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Electromagnetics: Boundary Conditions Explained

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5.12 Boundary Conditions
In Section 5.10 we summarized Maxwell's
a
equations for the general case of
medium characterized by arbitrary values of a, e, and
u and for different
special cases. For electromagnetic ficld problems involving several different
media, the ficlds in each medium must satisfy
separately the Maxwell's
equations in differential form for that medium. On the other hand, the
integral forms of Maxwell's equations must be satisfied collectively by the
ficlds in all the media associated with the contours,
surfaces, and volumes
over which the integrals are evaluated. Thus the sets
of solutions for the
fields in diflerent media obtained by solving the
corresponding Maxwell's
equations in diflerential form are tied together by a set of conditions determined by the integral forms of Maxwell's
equations. These conditions are
as
known
the "boundary conditions" since they relate the fields on one side
ofa boundary between two mcdia to the fields on the other side of that
boundary. The boundary conditions take into account any surface charges
and currents existing on the boundaries, which the dillerential equations
gnore.
In fact, we already introduced certain boundary conditions in
previous
sections without mentioning the name. An example of this is in Section 5.3,
where we found that the tangential component of the clectrie ficld intensity
at the boundary between a conductor placed in an electric ficld is zero,
whereas the normal component of the electrie field intensity at a point on
the boundary is equal to 1/e, times the surface charge density at that point
in order to satisfy the criterion of zero electrie field inside the conductor in
the absence of a mechanism to permit the flow of a current. tn this section
we will derive the boundary conditions for the most general case of timevarying fields in two media characterized by different sets of values of o, t,
and u by using the integral forms of Maxwell's
equations and the continuitu
equation. From the experience gained in this process, we will then write
simplified sets of boundary conditions for the difterent special cases. From
Table 5.5, the integral forms of Maxwell's equations are
D dS
pdo
S
(5-208)
BdS0
(5-209)
E dl=d
C
(5-210)
S
Hd
J. ds +
D.ds
(5-211)
and the integral form of the continuity equation is
J4+pd-0
(5-212)
Let us consider two semiinfinite media separated by the plane boundary
z= 0 as shown in Fig. 5.29. Let us denote all quantities pertinent to medium
by subscript 1 and all quantities pertinent to medium 2 by subscript 2.
I
Let i, be the unit normal vector to the surface z = 0 directed into medium
Medium 1, z>0
O, E1,
Jn
Bnl
Dnl
Hi2
im
b
d
H
Ps
Jn2
Bn2
Dn2
E
E2
Z
=
0
Medium 2,
z
2, 2
P2
< 0
Fig. 5.29. For deriving the boundary conditions at the interface
between two arbitrary media.
as shown in Fig. 5.29 and let all normal
components of fields at the boundsubseript n be directed along i,
Let the surface charge density and the surface current
density on z 0 be
and
p,
J,, respectively. Note that the fields at the boundary in both media
and the surface charge and current densities are, in
general, functions of x, y;
and whereas the fields away from the
boundary are, in general, functions
ary in both media denoted by an additional
of x, y, z, and i.
First we consider a rectangular box
abcdefgh of infinitesimal volume
enclosing an infinitesimal area of the boundary and parallel to it as shown
in Fig. 5-29. Applying (5-208) to this box in the limit that the side surfaces
(abbreviated ss) tend to zero, thereby shrinking the box to the surface, we
have
lim
D dS
lim
880As
P-0
F O
p dv
0
(5-213)
Av
where AS and Av are the surface area and the volume, respectively, of the
box. In the limit that the box shrinks to the surface, the contribution from
the side surfaces to the integral on the left side of (5-213) approaches zero.
The sum of the contributions from the top and bottom surfaces becomes
(abcd)- D,2(efgh)] since abcd and efgh are infinitesimal areas. The
D
quantity on the right side of (5-213) would be zero but for the surface charge
surface reduces only the
on the boundary, since shrinking the box to the
still enclosed
volume charge enclosed by it to zero, keeping the surface charge
byit. This surface charge is equal to p,abcd). Thus Eq. (5-213) gives
D,, (abed)- D,,(efgh)
p,(abcd)
=
or
(5-214)
D,D2 P,
since the two areas abcd and efgh
equal. In vector notation, (5-214)
are
is
written as
i, (D
and (5-215)
In words, Eqs. (5-214)
(5-215)
D,) =p,
state that, al any point on
the boundary,
to the boundary are discontinuous by
and D, normal
the components of D,
at that point.
surface charge density
the amount of the
in the limit that the box
box
to the
Similarly, applying (5-209)
we obtain
shrinks to the surface,
lim
$s 0
abcdefgh
B dS
AS
(5-216)
0
the quantity on the
as
for the lefi side of (5-213),
(5-216) gives
B,2(cfgh)). Thus Eq.
