(508696274) vector iii 2015
DESCRIPTION
Vector Calculus (Surface Intergral)TRANSCRIPT
Surface Integral
Surface Integral
1Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
2Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
3Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
4Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
5Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
6Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
7Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
8Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
Stoke’s Theorem
9Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
10Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
11Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
12Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
13Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
14Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
15Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
Triple Integrals - Divergence Theorem of Gauss (1777-1855)
The triple integral is a generalization of the double integral introduced above.
For defining this integral,
f x, y, z defined in a bounded closed region T of space.one considers a function One subdivides T by
planes parallel to the three coordinate planes. Then, one numbers the parallelepipeds inside T from 1 to n.16
Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
xk , yk , zk In each such parallelepiped, one chooses an arbitrary point, say in the kth
parallelepiped, and form the sum
n
f xk , yk , zk vk
k 1
(1)Jn
where vk is the volume of the kth parallelepiped. This limit is called the triple integral of
f x, y, z over the region T, and is denoted by
f x, y, z dxdydz f x, y, z dvT
or (2)T
Fˆ nˆd div Fˆdxdydz div
Fˆdv
(3)S T T
Example
17Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
Compute Fˆ nˆ d , whereS
Fˆ x, y, z x2iˆ 2 yˆj 4z2kˆ and S is the surface of the cylinder
x2 y2 4, 0 z 2 .
Solution
Fˆdiv 2x 2 8z , so
2
Fˆ nˆ 2x 2 8z dzdxdy
2x 2 8z dzdxdy
0x2 y2 4S T
2 xz 2 z 4 z 2 z=2 dxdy 4 x 20 dxdy
x2 y2 4
x2
y2 4
z=0
Let x r cos and y r sin , then x2 y2 4 r 2 cos2 r 2 sin2 r 2 r 2 .
The differential area in the polar coordinate system becomes dA dxdy rdrd .)
2 2 2 2 r cos 5r drd4r cos 20)rdrd 4 2 0 0 0 0
2 8 4 cos 10 d 800 3
18Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
Example
By transforming to a triple integral, evaluate
I x3dydz x2 y dxdz x2 z dxdy S
x2 y2 a2 0 z bwhere S is the closed surface consisting of the cylinder and the dicks z=0
and z=b. From (6), it is evident that
P x3 , Q x2 y, R x2 z
Hence, by taking advantage of the symmetry of the circle (evaluate only 1/4 of the circle), the
corresponding triple integral takes the from by (6)
a 1b a a2 y23/ 2 b
I 3x2 x2 x2 dxdydz 4 5 a2 y2 dydzx2 dxdydz 20 0 0 30 0 0 T
Let y a sin , dy a cos d , then
3/ 2
3/ 2
a2 3/ 2
a2
cos2
a3
cos3
a2 y2 1 sin2
and
1 3 a41 3/ 2 1 /2 aa2 y2 dy a4 cos4 d a4 3 3 3 8 2 160 0
Hence, the integral I becomes
19Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
4b a 5I 20 dz
a4b16 40
Example
F
ˆ
If and nˆ are expressed in terms of their Cartesian components such that
x iˆ
y ˆj z
kˆ nˆ cos x, n iˆ cos y, n ˆj cos z, n kˆ Fˆr r r
where
r x2 y2 z 2 and the region T is the sphere x2 y2 z2 a2
Evaluate the triple integral :
Solution
Assuming that r 0
x2 y2 z 2 x2 / x2 y2 z 2 r 2 x2P x
x x x2 y2 z 2 r3
x2 y2 z 2
Likewise,
Q r 2 y2 R r 2 z 2
and r 3 r 3y z
Hence,
3r 2 r 2 2 2 rdiv F if r 0 and dxdydzr3
r T
Since the triple integral is discontinuous when r=0, care must be exercised. Returning back to
the equivalent surface integral reveals that
2 2 2 x
y
z Fˆ nˆd d 1d 4 a2S
r 2 Sr 2 r 2
S
The integral is simply the surface area of a sphere of radius a, thus avoiding an integral
containing a discontinuity at r=0.
20Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
The triple integral may be evaluated by transforming the Cartesian coordinates into the spherical
coordinates. From the sketch, it is clear that
In this case, r . dv dxdydz r 2 sin drdd
2 2 a 1 2
dxdydz 2 r 2 sin drd d a2 sin d dr r0 0 0 0 0
T
2 cos 1 1 4 a2 2 2 d 2 a a0 0
As expected, it yields the same result.
21Sk/EUM114/ Vector 3 Lecture/2015
S (dx)i (dz)k (dxdz) j
S (dy) j (dz)k (dydz)i
Surface Integral
Hints on Surface Itegrals
surface S’ with the
Case 1. Parametrize and IntegrateWrite the parametric equation r(u,v) of the surface. Find dS = (ru x rv) du dv. Take the dot product with F and integrate over u and v.
Case 2. Use the Divergence (Gauss’s) Theorema) The Divergence Theorem has exactly the same flavor as Stoke’s Theorem.
You go up one dimension You take some kind of derivative of the integrand
You integrate over the region bounded by the closed shape
b)
c)
In the xz plane, d
In the yz plane, d
Case 3.In Stoke’s theorem,
Curl (F ) =0, implies that F = Grad (f.) for some f.Then it is easy to find the potential f and evaluate at the end points. Another way of saying this is that the integral depends only on the boundary of the curve, namely the end points. Thus, one could replace thecurve by the simplest curve with the same boundary, namely a line joining the end points. In practice onenever does this since it is simpler to evaluate f at the end points.22Sk/EUM114/ Vector 3 Lecture/2015
Is
No Yes
Is S closed? Is S closed?
No Yes No Yes
Parametrize andIntegrate
Choose simplest
same boundary=0
Surface Integral
In Gauss’s theorem, ifDiv(F)=0, implies that F=Curl(A) for some A.
Now it is not easy to find the vector potential A. But the situation is similar. The integral depends only on the boundary, so one can replace the original surface S with the simplest surface that has the same boundary. So, for example, if the surface is the upper hemisphere z=sqrt(a^2-x^2-y^2), where the computation of the differential of surface is nasty, one could use the surface z=0, (where dS = dx dy k) and integrate over a circle of radius a.
Think of this as the butterfly net catcher theorem. If Div (F) =0 then there are no sources or sinks insidethe surface, the flux of butterflies coming into the surface net depends only on the Rim of the net.Case 4.
If Div(F)=0 and the surface is closed, then there are no sources or sinks inside the surface, so the net Fluxis zero! Whatever goo comes in, must come out..So Why is this Important?
Gauss’s and Stoke’s theorem are central to Physics. Without Gradients, Curls and Divergences, one couldnot give a full quantitative description of Gravitation, Electrodynamics, Fluid Dynamics, AerospaceEngineering, Atmospheric Sciences…you get the point.
23Sk/EUM114/ Vector 3 Lecture/2015
Surface Integral
Summary of Surface Integrals
Indicate How to Compute
dz dz
f ( x, y, z)
1 dA , where dx dy D
f (P* )Slimm,n
1 1S
Du v
S
S
dS , OR
ndS
C S
* *F (r r )dA , where D is the pre-image
m,nS E
is the boundary of E
Note: There are analogous notations, definitions, and formulas for situations in which the roles of x, y, and/or z are swapped.
24Sk/EUM114/ Vector 3 Lecture/2015
inte
gral
of
a ve
ctor
Type of Int.
Notation Definition andInterpretations/Applications
Standard/Direct Way to ComputeMajor Theorems that
Indirectly
surf
ace
inte
gral
of
a re
al-v
alu
ed f
un
ctio
n
f ( x, y, z)dS
m n
ij ij
i j
(mass/moments of a surface)
2 2
z g(x, y) is the function whose graph is the surface S of integration and D is the
projection of S; OR f (r(u, v)) r r dA
where D is the pre-image (in the uv-plane) ofS
Su
rfac
e (o
r fl
ux)
fiel
d
F
F
(this notation infers outward orientation if S is closed and upward orientation if S is not closed)
Based on an upward orientation of S
m n
lim FPij nPij S ij
i1 j 1
(rate of flow through a surface)
g gD
P(x, y, z) x
Q(x, y, z) y
R(x, y, z) dA
where z = g(x,y) is the function whose graph is the surface S of integration and D is the projection of S; OR
D u v
(in the uv-plane) of S
Stokes’ Theorem:
F dr curlF dS where
C
is the boundary of SDivergence Theorem:
F dS divFdV where
S