- Key People:
- Sir Edmund Taylor Whittaker
special function
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What is a special function in mathematics?
In mathematics, a special function refers to any member of a class of mathematical functions that arise in the solutions of diverse classical physics problems. These problems often involve the flow of thermal, acoustic, or electromagnetic energy. Examples of special functions include Bessel functions, spherical harmonics, Hermite polynomials, and many others.
These functions appear when using the separation of variables method to reduce partial differential equations to ordinary differential equations. The solutions to these ordinary differential equations form the majority of the special functions of mathematical physics.
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Why do mathematicians study special functions?
Mathematicians study special functions because these functions frequently appear when solving classical physics problems involving energy flow. Although these physical problems may seem limited, different mathematical representations are needed based on the physical system's configuration.
These functions, including Bessel functions, hypergeometric functions, Legendre polynomials, and others, arise from solving partial differential equations that describe phenomena like heat flow and wave propagation. While these functions have historical and practical applications in mathematical physics, they also have uses in both pure and applied mathematics, such as number theory and random-walk problems.
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Can you name some common examples of special functions?
Special functions are a class of mathematical functions that arise in the solutions of many classical physics problems, especially those involving electromagnetic, acoustic, or thermal energy flow.
Examples of special functions:
* Bessel functions are solutions to Besselβs differential equation and appear in problems involving cylindrical coordinates.
* Gamma functions generalize the factorial function to nonintegral values and have applications in calculus, differential equations, complex analysis, and statistics.
* Legendre polynomials are special cases of spherical harmonics.
* Other special functions include Chebyshev polynomials, Hermite polynomials, Jacobi polynomials, Laguerre polynomials, Whittaker functions, parabolic cylinder functions, elliptic functions, and hypergeometric functions.5 Britannica SourcesCreated from Britannica articles using AI. AI can make mistakes, so verify using Britannica articles. -
How are special functions different from basic functions like addition or multiplication?
Special functions, unlike basic functions such as addition or multiplication, typically arise in solving complex physics problems related to energy flow. These problems, while seemingly limited, require different mathematical representations based on the physical system's configuration.
The solutions of ordinary differential equations form the majority of the special functions of mathematical physics. Examples include Bessel functions, Legendre polynomials, Chebyshev polynomials, and hypergeometric functions. Each of these functions possesses unique properties that warrant separate study, though attempts have been made to unify them.
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In what kinds of problems or equations do special functions often appear?
Special functions commonly appear when solving various classical physics problems involving electromagnetic, acoustic, or thermal energy flow. These problems often require different mathematical representations based on the physical system's configuration.
These functions arise from solving partial differential equations, which describe the behavior of these systems. Using techniques like separation of variables on these partial differential equations leads to ordinary differential equations. The solutions to these ordinary differential equations are the special functions of mathematical physics. Examples include Bessel functions (appearing in heat flow or wave propagation problems in cylindrical coordinates), Legendre polynomials and hypergeometric functions.
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How do special functions help scientists and engineers solve real-world problems?
Special functions are a class of mathematical functions that arise in solving classical physics problems involving electromagnetic, acoustic, or thermal energy flow. While these problems may seem limited, different representations are needed based on the physical system's configuration, leading to different mathematical equations.
These equations are partial differential equations that can be reduced to ordinary differential equations through separation of variables. The solutions form the majority of special functions in mathematical physics. For example, solving heat flow or wave propagation equations in cylindrical coordinates leads to Bessel's differential equation, whose solution is the Bessel function. Bessel functions appear in mathematical descriptions of numerous physical phenomena, including heat or electricity flow in a solid cylinder, electromagnetic wave propagation along wires, light diffraction, fluid motions, and elastic body deformations.
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special function, any of a class of mathematical functions that arise in the solution of various classical problems of physics. These problems generally involve the flow of electromagnetic, acoustic, or thermal energy. Different scientists might not completely agree on which functions are to be included among the special functions, although there would certainly be very substantial overlap.
At first glance, the physical problems mentioned above seem to be very limited in scope. From a mathematical point of view, however, different representations have to be sought, depending on the configuration of the physical system for which these problems are to be solved. For example, in studying propagation of heat in a metallic bar, one could consider a bar with a rectangular cross section, a round cross section, an elliptical cross section, or even more-complicated cross sections; the bar might be straight or curved. Every one of these situations, while dealing with the same type of physical problem, leads to somewhat different mathematical equations.
The equations to be solved are partial differential equations. To apprehend how these equations come about, one can consider a straight rod along which there is a uniform flow of heat. Let u(x, t) denote the temperature of the rod at time t and location x, and let q(x, t) denote the rate of heat flow. The expression βq/βx denotes the rate at which the rate of heat flow changes per unit length and therefore measures the rate at which heat is accumulating at a given point x at time t. If heat is accumulating, the temperature at that point is rising, and the rate is denoted by βu/βt. The principle of conservation of energy leads to βq/βx = k(βu/βt), where k is the specific heat of the rod. This means that the rate at which heat is accumulating at a point is proportional to the rate at which the temperature is increasing. A second relationship between q and u is obtained from Newtonβs law of cooling, which states that q = K(βu/βx). The latter is a mathematical way of asserting that the steeper the temperature gradient (the rate of change of temperature per unit length), the higher the rate of heat flow. Elimination of q between these equations leads to β2u/βx2 = (k/K)(βu/βt), the partial differential equation for one-dimensional heat flow.
The partial differential equation for heat flow in three dimensions takes the form β2u/βx2 + β2u/βy2 + β2u/βz2 = (k/K)(βu/βt); the latter equation is often written β2u = (k/K)(βu/βt), where the symbol β, called del or nabla, is known as the Laplace operator. β also enters the partial differential equation dealing with wave-propagation problems, which has the form β2u = (1/c2)(β2u/βt2), where c is the speed at which the wave propagates.
Partial differential equations are harder to solve than ordinary differential equations, but the partial differential equations associated with wave propagation and heat flow can be reduced to a system of ordinary differential equations through a process known as separation of variables. These ordinary differential equations depend on the choice of coordinate system, which in turn is influenced by the physical configuration of the problem. The solutions of these ordinary differential equations form the majority of the special functions of mathematical physics.
For example, in solving the equations of heat flow or wave propagation in cylindrical coordinates, the method of separation of variables leads to Besselβs differential equation, a solution of which is the Bessel function, denoted by Jn(x).
Among the many other special functions that satisfy second-order differential equations are the spherical harmonics (of which the Legendre polynomials are a special case), the Tchebychev polynomials, the Hermite polynomials, the Jacobi polynomials, the Laguerre polynomials, the Whittaker functions, and the parabolic cylinder functions. As with the Bessel functions, one can study their infinite series, recursion formulas, generating functions, asymptotic series, integral representations, and other properties. Attempts have been made to unify this rich topic, but not one has been completely successful. In spite of the many similarities among these functions, each has some unique properties that must be studied separately. But some relationships can be developed by introducing yet another special function, the hypergeometric function, which satisfies the differential equation z(1 β z) d2y/dx2 + [c β (a + b + 1)z] dy/dx β aby = 0. Some of the special functions can be expressed in terms of the hypergeometric function.
While it is true, both historically and practically, that the special functions and their applications arise primarily in mathematical physics, they do have many other uses in both pure and applied mathematics. Bessel functions are useful in solving certain types of random-walk problems. They also find application in the theory of numbers. The hypergeometric functions are useful in constructing so-called conformal mappings of polygonal regions whose sides are circular arcs.

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