Using the s a m e argument to
is cqual
[B,,(abed)
left side of (5-216)
B,(abcd)
B(/elh)
0
or
B
B
0
(5-217)
0
5-218)
In vector notation, Eq. (5-217) is written as
i, (B,-B,)
=
In words, Eqs. (5-217) and (5-218) state that, at any point on the boundary
the components of B, and B, normal to the boundary are equal.
Now, we consider a rectangular contour abcda of infinitesimal area in
the plane normal to the boundary and with its sides ab and cd parallel to the
boundary as shown in Fig. 5-29. Applying (5-210) to this contour in the limit
that ad and hc
0, thereby shrinking the rectangle to the surface, we have
lim
ad-0
be--0bcda
lim BB.ds
E dl = lim
e
(5-219)
are
In the limit that the rectangle shrinks to the surface, the contribution from
ad and he to the integral on the left side of (5-219) approaches zero. Since
ah and cd are infinitesimal, the sum of the con:ributions from ab and cd
becomes [E(ab)E, Acd). where F,, and E
are the components of E,
is
and E, along ab and c, respectivcly The
zero since the magnetic flux crossing the area abed approaches zero as the
right side of(5-219) cqualto
area abcd tends to ero. Thus Eq (5-219) gives
Etub)
EAcd)
0
or, since ah and cd are equal,
i(E,
E)0
(5-220)
where i, is the unit vector along ab. Let us now define i to be the unit vector
normal to the area abcd and in the direction of advance of a right-hand serew
it
the sense of the path abcda. Note that i, is tangential to the
as
boundary. We then have
is turned in
(5-221)
x i,
Substituting (5-221) into (5-220) and rearranging the order of the scalar
triple product, we obtain
i i , x (E, - E,)0
(5-222)
Since we can choose the rectangle abcd to be in any plane normal to the
boundary. (5-222) must be true for all orientations of i. It then follows that
i,x (E, -
E) =
0
(5-223)
or, in scalar form,
(5-224)
where E and E
the tangential
components of E, and E. respectivety
at the boundary. In words,
Eqs. (5-223) and (5-224) state that, at any poi
are
331
Boundary Conditions
on the
equai.
Sec. 5.12
boundary, the components of E, and E, tangential to the
boundary are
Similarly, applying (5-211) to the contour abcdain the limit that ad and
hc0, we have
lim
HH dllim J
ad0
bc0 abcda
ad
0
bc0
ds +lim |
D. ds
ad-0 dtt
bc--0
area
abcd
(5-225)
area
abcd
Using the same argument as for the left side of (5-219), the quantity on the
left side of (5-225) is equal to [Hab) t Hcd)], where Hab and H
are
the components of H, and H, along ab and cd, respectively. The second
integral on the right side of (5-225) is zero since the displacementflux erossingthe area abcd approaches zero_as thearea abcd tends to zero. The first
integral on the right side of (5-225) would also be cqual to zero but for a con-
tribution from the surface current on the boundary because shrinking the
rectangle to the surface reduces only the volume current enclosed by it to
This contribution is the
normal to the line which abcd approaches when it
0zero, keeping the surfacecurrent stillenclosed by it.
surface current flowing
shrinks to the surface, that is, the current crossing this line along the
Thus Eq. (5-225) gives
ofiThis quantity is equal to [J,. i,(ab).
direction
Haab) + Heded)= (J, i,)ab)
or, since ab and cd are equal,
(H,
p
Substituting (5-221) into (5-226)
triple product, we obtain
(5-226)
H,) = J, i
and rearranging the order of the
scalar
(5-227)
i, x (H, -H) i, =J, . i,,
all orientations of i, that is,
Since (5-227) must be true for
it follows that
normal to the boundary,
plane
abcd in any
for a rectangle
,x (H, - H,)=J,
(5-228)
H,H J
(5-229)
in the limit that
point.
