In this section the direct and indirect boundary and shell integral
equation formulations of the interior Laplace equation are given.
The boundary and shell integral
equations may be regarded as hybrids of their respective
standard boundary integral equation formulations as given, for example
in Jaswon and Symm (1977) and shell
integral equation formulations given in Ben Mariem and Hamdi (1987)
and Warham (1988).
Let the function v(p) for p Î S be defined as follows
v(p) =
lim
e® 0+
¶j
¶np
(p + enp ) (p Î S),
where np is the unit outward normal to S at p.
Each shell is assumed to have two sides or surfaces, let G+
be the upper surface and let G- be the lower surface.
The potential j and its derivatives are generally discontinuous at
the shell, however they
take limiting values on G+ and G-.
Let the functions j+ (p), j- (p),
v+ (p) and v- (p) (p Î G)
be defined as follows:
j+(p) =
lim
e® 0+
j(p + enp ) ,
j-(p) =
lim
e® 0+
j(p - enp ) ,
v+(p) =
lim
e® 0+
¶j
¶np
(p + enp ) ,
v-(p) =
lim
e® 0+
¶j
¶np
(p - enp ) .
The geometrical function c(p) (p Î S ÈG) is
defined to be the angle subtended by the interior region at p for
points on S and the angle subtended by G+ for points on G.
It is helpful to introduce the functions
d(p), n(p), F(p) and
V(p) for p Î G which are defined as follows:
The Laplace integral operators L, M, Mt, and N
are defined as follows:
{ L m}P(p) º
ó õ P
G (p,q) m(q) dSq (p Î E ÈS ÈG) ,
{ M m}P(p) º
ó õ P
¶G
¶nq
(p,q) m(q) dSq (p Î E ÈS ÈG) ,
{ Mt m}P(p) º
¶
¶np
ó õ P
G(p,q) m(q) dSq (p Î S ÈG) ,
{ N m}P(p) º
¶
¶np
ó õ P
¶G
¶nq
(p,q) m(q) dSq (p Î S ÈG) ,
where P Ì S ÈG, nq and
np are unit outward normal to P when P Ì S
or the unit normal to P+ when P Ì G
at q, p and m(q)
is a bounded function defined for q Î P. G(p, q) is the free-space Green's function for the Laplace equation,
The equations that make up the boundary and shell integral equation
formulation of the Laplace equation are given in this subsection.
For points on the boundary the following equation holds:
{ M j}S (p) + c(p) j(p) = { L v } S (p)+ { M d}G (p) - { L n}G (p) (p Î S).
(1)
This equation relates
j(p) and v(p) for points p on the boundary S.
For points on the shell, we have the following equations:
F(p) = - {M j}S(p) + {L v }S(p)+ {M d}G(p) - {L n}G(p) (p Î G) ,
(2)
V (p) = - {N j}S(p) + {Mt v }S(p)+ {N d}G(p) - {Mt n}G(p) (p Î G) .
(3)
The value of j(p) for points in the domain
are related to the solutions on S and G through the following equation:
j(p) = - { M j}S (p) + { L v }S (p) + { M d}G(p) -{ L n}G (p) (p Î D) .
The equations that make up the indirect boundary and shell integral equation
formulation of the Helmholtz equation are given in this subsection.
For points on the boundary the following equations hold:
j(p) = { L s} S (p)+ { M d}G (p) - { L n}G (p) (p Î S),
(5)
v (p) = {Mt s}S(p) + c(p) s(p)+ {N d}G(p) - {Mt n}G(p) (p Î S),
(6)
where s is generally known as a source density function.
These equations relate
j(p) and v(p) for points p on the boundary S.
For points on the shell, we have the following equations: