In mathematical analysis, the Dirac delta function (or δ {\displaystyle {\boldsymbol {\delta }}} distribution), also known as the unit impulse, is a generalized function on the real numbers, whose value is zero everywhere except at zero, where it is infinite, and whose integral over the entire real line is equal to one. Thus it can be represented heuristically as δ ( x ) = { 0 , x ≠ 0 ∞ , x = 0 {\displaystyle \delta (x)={\begin{cases}0,&x\neq 0\\{\infty },&x=0\end{cases}}} such that ∫ − ∞ ∞ δ ( x ) d x = 1. {\displaystyle \int _{-\infty }^{\infty }\delta (x)\,dx=1.}
Since no function has this property, modelling the delta "function" rigorously involves the use of limits or, as is common in mathematics, measure theory and the theory of distributions. The delta function is named after physicist Paul Dirac, and has been applied routinely in physics and engineering to model point masses and concentrated loads. It is called the delta function because it is a continuous analogue of the Kronecker delta function. The mathematical rigor of the delta function was disputed until Laurent Schwartz developed the theory of distributions, where it is defined as a linear form acting on functions.
Motivation and overview The graph of the Dirac delta is usually thought of as following the whole x {\displaystyle x} -axis and the positive y {\displaystyle y} -axis. The Dirac delta is used to model a tall narrow spike function (an impulse), and other similar abstractions such as a point charge or point mass. For example, to calculate the dynamics of a billiard ball being struck, one can approximate the force of the impact by a Dirac delta. In doing so, one can simplify the equations and calculate the motion of the ball by only considering the total impulse of the collision. In applied mathematics, the delta function is often manipulated as a kind of limit (a weak limit) of a sequence of functions, each member of which has a tall spike at the origin: for example, a sequence of Gaussian distributions centered at the origin with variance tending to zero. (However, even in some applications, highly oscillatory functions are used as approximations to the delta function, see below.) The Dirac delta, given the desired properties outlined above, cannot be a function with domain and range in real numbers. For example, the objects f ( x ) = δ ( x ) {\displaystyle f(x)=\delta (x)} and g ( x ) = 0 {\displaystyle g(x)=0} are equal everywhere except at x = 0 {\displaystyle x=0} yet have integrals that are different. According to Lebesgue integration theory, if f {\displaystyle f} and g {\displaystyle g} are functions such that f = g {\displaystyle f=g} almost everywhere, then f {\displaystyle f} is integrable if and only if g {\displaystyle g} is integrable and the integrals of f {\displaystyle f} and g {\displaystyle g} are identical. A rigorous approach to regarding the Dirac delta function as a mathematical object in its own right uses measure theory or the theory of distributions.
History As part of his development of quantum mechanics, Paul Dirac introduced the δ {\displaystyle \delta } -function in a 1927 paper, subsequently popularized in his 1930 book The Principles of Quantum Mechanics. He called it the "delta function" since he used it as a continuum analog of the discrete Kronecker delta. However, it had been used by multiple mathematical scientists in the nineteenth century. Dirac biographer Graham Farmelo surmised that Oliver Heaviside was likely a direct influence on Dirac, given Dirac's background in engineering. Indeed, Heaviside introduced the δ {\displaystyle \delta } -function in his work on electromagnetism and electrical engineering. In a 1963 interview, Dirac stated, "All electrical engineers are familiar with the idea of a pulse, and the δ {\displaystyle \delta } -function is just a way of expressing a pulse mathematically." Mathematicians refer to the same concept as a generalized function or distribution rather than a function in the ordinary sense. The earliest known use of the δ {\displaystyle \delta } -function is in the works of Jean-Baptiste Joseph Fourier. Fourier presented what is now called the Fourier integral theorem in his treatise Théorie analytique de la chaleur (1822) in the form:
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