to the box abcdefgh
(5-212)
Finally, applying
the box
form,
or, in scalar
respectively.
components of H, and H,,
are the tangential
and
H,2
where H,,
at any point
(5-228) and (5-229) state that,
Eqs.
words,
In
boundary
at the boundary.
and H, tangential to the
H
of
components
the
on the boundary,
density at that/,
cqual to.the surfacecurrent
amount
are discontinuous by the
shrinks to the surface,
lim
we
have
ss0AS
J . dS lim
pdv
Av
0
(5-230)
332
Materials and Fields
Chap. 5
In the limit that the box shrinks to the surface, the contribution to the first
integral on the left side of (5-230) from the side surfaces of the box would
be zero but for the surface current on the boundary, since although the volume
current emanating from the side surfaces reduces to zero, there still remains
the surface current emanating from them. This current is
J
(d1 x i,)
V, . J,)dS
(V, J,Xahcd)
abcd
abcd
where the subscript s in V, denotes that the divergence is computed in the
two dimensions tangential to the surface. The sum of the contributions
from
the top
and
bottom
surfaces
is
equal
to [/,, (abed)
- J,,(efgh)]
or
i, (J,-J,Mabcd). The second integral on the left side of (5-230) is equal
to (dp,/0r)abcd). Thus Eq. (5-230) gives
V, J, +i, (J,
-
abcd) - 0
J,N(abcd) +
or
i,
J ) = -V, J,
-
(5-231)
In words, Eq. (5-231) states that, at any point on the boundary, the components of J, and J, normal to the boundary are discontinuous by the amount
equal to the negative of the sum of the two-dimensional divergence of the
surface current density and the time derivative of the surface charge density
at that point.
Equations (5-215), (5-218), (5-223), (5-228), and (5-231) form the set of
boundary conditions for the most general case of time-varying fields in two
arbitrary media. Although we have derived these boundary conditions by
considering a plane surface, it should be obvious that we can consider any
arbitrary-shaped boundary and obtain the same results by letting the bo0x
and the rectangle shrink to points on the boundary. We can now write the
boundary conditions for various special eases by inspection of the corre
sponding sets of Maxwell's equations and continuity equation listed in Table
5.5. These boundary conditions are listed in Table 5.6, together with the
general boundary conditions. Depending upon the problem, only some of the
boundary conditions need to be used in the determination of the fields.
whereas some or all of the remaining boundary conditions are automaticaly
satisfied and the rest deternmine the surface charge and current densities on
the boundary. Before we consider some examples, let us investigate the
boundary condition for the power flow normal to the boundary. Letting
P, and P, be the Poynting vectors corresponding to the fields in media
and 2, respectively, we have
i(P,- P,) =i (E, x H, - E, x H,)
=G, x E,) x (G, x H,) i , - (G, x E,) x G, x H,) i,
(5-232)
Se, 1.12
TABL 5.6, Summary of Boundary (Conditions for
vector
normal to the boundary and
Varos a s (i, is the ut
dran towardo medinum )
Deuriptim
Buumdary undisia
Time-varying fields
Mcdium 1; arbitrAry, a
Medium 2: arbitrary, a
/
(1
, (
D,)P
, (H,
H),
,(JJ;)Static field
(D
Medium1; arbitrary, a /
V,,
D)P
B)0
Medium 2: arbitrary, a2 /
, x(E
E2)0
H2)
J)
Time-varying fields
Medium 1: perfect dielectrie, a
Medium 2: perfect dielectric, a2
3,
V, . ,
D2)
(B
Ba)
0
, x(E,E)0
Static ficlds
Medium 1: perfect dielectric, ai0
i,x(H,
H)0
i
Da)
(D
iX (E
Medium 2: perfect dielectric, a0
0
B2)
E2)0
(B
inX (H
H2)
0
in D
Time-varying fields
B
Medium1: perfect diclectric, dj 0
inx E
Medium 2: perfect conductor, d2
0
i,x H1,
Statie electric field
i, D
Medium 1: perfect dielectric,
inX E
Medium 2: perfect conductor, d2
into (5-232),
we
0
get
Substituting (5-223) and (5-228)
P) (i, x E,) x [i, x H,) J,] . i,
i, (P,
, x E) x ti, x H,).i
+
Ii, x E,) x J,] i,
.
