Use Jacobians to transform double integrals into coordinates that fit the region or the integrand.
This page changes the coordinates of a double integral to fit the region or
the integrand. When the Cartesian slices from regions and order of
integration are
awkward, another coordinate system may be simpler. A disk, for example, has
square-root bounds in Cartesian coordinates but constant bounds in polar
coordinates.
The new coordinates simplify the description and the Jacobian corrects the
area element for how small pieces stretch or shrink. The same tools evaluate
weighted integrals in mass, centroids and
probability and
the series integral in Euler's Basel sum.
Its absolute value is the local area-scaling factor:
dA=dxdy=∣detJg(u,v)∣dudv.
The determinant is negative when the map reverses orientation. Area is
non-negative, so the change-of-variables formula uses its absolute value.
To see why it measures area, take small increments Δu,Δv:
g(u+Δu,v+Δv)−g(u,v)≈Jg(u,v)(ΔuΔv).
The linear map Jg(u,v) sends a small coordinate rectangle of area
ΔuΔv to a parallelogram of area approximately
∣detJg(u,v)∣ΔuΔv. Taking the limit gives the area element
dA=∣detJg(u,v)∣dudv.
Let Ω be a region in (x,y)-coordinates and let Φ be a region
in (u,v)-coordinates. Assume that f is integrable on Ω, that g
is C1 on Φ, that Φ can be split into finitely many pieces on
which g is one-to-one with non-overlapping interiors and that the Jacobian
is nonzero away from boundary or other exceptional sets of area zero. The
images of those pieces must cover Ω once, apart from boundaries of area
zero; otherwise the transformed integral can omit or count part of the region
more than once. If a map covers the target with multiplicity, split the
parameter region into one-to-one pieces (or account for that multiplicity)
before applying the formula.
Then
Applying the theorem involves two separate tasks: rewriting the integrand in
terms of u,v and describing the old region in the new coordinates. The
second task is geometric and cannot be skipped.
For r≥0, the polar-coordinate change of variables is
x=rcosθ,y=rsinθ,
and its Jacobian satisfies
∂(r,θ)∂(x,y)=r.
Consequently,
dA=rdrdθ,
and
∬Ωf(x,y)dA=∬Φf(rcosθ,rsinθ)rdrdθ.
The factor r is also visible geometrically. A small polar rectangle has
radial side approximately dr and angular side approximately rdθ,
so its area is approximately rdrdθ. The same (r,θ) pair
parametrises complex numbers in polar form,
with x+iy=reiθ.
A usual polar description takes r≥0 and an angular interval of length at
most 2π. Each point then has one representation, except on a boundary ray
and at the origin. Those exceptional sets have area zero, so the
change-of-variables theorem still applies.
The radial limits are read along each ray from the boundary of the region;
they need not be constant.
The region is unbounded, so apply the change of variables on bounded
quarter-disks and then let their radius tend to infinity. The integrand is
nonnegative, so monotone convergence justifies this limit. Polar coordinates
give
I=∫0π/2∫0∞e−r2rdrdθ=∫0π/221dθ=4π.
In Cartesian coordinates the integrand is a product
e−x2e−y2. Because it is nonnegative, Tonelli's theorem (or monotone
limits over bounded rectangles) justifies separating the two improper
integrals: