{3}-x_{0}\end{aligned}$$

Thus, the table corresponding to these terms upto two columns has the following form: $${\displaystyle {\begin{matrix}x_{0}&y_{0}&&\\&&{y_{1}-y_{0} \over x_{1}-x_{0}&\\x_{1}&y_{1}&&{y_{2}-y_{1} \over x_{2}-x_{1}-{y_{1}-y_{0} \over x_{1}-x_{0} \over x_{2}-x_{0}\\&&{y_{2}-y_{1} \over x_{2}-x_{1}&\\x_{2}&y_{2}&&\vdots \\&&\vdots &\\\vdots &&&\vdots \\&&\vdots &\\x_{n}&y_{n}&&\\\end{matrix}$$

• Linearity $${\displaystyle {\begin{aligned}(f+g)[x_{0},\dots ,x_{n}]&=f[x_{0},\dots ,x_{n}]+g[x_{0},\dots ,x_{n}]\\(\lambda \cdot f)[x_{0},\dots ,x_{n}]&=\lambda \cdot f[x_{0},\dots ,x_{n}]\end{aligned}$$
• Leibniz rule $${\displaystyle (f\cdot g)[x_{0},\dots ,x_{n}]=f[x_{0}]\cdot g[x_{0},\dots ,x_{n}]+f[x_{0},x_{1}]\cdot g[x_{1},\dots ,x_{n}]+\dots +f[x_{0},\dots ,x_{n}]\cdot g[x_{n}]=\sum _{r=0}^{n}f[x_{0},\ldots ,x_{r}]\cdot g[x_{r},\ldots ,x_{n}]}$$
• Divided differences are symmetric: If ${\displaystyle \sigma :\{0,\dots ,n\}\to \{0,\dots ,n\}$ is a permutation then $${\displaystyle f[x_{0},\dots ,x_{n}]=f[x_{\sigma (0)},\dots ,x_{\sigma (n)}]}$$
• Polynomial interpolation in the Newton form: if ${\displaystyle P}$ is a polynomial function of degree ${\displaystyle \leq n}$, and ${\displaystyle p[x_{0},\dots ,x_{n}]}$ is the divided difference, then $${\displaystyle P_{n-1}(x)=p[x_{0}]+p[x_{0},x_{1}](x-x_{0})+p[x_{0},x_{1},x_{2}](x-x_{0})(x-x_{1})+\cdots +p[x_{0},\ldots ,x_{n}](x-x_{0})(x-x_{1})\cdots (x-x_{n-1})}$$
• If ${\displaystyle p}$ is a polynomial function of degree ${\displaystyle <n}$, then $${\displaystyle p[x_{0},\dots ,x_{n}]=0.}$$
• Mean value theorem for divided differences: if ${\displaystyle f}$ is n times differentiable, then $${\displaystyle f[x_{0},\dots ,x_{n}]={\frac {f^{(n)}(\xi )}{n!}$$ for a number ${\displaystyle \xi }$ in the open interval determined by the smallest and largest of the ${\displaystyle x_{k}$'s.

The divided difference scheme can be put into an upper triangular matrix: $${\displaystyle T_{f}(x_{0},\dots ,x_{n})={\begin{pmatrix}f[x_{0}]&f[x_{0},x_{1}]&f[x_{0},x_{1},x_{2}]&\ldots &f[x_{0},\dots ,x_{n}]\\0&f[x_{1}]&f[x_{1},x_{2}]&\ldots &f[x_{1},\dots ,x_{n}]\\0&0&f[x_{2}]&\ldots &f[x_{2},\dots ,x_{n}]\\\vdots &\vdots &&\ddots &\vdots \\0&0&0&\ldots &f[x_{n}]\end{pmatrix}.}$$