(5-233)
i, x E,) x J,] . i,
J,)E,
(J
E,i,] . i,
J, E
since (i,
zero. Thus.
J) is equal to
ponents of the Poynting
al any point on
vector normal
to the
the boundary, the c o m -
boundary are
discontinuous
associated with the surface
current
equal to the power densilysurface current, the normal compoby
In the absence of a
density at that point.
continuous.
the amount
nents
EXAMPLt
of the Poynting
5-14.
In
Fig. 5.30,
vector are
comprises the region 2
0 and medium 2
comprises the region z
uniform in both media
0. All fields are spatially
medium )
Medium
x
0
L
=
Medium 2
02
0
0
360
Fig. 5.30. For Example 5-14.
and independent of time. The quantities o, and e, are constants. If the current
density in medium 1 is given by
J, = J,G,+2i, + 6i,)
where ,
is a constant, find (a) the electric field intensity vector E, in medium
2, and (b) the surface charge density p, on the interface z =0.
The electric field intensity E, in medium 1 is given by
E,
6 , +21, + 6i)
From (5-223), the tangential component of
E, is equal to the tangential
component of E,. Thus E2z = Jo/0, and E2, = 2J,/a. Since all fields are
spatially uniform and independent of time, V, J, = 0 and ôp,/dt = 0.
Then, from (5-231) the normal component of J, is equal to the normal
component of J,. Thus J,, 6J, and E2, J2/o, 6J,/3o,
The electric field intensity
E, in medium 2 is therefore given by
=
E
From (5-215), the surface
=
=
2J,/do"
, +2i, +2i,)
charge density p, on the interface z = 0 is given by
P , i , (D, -
D,)
D-D,.=6,E1,:f,E
E
-2e
2 Eodo
Oo
EXAMPLE S-15.
In Fig.
5.31, a perfect dielectric medium x<0 is
bounded by a
perfect conductor (x 0). The electric
field intensity for x <0 is
oy
=
given
E(x, y, z, 1) ==[E, cos (0t-- Bx cos 6
Bz sin 8)
E cos (wt + Bx cos 6Bz sin 0)]i,
where E, Ez, 0, P, and 0
are constants.
Find the relationship between
and E. Then find the
E
surface current
density on the surface
0.
335
Boundary Conditions
Sec. 5.12
,
E, B
-07777IITT77IIT777
Perfect
Conductor
Fig. 5.31. For Example 5-15.
From the boundary conditions listed in
Table 5.6, the
component of the electric field intensity at the surface of a tangential
perfect conductor
must be zero. Thus
E
(E, + E,) cos (wt
For this to be true for all values of z and
Bz sin 0) == 0
,
E, t E must be zero. Hence
E,=E
The electric field intensity for
x<0 is then given by
E[E, cos (otBx cos 6-ßzsin 8)
E, cos (ot + Bx cos 0-Bz sin 0)]i,
(5-234)
2E, sin (Bx cos 0) sin (»t- Bz sin 6)i,
The corresponding magnetic flux density B can be obtained
by using
Maxwell's curl equation for E, given by
OB x
V
E
OE,
(5-235)
dz
Substituting for E, in (5-235) from (5-234) and integrating with respect to
time, we obtain
B
iP [sin 0 sin(Bx cos 0) sin(ot- Bz sin 8)i,
cos 0
cos (ßx cos 0) cos (ot- Bz sin 8)i,]
The magnetic flux density at the surface of the perfect conductor is given by
B],-
EiP cos 0 cos (ot
z sin 0)i,
Note that the condition of zero nornmal component of B at the surface
of the perfect conductor is automatically satisfied by the zero tangential
component of E. This is because the boundary condition for the tangential
component of E is obtained from the integral form of V x E -0B/0t
whereas the boundary condition for the normal component of B is obtained
from the integral form of V B 0 . However, V B 0 follows from
VxE
Finally,
OB/ð1. Hence the two boundary conditions are not independent.
the surface current density at the surface of the perfect conductor
336
Materials and Fields
is given by
J3,, = i , x [H),-o
2E, cos 0 cos (t- Bz sin 0) i, T
Chap. 5
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