3.3 Multivariable Differential and Integral Calculus 175
There are three special situations worth mentioning:
- The change in two dimensions from Cartesian to polar coordinatesx =rcosθ,
y=rsinθ, with the Jacobian∂(x,y)∂(r,θ)=r. - The change in three dimensions from Cartesian to cylindrical coordinatesx=rcosθ,
y=rsinθ,z=z, with the Jacobian∂(x,y,z)∂(r,θ,z)=r. - The change in three dimensions from Cartesian to spherical coordinates x =
ρsinφcosθ,y=ρsinφsinθ,z=ρcosφ, with the Jacobian∂(ρ,θ,φ)∂(x,y,z)=ρ^2 sinφ.
As an illustration, we show how multivariable integrals can be used for calculating
the Fresnel integrals. These integrals arise in the theory of diffraction of light.
Example.Compute the Fresnel integrals
I=
∫∞
0
cosx^2 dx and J=
∫∞
0
sinx^2 dx.
Solution.For the computation of the first integral, we consider the surfacez=e−y
2
cosx^2
and determine the volume of the solid that lies below this surface in the octantx, y, z≥0.
This will be done in both Cartesian and polar coordinates. We will also make use of the
Gaussian integral
∫∞
0
e−t
2
dt=
√
π
2
,
which is the subject of one of the exercises that follow.
In Cartesian coordinates,
V=
∫∞
0
∫∞
0
e−y
2
cosx^2 dydx=
∫∞
0
(∫∞
0
e−y
2
dy
)
cosx^2 dx
=
∫∞
0
√
π
2
cosx^2 dx=
√
π
2
I.
In polar coordinates,
V=
∫ π 2
0
∫∞
0
e−ρ
(^2) sin (^2) θ
cos(ρ^2 cos^2 θ)ρdρdθ
=
∫ π 2
0
1
cos^2 θ
∫∞
0
e−utan
(^2) θ
cosududθ=
∫ π 2
0
1
cos^2 θ
·
tan^2 θ
1 +tan^4 θ
dθ,
where we made the substitutionu=u(ρ)=ρ^2 cos^2 θ. If in this last integral we substitute
tanθ=t, we obtain