Then it holds

• ${\displaystyle T_{f+g}(x)=T_{f}(x)+T_{g}(x)}$
• ${\displaystyle T_{\lambda f}(x)=\lambda T_{f}(x)}$ if ${\displaystyle \lambda }$ is a scalar
• ${\displaystyle T_{f\cdot g}(x)=T_{f}(x)\cdot T_{g}(x)}$
  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 ${\displaystyle T_{f}(x)}$ is a triangular matrix, its eigenvalues are obviously ${\displaystyle f(x_{0}),\dots ,f(x_{n})}$.
• Let ${\displaystyle \delta _{\xi }$ be a Kronecker delta-like function, that is $${\displaystyle \delta _{\xi }(t)={\begin{cases}1&:t=\xi ,\\0&:{\mbox{else}.\end{cases}$$ Obviously ${\displaystyle f\cdot \delta _{\xi }=f(\xi )\cdot \delta _{\xi }$, thus ${\displaystyle \delta _{\xi }$ is an eigenfunction of the pointwise function multiplication. That is ${\displaystyle T_{\delta _{x_{i}(x)}$ is somehow an "eigenmatrix" of ${\displaystyle T_{f}(x)}$: ${\displaystyle T_{f}(x)\cdot T_{\delta _{x_{i}(x)=f(x_{i})\cdot T_{\delta _{x_{i}(x)}$. However, all columns of ${\displaystyle T_{\delta _{x_{i}(x)}$ are multiples of each other, the matrix rank of ${\displaystyle T_{\delta _{x_{i}(x)}$ is 1. So you can compose the matrix of all eigenvectors of ${\displaystyle T_{f}(x)}$ from the ${\displaystyle i}$-th column of each ${\displaystyle T_{\delta _{x_{i}(x)}$. Denote the matrix of eigenvectors with ${\displaystyle U(x)}$. Example $${\displaystyle U(x_{0},x_{1},x_{2},x_{3})={\begin{pmatrix}1&{\frac {1}{(x_{1}-x_{0})}&{\frac {1}{(x_{2}-x_{0})(x_{2}-x_{1})}&{\frac {1}{(x_{3}-x_{0})(x_{3}-x_{1})(x_{3}-x_{2})}\\0&1&{\frac {1}{(x_{2}-x_{1})}&{\frac {1}{(x_{3}-x_{1})(x_{3}-x_{2})}\\0&0&1&{\frac {1}{(x_{3}-x_{2})}\\0&0&0&1\end{pmatrix}$$ The diagonalization of ${\displaystyle T_{f}(x)}$ can be written as $${\displaystyle U(x)\cdot \operatorname {diag} (f(x_{0}),\dots ,f(x_{n}))=T_{f}(x)\cdot U(x).}$$

The matrix $${\displaystyle J={\begin{pmatrix}x_{0}&1&0&0&\cdots &0\\0&x_{1}&1&0&\cdots &0\\0&0&x_{2}&1&&0\\\vdots &\vdots &&\ddots &\ddots &\\0&0&0&0&\;\ddots &1\\0&0&0&0&&x_{n}\end{pmatrix}$$ contains the divided difference scheme for the identity function with respect to the nodes ${\displaystyle x_{0},\dots ,x_{n}$, thus ${\displaystyle J^{m}$ contains the divided differences for the power function with exponent ${\displaystyle m}$. Consequently, you can obtain the divided differences for a polynomial function ${\displaystyle p}$ by applying ${\displaystyle p}$ to the matrix ${\displaystyle J}$: If $${\displaystyle p(\xi )=a_{0}+a_{1}\cdot \xi +\dots +a_{m}\cdot \xi ^{m}$$ and $${\displaystyle p(J)=a_{0}+a_{1}\cdot J+\dots +a_{m}\cdot J^{m}$$ then $${\displaystyle T_{p}(x)=p(J).}$$ This is known as Opitz' formula.^[2][3]

Now consider increasing the degree of ${\displaystyle p}$ to infinity, i.e. turn the Taylor polynomial into a Taylor series. Let ${\displaystyle f}$ be a function which corresponds to a power series. You can compute the divided difference scheme for ${\displaystyle f}$ by applying the corresponding matrix series to ${\displaystyle J}$: If $${\displaystyle f(\xi )=\sum _{k=0}^{\infty }a_{k}\xi ^{k}$$ and $${\displaystyle f(J)=\sum _{k=0}^{\infty }a_{k}J^{k}$$ then $${\displaystyle T_{f}(x)=f(J).}$$

$${\displaystyle {\begin{aligned}f[x_{0}]&=f(x_{0})\\f[x_{0},x_{1}]&={\frac {f(x_{0})}{(x_{0}-x_{1})}+{\frac {f(x_{1})}{(x_{1}-x_{0})}\\f[x_{0},x_{1},x_{2}]&={\frac {f(x_{0})}{(x_{0}-x_{1})\cdot (x_{0}-x_{2})}+{\frac {f(x_{1})}{(x_{1}-x_{0})\cdot (x_{1}-x_{2})}+{\frac {f(x_{2})}{(x_{2}-x_{0})\cdot (x_{2}-x_{1})}\\f[x_{0},x_{1},x_{2},x_{3}]&={\frac {f(x_{0})}{(x_{0}-x_{1})\cdot (x_{0}-x_{2})\cdot (x_{0}-x_{3})}+{\frac {f(x_{1})}{(x_{1}-x_{0})\cdot (x_{1}-x_{2})\cdot (x_{1}-x_{3})}+\\&\quad \quad {\frac {f(x_{2})}{(x_{2}-x_{0})\cdot (x_{2}-x_{1})\cdot (x_{2}-x_{3})}+{\frac {f(x_{3})}{(x_{3}-x_{0})\cdot (x_{3}-x_{1})\cdot (x_{3}-x_{2})}\\f[x_{0},\dots ,x_{n}]&=\sum _{j=0}^{n}{\frac {f(x_{j})}{\prod _{k\in \{0,\dots ,n\}\setminus \{j\}(x_{j}-x_{k})}\end{aligned}$$

