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Numerical integration

In analysis, numerical integration comprises a broad family of algorithms for calculating the numerical value of a definite integral. The term numerical quadrature (often abbreviated to quadrature) is more or less a synonym for "numerical integration", especially as applied to one-dimensional integrals. Some authors refer to numerical integration over more than one dimension as cubature;[1] others take "quadrature" to include higher-dimensional integration.

The basic problem in numerical integration is to compute an approximate solution to a definite integral


to a given degree of accuracy. If f(x) is a smooth function integrated over a small number of dimensions, and the domain of integration is bounded, there are many methods for approximating the integral to the desired precision.


Numerical integration has roots in the geometrical problem of finding a square with the same area as a given plane figure (quadrature or squaring), as in the quadrature of the circle. The term is also sometimes used to describe the numerical solution of differential equations.

The area of the surface of a sphere is equal to quadruple the area of a of this sphere.

great circle

The area of a segment of the cut from it by a straight line is 4/3 the area of the triangle inscribed in this segment.

parabola

The term "numerical integration" first appears in 1915 in the publication A Course in Interpolation and Numeric Integration for the Mathematical Laboratory by David Gibb.[2]


"Quadrature" is a historical mathematical term that means calculating area. Quadrature problems have served as one of the main sources of mathematical analysis. Mathematicians of Ancient Greece, according to the Pythagorean doctrine, understood calculation of area as the process of constructing geometrically a square having the same area (squaring). That is why the process was named "quadrature". For example, a quadrature of the circle, Lune of Hippocrates, The Quadrature of the Parabola. This construction must be performed only by means of compass and straightedge.


The ancient Babylonians used the trapezoidal rule to integrate the motion of Jupiter along the ecliptic.[3]


For a quadrature of a rectangle with the sides a and b it is necessary to construct a square with the side (the Geometric mean of a and b). For this purpose it is possible to use the following fact: if we draw the circle with the sum of a and b as the diameter, then the height BH (from a point of their connection to crossing with a circle) equals their geometric mean. The similar geometrical construction solves a problem of a quadrature for a parallelogram and a triangle.


Problems of quadrature for curvilinear figures are much more difficult. The quadrature of the circle with compass and straightedge had been proved in the 19th century to be impossible. Nevertheless, for some figures (for example the Lune of Hippocrates) a quadrature can be performed. The quadratures of a sphere surface and a parabola segment done by Archimedes became the highest achievement of the antique analysis.


For the proof of the results Archimedes used the Method of exhaustion of Eudoxus.


In medieval Europe the quadrature meant calculation of area by any method. More often the Method of indivisibles was used; it was less rigorous, but more simple and powerful. With its help Galileo Galilei and Gilles de Roberval found the area of a cycloid arch, Grégoire de Saint-Vincent investigated the area under a hyperbola (Opus Geometricum, 1647), and Alphonse Antonio de Sarasa, de Saint-Vincent's pupil and commentator, noted the relation of this area to logarithms.


John Wallis algebrised this method: he wrote in his Arithmetica Infinitorum (1656) series that we now call the definite integral, and he calculated their values. Isaac Barrow and James Gregory made further progress: quadratures for some algebraic curves and spirals. Christiaan Huygens successfully performed a quadrature of some Solids of revolution.


The quadrature of the hyperbola by Saint-Vincent and de Sarasa provided a new function, the natural logarithm, of critical importance.


With the invention of integral calculus came a universal method for area calculation. In response, the term "quadrature" has become traditional, and instead the modern phrase "computation of a univariate definite integral" is more common.

Truncation error (numerical integration)

Clenshaw–Curtis quadrature

Gauss-Kronrod quadrature

or Riemann Integral

Riemann Sum

Trapezoidal rule

Romberg's method

Tanh-sinh quadrature

Nonelementary Integral

and Philip Rabinowitz, Methods of Numerical Integration.

Philip J. Davis

Michael A. Malcolm, and Cleve B. Moler, Computer Methods for Mathematical Computations. Englewood Cliffs, NJ: Prentice-Hall, 1977. (See Chapter 5.)

George E. Forsythe

; Teukolsky, S.A.; Vetterling, W.T.; Flannery, B.P. (2007), "Chapter 4. Integration of Functions", Numerical Recipes: The Art of Scientific Computing (3rd ed.), New York: Cambridge University Press, ISBN 978-0-521-88068-8

Press, W.H.

and Roland Bulirsch, Introduction to Numerical Analysis. New York: Springer-Verlag, 1980. (See Chapter 3.)

Josef Stoer

A History of Mathematics, 2nd ed. rev. by Uta C. Merzbach, New York: Wiley, 1989 ISBN 0-471-09763-2 (1991 pbk ed. ISBN 0-471-54397-7).

Boyer, C. B.

An Introduction to the History of Mathematics, Saunders, 1990, ISBN 0-03-029558-0,

Eves, Howard

at Holistic Numerical Methods Institute

Integration: Background, Simulations, etc.

from Wolfram Mathworld

Lobatto Quadrature

from Encyclopedia of Mathematics

Lobatto quadrature formula

within the free Tracker Component Library.

Implementations of many quadrature and cubature formulae

SageMath Online Integrator