Hill differential equation explained

In mathematics, the Hill equation or Hill differential equation is the second-order linear ordinary differential equation

d2y
dt2

+f(t)y=0,

where

f(t)

is a periodic function with minimal period

\pi

and average zero. By these we mean that for all

t

f(t+\pi)=f(t),

and

\pi
\int
0

f(t)dt=0,

and if

p

is a number with

0<p<\pi

, the equation

f(t+p)=f(t)

must fail for some

t

.[1] It is named after George William Hill, who introduced it in 1886.[2]

Because

f(t)

has period

\pi

, the Hill equation can be rewritten using the Fourier series of

f(t)

:
d2y
dt2

+\left(\theta0+2\sum

infty
n=1

\thetan

infty
\cos(2nt)+\sum
m=1

\phim\sin(2mt)\right)y=0.

Important special cases of Hill's equation include the Mathieu equation (in which only the terms corresponding to n = 0, 1 are included) and the Meissner equation.

Hill's equation is an important example in the understanding of periodic differential equations. Depending on the exact shape of

f(t)

, solutions may stay bounded for all time, or the amplitude of the oscillations in solutions may grow exponentially.[3] The precise form of the solutions to Hill's equation is described by Floquet theory. Solutions can also be written in terms of Hill determinants.[1]

Aside from its original application to lunar stability,[2] the Hill equation appears in many settings including in modeling of a quadrupole mass spectrometer,[4] as the one-dimensional Schrödinger equation of an electron in a crystal,[5] quantum optics of two-level systems, accelerator physics and electromagnetic structures that are periodic in space[6] and/or in time.[7]

Notes and References

  1. Book: Magnus. W.. Winkler. S.. Hill's equation. 2013. Courier. 9780486150291.
  2. 10.1007/BF02417081. George William Hill. G.W.. Hill. On the Part of the Motion of Lunar Perigee Which is a Function of the Mean Motions of the Sun and Moon. Acta Math.. 8. 1. 1–36. 1886. free.
  3. Book: Teschl . Gerald Teschl

    . Gerald . Gerald Teschl . Ordinary Differential Equations and Dynamical Systems . . . 2012 . 978-0-8218-8328-0 .

  4. Sheretov . Ernst P. . Opportunities for optimization of the rf signal applied to electrodes of quadrupole mass spectrometers.: Part I. General theory . . April 2000 . 198 . 1-2 . 83–96 . 10.1016/S1387-3806(00)00165-2.
  5. Casperson . Lee W. . Lee Casperson . Solvable Hill equation . . November 1984 . 30 . 2749 . 10.1103/PhysRevA.30.2749.
  6. [Léon Brillouin|Brillouin, L.]
  7. Koutserimpas . Theodoros T. . Fleury . Romain . Electromagnetic Waves in a Time Periodic Medium With Step-Varying Refractive Index . . October 2018 . 66 . 10 . 5300–5307 . 10.1109/TAP.2018.2858200. free .