With the help of the polynomial function ${\displaystyle \omega (\xi )=(\xi -x_{0})\cdots (\xi -x_{n})}$ this can be written as $${\displaystyle f[x_{0},\dots ,x_{n}]=\sum _{j=0}^{n}{\frac {f(x_{j})}{\omega '(x_{j})}.}$$

If ${\displaystyle x_{0}<x_{1}<\cdots <x_{n}$ and ${\displaystyle n\geq 1}$, the divided differences can be expressed as^[4] $${\displaystyle f[x_{0},\ldots ,x_{n}]={\frac {1}{(n-1)!}\int _{x_{0}^{x_{n}f^{(n)}(t)\;B_{n-1}(t)\,dt}$$ where ${\displaystyle f^{(n)}$ is the ${\displaystyle n}$-th derivative of the function ${\displaystyle f}$ and ${\displaystyle B_{n-1}$ is a certain B-spline of degree ${\displaystyle n-1}$ for the data points ${\displaystyle x_{0},\dots ,x_{n}$, given by the formula $${\displaystyle B_{n-1}(t)=\sum _{k=0}^{n}{\frac {(\max(0,x_{k}-t))^{n-1}{\omega '(x_{k})}$$

This is a consequence of the Peano kernel theorem; it is called the Peano form of the divided differences and ${\displaystyle B_{n-1}$ is the Peano kernel for the divided differences, all named after Giuseppe Peano.

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 $${\displaystyle (x_{0},y_{0}),\ldots ,(x_{n},y_{n})}$$ with $${\displaystyle x_{k}=x_{0}+kh,\ {\text{ for }\ k=0,\ldots ,n{\text{ and fixed }h>0}$$ the forward differences are defined as $${\displaystyle {\begin{aligned}\Delta ^{(0)}y_{k}&:=y_{k},\qquad k=0,\ldots ,n\\\Delta ^{(j)}y_{k}&:=\Delta ^{(j-1)}y_{k+1}-\Delta ^{(j-1)}y_{k},\qquad k=0,\ldots ,n-j,\ j=1,\dots ,n.\end{aligned}$$whereas the backward differences are defined as: $${\displaystyle {\begin{aligned}\nabla ^{(0)}y_{k}&:=y_{k},\qquad k=0,\ldots ,n\\\nabla ^{(j)}y_{k}&:=\nabla ^{(j-1)}y_{k}-\nabla ^{(j-1)}y_{k-1},\qquad k=0,\ldots ,n-j,\ j=1,\dots ,n.\end{aligned}$$ Thus the forward difference table is written as:$${\displaystyle {\begin{matrix}y_{0}&&&\\&\Delta y_{0}&&\\y_{1}&&\Delta ^{2}y_{0}&\\&\Delta y_{1}&&\Delta ^{3}y_{0}\\y_{2}&&\Delta ^{2}y_{1}&\\&\Delta y_{2}&&\\y_{3}&&&\\\end{matrix}$$whereas the backwards difference table is written as:$${\displaystyle {\begin{matrix}y_{0}&&&\\&\nabla y_{1}&&\\y_{1}&&\nabla ^{2}y_{2}&\\&\nabla y_{2}&&\nabla ^{3}y_{3}\\y_{2}&&\nabla ^{2}y_{3}&\\&\nabla y_{3}&&\\y_{3}&&&\\\end{matrix}$$

The relationship between divided differences and forward differences is^[5] $${\displaystyle [y_{j},y_{j+1},\ldots ,y_{j+k}]={\frac {1}{k!h^{k}\Delta ^{(k)}y_{j},}$$whereas for backward differences:^{[citation needed]}$${\displaystyle [{y}_{j},y_{j-1},\ldots ,{y}_{j-k}]={\frac {1}{k!h^{k}\nabla ^{(k)}y_{j}.}$$

• Difference quotient
• Neville's algorithm
• Polynomial interpolation
• Mean value theorem for divided differences
• Nörlund–Rice integral
• Pascal's triangle

• Louis Melville Milne-Thomson (2000) [1933]. The Calculus of Finite Differences. American Mathematical Soc. Chapter 1: Divided Differences. ISBN 978-0-8218-2107-7.
• Myron B. Allen; Eli L. Isaacson (1998). Numerical Analysis for Applied Science. John Wiley & Sons. Appendix A. ISBN 978-1-118-03027-1.
• 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. ISBN 978-0-08-051547-2.

• An implementation in Haskell.