In the physical sciences, the Airy function (or Airy function of the first kind) is a special function named after the British astronomer George Biddell Airy (1801–1892). The function and the related function, are linearly independent solutions to the differential equationknown as the Airy equation or the Stokes equation.
Because the solution of the linear differential equationis oscillatory for and exponential for, the Airy functions are oscillatory for and exponential for . In fact, the Airy equation is the simplest second-order linear differential equation with a turning point (a point where the character of the solutions changes from oscillatory to exponential).
For real values of, the Airy function of the first kind can be defined by the improper Riemann integral:which converges by Dirichlet's test. For any real number there is a positive real number such that function is increasing, unbounded and convex with continuous and unbounded derivative on interval
[M,infty).
satisfies the Airy equationThis equation has two linearly independent solutions.Up to scalar multiplication, is the solution subject to the condition as .The standard choice for the other solution is the Airy function of the second kind, denoted Bi(x). It is defined as the solution with the same amplitude of oscillation as as which differs in phase by :
The values of and and their derivatives at are given byHere, denotes the Gamma function. It follows that the Wronskian of and is .
When is positive, is positive, convex, and decreasing exponentially to zero, while is positive, convex, and increasing exponentially. When is negative, and oscillate around zero with ever-increasing frequency and ever-decreasing amplitude. This is supported by the asymptotic formulae below for the Airy functions.
The Airy functions are orthogonal[1] in the sense thatagain using an improper Riemann integral.
As explained below, the Airy functions can be extended to the complex plane, giving entire functions. The asymptotic behaviour of the Airy functions as goes to infinity at a constant value of depends on : this is called the Stokes phenomenon. For we have the following asymptotic formula for :[3]
orwhere
\zeta=\tfrac23z3/2.
A more accurate formula for and a formula for when or, equivalently, for and when but not zero, are:[5]
&-\frac \cos\left(\fracz^+\frac \right) \left[\sum_{n=0}^{\infty} \dfrac{(-1)^n \, \Gamma\!\left(2n + \frac{11}{6}\right) \, \Gamma\!\left(2n + \frac{7}{6}\right) \left(\frac{3}{4}\right)^{2n+1}}{2\pi \, (2n+1)! \, z^{3n\,+\,3/2}} \right] \\[6pt] \operatorname(-z) \sim& \frac \cos \left(\fracz^ + \frac \right) \left[\sum_{n=0}^{\infty} \dfrac{(-1)^n \, \Gamma\!\left(2n + \frac{5}{6}\right) \, \Gamma\!\left(2n + \frac{1}{6}\right) \left(\frac{3}{4}\right)^{2n}}{2\pi \, (2n)! \, z^{3n}} \right] \\[6pt] &+ \frac \sin\left(\fracz^ + \frac \right) \left[\sum_{n=0}^{\infty} \dfrac{(-1)^n \, \Gamma\!\left(2n + \frac{11}{6}\right) \, \Gamma\!\left(2n + \frac{7}{6}\right) \left(\frac{3}{4}\right)^{2n+1}}{2\pi \, (2n+1)! \, z^{3n\,+\,3/2}} \right].\end
When these are good approximations but are not asymptotic because the ratio between or and the above approximation goes to infinity whenever the sine or cosine goes to zero.Asymptotic expansions for these limits are also available. These are listed in (Abramowitz and Stegun, 1983) and (Olver, 1974).
