For Differential Equations > s.a. fokker-planck.
$ Def: For a second order linear differential operator L, the symmetric
2-point function G satisfying
L G(x, x') =
(x–x')
.
Notice that a given operator L has many Green functions, depending
on the boundary conditions imposed on the solution.
* Applications: Used
to find solutions of the de L
= j,
given the source j and the boundary conditions on the field
,
i.e., to propagate the field;
It
is thus also called propagator.
@ Specific types of equations: Haba JPA(04)ht, JMP(05)mp [strongly
inhomogeneous media, singular coefficients]; Tyagi JPA(05)
[Poisson, periodic boundary conditions]; Moroz JPA(06)mp [Helmholtz
and Laplace, quasi-periodic].
@ For non-linear equations: Frasca MPLA(07)ht/07 [and
quantum field theory applications]; Frasca a0704 [short-time
expansion].
For Classical Field Theory > s.a. gravitational
radiation.
* Interpretation: The field produced by a unit strength point source
at
a given point x.
* In electrodynamics: Used to write the electrostatic potential as
(x)
=
V
dv'
(x') G(x, x')
+ (1/4
)
bdry(V) da' · (G
'
–
'G)
.
@ General references: Green 1828-a0807;
in Morse & Feschbach 53;
Barton 89.
@ In curved spacetime: Waylen PRS(78)
[early universe, singular and regular terms]; Molnár CQG(01)gq [electrostatic,
in Schwarzschild].
For Other Classical Systems > see Kadanoff-Baym [transport].
For Quantum Systems > s.a. feynman
propagator; green functions in quantum field
theory; quantum
oscillator.
@ References: Tsaur & Wang AJP(06)
[Schrödinger equation]; Miyazawa JPA(06)
[1D, ito reflection coefficients].
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Send feedback and suggestions to bombelli at olemiss.edu – Modified
11 jul 2008