A 'finite difference' is a mathematical expression of the form ''f''(''x'' + ''b'') − ''f''(''x'' + ''a''). If a finite difference is divided by ''b'' − ''a'', one gets a
difference quotient. The approximation of derivatives by finite differences plays a central role in
finite difference methods for the
numerical solution of
differential equations, especially
boundary value problems.
In
mathematical analysis operators involving finite differences are studied. A
difference operator is an operator which maps a function ''f'' to a function whose values are the corresponding finite differences.
Forward, backward and central differences
Only three forms are commonly considered: forward, backward and central differences.
A 'forward difference' is an expression of the form
:
Depending on the application, the spacing ''h'' is may be variable or held constant.
A 'backward difference' uses the function values at ''x'' and ''x'' − ''h'', instead of the values at ''x'' + ''h'' and ''x'':
:
Finally, the 'central difference' is given by
:
Relation with derivatives
The
derivative of a function ''f'' at a point ''x'' is defined by the
limit
:
If ''h'' has a fixed (non-zero) value, instead of approaching zero, then the right-hand side is
:
Hence, the forward difference divided by ''h'' approximates the derivative when ''h'' is small. The error in this approximation can be derived from
Taylor's theorem. Assuming that ''f'' is continuously differentiable, the error is
:
The same formula holds for the backward difference:
:
However, the central difference yields a more accurate approximation. Its error is proportional to square of the spacing (if ''f'' is twice continuously differentiable):
:
Higher-order differences
In an analogous way one can obtain finite difference approximations to higher order derivatives and differential operators. For example, by using the above central difference formula for
and
and applying a central difference formula for the derivative of
at ''x'', we obtain the central difference approximation of the second derivative of ''f'':
:
More generally, the ''n''
th-order forward, backward, and central differences are respectively given by:
:
:
:
Note that the central difference will, for odd
, have
multiplied by non-integers. If this is a problem (usually it is), it may be remedied taking the average of
and
.
The relationship of these higher-order differences with the respective derivatives is very straightforward:
:
Higher-order differences can also be used to construct better approximations. As mentioned above, the first-order difference approximates the first-order derivative up to a term of order ''h''. However, the combination
:
approximates ''f'(''x'') up to a term of order ''h''
2. This can be proven by expanding the above expression in
Taylor series, or by using the calculus of finite differences, explained below.
If necessary, the finite difference can be centered about any point by mixing forward, backward, and central differences.
Finite difference methods
Main articles: finite difference method
An important application of finite differences is in
numerical analysis, especially in
numerical ordinary differential equations and
numerical partial differential equations, which aim at the numerical solution of
ordinary and
partial differential equations respectively. The idea is to replace the derivatives appearing in the differential equation by finite differences that approximate them. The resulting methods are called ''finite difference methods''.
Common applications of the finite difference method are in computational science and engineering disciplines, such as thermal engineering, fluid mechanics, etc.
Calculus of finite differences
Main articles: difference operator
The forward difference can be considered as a difference operator, which maps the function ''f'' to Δ
''h''[''f'']. This operator satisfies
:
where
is the
shift operator with step
, defined by
, and
is an
identity operator. The difference operator Δ
''h'' is
linear and satisfies
Leibniz rule. Similar statements hold for the backward and central difference.
Taylor's theorem can now be expressed by the formula
:
where ''D'' denotes the derivative operator, mapping ''f'' to its derivative ''f'. Formally inverting the exponential suggests that
:
This formula holds in the sense that both operators give the same result when applied to a polynomial. Even for analytic functions, the series on the right is not guaranteed to converge; it may be an
asymptotic series. However, it can be used to obtain more accurate approximations for the derivative. For instance, retaining the first two terms of the series yields the second-order approximation to
mentioned at the end of the
section ''Higher-order differences''.
The analogous formulas for the backward and central difference operators are
:
Generalizations
A 'generalized finite difference' is usually defined as
:
where
is its coefficients vector. An 'infinite difference' is a further generalization, where the finite sum above is replaced by an
infinite series.
See also
★
Numerical differentiation
★
Five-point stencil
★
Divided differences
★
Faulhaber's formula
References
★ William F. Ames, ''Numerical Method for Partial Differential Equations'', Section 1.6. Academic Press, New York, 1977. ISBN 0-12-056760-1.
★ Francis B. Hildebrand, ''Finite-Difference Equations and Simulations'', Section 2.2. Prentice-Hall, Englewood Cliffs, New Jersey, 1968.
★ Boole, George, ''A Treatise On The Calculus of Finite Differences'', 2nd Ed., Macmillan and Company, 1872. [See also: Dover edition 1960].
★ Freeman, Harry, ''Finite Differences for Actuarial Students''. 1967.
External links
★
Finite Difference Method
★
Finite Difference Method for Boundary Value Problems
★
Table of useful finite difference formula generated using Mathematica