One is also able to obtain asymptotic expressions for the derivatives and . Similarly to before, when :
When we have:
Similarly, an expression for and when but not zero, are
&-\frac \sin\left(\fracz^ + \frac \right) \left[\sum_{n=0}^{\infty} \frac{7+12n}{-5-12n} \dfrac{(-1)^n \, \Gamma\!\left(2n + \frac{11}{6}\right) \, \Gamma\!\left(2n + \frac{7}{6}\right) \left(\frac{3}{4}\right)^{2n+1}}{2\pi \, (2n+1)! \, z^{3n\,+\,3/2}} \right] \\[6pt] \operatorname'(-z) \sim& \ \frac \sin\left(\fracz^ + \frac \right) \left[\sum_{n=0}^{\infty} \frac{1+12n}{1-12n} \dfrac{(-1)^n \, \Gamma\!\left(2n + \frac{5}{6}\right) \, \Gamma\!\left(2n + \frac{1}{6}\right) \left(\frac{3}{4}\right)^{2n}}{2\pi \, (2n)! \, z^{3n}} \right] \\[6pt] &-\frac \cos\left(\fracz^ + \frac \right) \left[\sum_{n=0}^{\infty} \frac{7+12n}{-5-12n} \dfrac{(-1)^n \, \Gamma\!\left(2n + \frac{11}{6}\right) \, \Gamma\!\left(2n + \frac{7}{6}\right) \left(\frac{3}{4}\right)^{2n+1}}{2\pi \, (2n+1)! \, z^{3n\,+\,3/2}} \right] \\\end
We can extend the definition of the Airy function to the complex plane bywhere the integral is over a path C starting at the point at infinity with argument and ending at the point at infinity with argument π/3. Alternatively, we can use the differential equation to extend and to entire functions on the complex plane.
The asymptotic formula for is still valid in the complex plane if the principal value of is taken and is bounded away from the negative real axis. The formula for is valid provided is in the sector
x\in\C:\left|\arg(x)\right|<\tfrac{\pi}{3}-\delta
x\in\C:\left|\arg(x)\right|<\tfrac{2\pi}{3}-\delta.
It follows from the asymptotic behaviour of the Airy functions that both and have an infinity of zeros on the negative real axis. The function has no other zeros in the complex plane, while the function also has infinitely many zeros in the sector
z\in\C:\tfrac{\pi}{3}<\left|\arg(z)\right|<\tfrac{\pi}{2}.
For positive arguments, the Airy functions are related to the modified Bessel functions:Here, and are solutions of
The first derivative of the Airy function is
Functions and can be represented in terms of rapidly convergent integrals[6] (see also modified Bessel functions)
For negative arguments, the Airy function are related to the Bessel functions:Here, are solutions of
The Scorer's functions and solve the equation . They can also be expressed in terms of the Airy functions:
Using the definition of the Airy function Ai(x), it is straightforward to show its Fourier transform is given byThis can be obtained by taking the Fourier transform of the Airy equation. Let , then
i\haty'+k2\haty=0
\haty=C
ik3/3 | |
e |
.
The Airy function is the solution to the time-independent Schrödinger equation for a particle confined within a triangular potential well and for a particle in a one-dimensional constant force field. For the same reason, it also serves to provide uniform semiclassical approximations near a turning point in the WKB approximation, when the potential may be locally approximated by a linear function of position. The triangular potential well solution is directly relevant for the understanding of electrons trapped in semiconductor heterojunctions.
A transversally asymmetric optical beam, where the electric field profile is given by the Airy function, has the interesting property that its maximum intensity accelerates towards one side instead of propagating in a straight line as is the case in symmetric beams. This is at expense of the low-intensity tail being spread in the opposite direction, so the overall momentum of the beam is of course conserved.
The Airy function underlies the form of the intensity near an optical directional caustic, such as that of the rainbow (called supernumerary rainbow). Historically, this was the mathematical problem that led Airy to develop this special function. In 1841, William Hallowes Miller experimentally measured the analog to supernumerary rainbow by shining light through a thin cylinder of water, then observing through a telescope. He observed up to 30 bands.[7]
In the mid-1980s, the Airy function was found to be intimately connected to Chernoff's distribution.[8]
The Airy function also appears in the definition of Tracy–Widom distribution which describes the law of largest eigenvalues in Random matrix. Due to the intimate connection of random matrix theory with the Kardar–Parisi–Zhang equation, there are central processes constructed in KPZ such as the Airy process. [9]
The Airy function is named after the British astronomer and physicist George Biddell Airy (1801–1892), who encountered it in his early study of optics in physics (Airy 1838). The notation Ai(x) was introduced by Harold Jeffreys. Airy had become the British Astronomer Royal in 1835, and he held that post until his retirement in 1881.