All chapters Unit 2 · Integral & Vector Calculus

Change of variables and the Jacobian

Chapter 11 of 15
The hook

The integral even sideways slicing can't save

Chapter 10 left you with a promise: there is a famous integral that the order-swap trick cannot rescue. Here it is — the Gaussian, the most important integral in all of probability:

I=ex2dx.I = \int_{-\infty}^{\infty} e^{-x^2}\,dx.

Every Chapter 10 move fails. There is no elementary antiderivative for ex2e^{-x^2} — so the Fundamental Theorem is useless. And there is no inner integral to swap: this is a single integral, so changing the order of integration has nothing to change. We are stuck — until we do something that looks insane.

√π area ∫ e^(−x²) dx — no antiderivative y = e^(−x²) r dr dθ square it, then go polar e^(−r²) on the plane
The bell curve's area (left) is exactly π\sqrt{\pi} — but you cannot get there along the xx-axis. Square the integral, read it as a double integral over the whole plane, and switch to polar (right): a factor rr drops out of nowhere and makes the impossible a one-liner.

The punchline, which we will earn in full after the break:

(ex2dx) ⁣2=R2e(x2+y2)dA=πI=π.\left(\int_{-\infty}^{\infty} e^{-x^2}\,dx\right)^{\!2} = \iint_{\mathbb{R}^2} e^{-(x^2+y^2)}\,dA = \pi \qquad\Longrightarrow\qquad I = \sqrt{\pi}.

The whole trick turns on that rr appearing when we go polar. Where did it come from? Chapter 10 told you to write dA=rdrdθdA = r\,dr\,d\theta and never drop the rr — but it never told you why the rr is there. That "why" is this entire chapter, and its name is the Jacobian.

Why this matters

Polar was a special recipe you memorised. The Jacobian is the general tool behind it: any substitution re-grids the plane, and the factor that corrects for the re-gridding is J|J|. Master it once and you never again have to remember a coordinate system's area element — you can derive it. And the payoff is not academic: the π\sqrt{\pi} you are about to compute is the exact reason the normal distribution — the bell curve under nearly every dataset she will ever model — normalises the way it does.

Intuition before formulas

A substitution warps the plane

In single-variable calculus, uu-substitution carries a dudx\dfrac{du}{dx} factor — the substitution stretches the line, and du=dudxdxdu = \dfrac{du}{dx}\,dx corrects for the stretch. In two dimensions the same thing happens, but the plane can stretch differently in different directions, so the correction is richer.

Picture a clean uvuv-grid of little unit squares. A change of variables x=x(u,v)x = x(u,v), y=y(u,v)y = y(u,v) sends that grid to a warped grid in the xyxy-plane. A small cell of area dudvdu\,dv lands as a small parallelogram, and its area is no longer dudvdu\,dv — it is scaled by some local factor:

du dv u v x(u,v), y(u,v) |J|·du dv x y
The map sends the square uvuv-grid (left) to a warped grid (right). One unit cell of area dudvdu\,dv becomes a parallelogram of area Jdudv|J|\,du\,dv. The number J|J| is just the local area-scaling factor — nothing more mystical than that.
The honest truth about "seeing" the warp

Nobody pictures the global warp of the plane — the way the whole grid bends is genuinely hard to hold in your head, and you never need to. You compute the stretch factor locally, at the cell, with a determinant, and trust it everywhere. That single local number is the entire idea; the rest of the chapter is learning to compute it and remembering to keep its absolute value.

Formal statement

The Jacobian, stated and used

That local area-scaling factor has a formula. It is the determinant of the matrix of partial derivatives of the old coordinates with respect to the new ones:

The Jacobian, and the change-of-variables theorem
J=(x,y)(u,v)=xuxvyuyv,Rf(x,y)dA=Sf(x(u,v),y(u,v))Jdudv.J = \frac{\partial(x,y)}{\partial(u,v)} = \begin{vmatrix} x_u & x_v \\ y_u & y_v \end{vmatrix}, \qquad \iint_R f(x,y)\,dA = \iint_S f\big(x(u,v),y(u,v)\big)\,|J|\,du\,dv.

The region RR in the xyxy-plane is described, in the new coordinates, by a simpler region SS in the uvuv-plane — usually a rectangle. Three things to hold onto:

The three load-bearing facts
  • The area element is Jdudv|J|\,du\,dv — the absolute value, always. A negative determinant means the map flips orientation; it never means negative area.
  • The integrand must be rewritten in uu and vv — every xx and yy inside ff is replaced via the substitution.
  • Reciprocal shortcut. If (x,y)(u,v)\dfrac{\partial(x,y)}{\partial(u,v)} is awkward but (u,v)(x,y)\dfrac{\partial(u,v)}{\partial(x,y)} is easy, compute the easy one and flip it:  (x,y)(u,v)=1(u,v)/(x,y).\ \dfrac{\partial(x,y)}{\partial(u,v)} = \dfrac{1}{\partial(u,v)/\partial(x,y)}.

And now the chapter's spine, paid off. For polar coordinates x=rcosθx = r\cos\theta, y=rsinθy = r\sin\theta, with (u,v)=(r,θ)(u,v) = (r,\theta):

J=(x,y)(r,θ)=cosθrsinθsinθrcosθ=rcos2θ+rsin2θ=r.J = \frac{\partial(x,y)}{\partial(r,\theta)} = \begin{vmatrix} \cos\theta & -r\sin\theta \\ \sin\theta & r\cos\theta \end{vmatrix} = r\cos^2\theta + r\sin^2\theta = r.

So J=r|J| = r, and dA=rdrdθdA = r\,dr\,d\thetaexactly the recipe you were handed in Chapter 10. The mysterious rr was the Jacobian of the polar map all along.

Worked example · WE-1 · compute a Jacobian, see the area scale

Take the linear map u=x+yu = x + y, v=xyv = x - y. Invert it: x=u+v2x = \tfrac{u+v}{2}, y=uv2y = \tfrac{u-v}{2}. Then

J=(x,y)(u,v)=12121212=1414=12,J=12.J = \frac{\partial(x,y)}{\partial(u,v)} = \begin{vmatrix} \tfrac12 & \tfrac12 \\[2pt] \tfrac12 & -\tfrac12 \end{vmatrix} = -\tfrac14 - \tfrac14 = -\tfrac12, \qquad |J| = \tfrac12.

Every area halves. Check it with the shortcut: (u,v)(x,y)=1111=2\dfrac{\partial(u,v)}{\partial(x,y)} = \begin{vmatrix} 1 & 1 \\ 1 & -1 \end{vmatrix} = -2, and 12=12\dfrac{1}{-2} = -\tfrac12 — same answer. The sign of JJ is bookkeeping (the map reflects); the area element takes J=12|J| = \tfrac12.

Worked example · WE-2 · a full evaluation, linear

Evaluate Re(xy)/(x+y)dA\displaystyle\iint_R e^{(x-y)/(x+y)}\,dA over the triangle with vertices (0,0)(0,0), (1,0)(1,0), (0,1)(0,1). The exponent begs for u=xyu = x - y, v=x+yv = x + y; from WE-1, J=12|J| = \tfrac12. The triangle x0, y0, x+y1x \ge 0,\ y \ge 0,\ x + y \le 1 becomes the clean region 0v10 \le v \le 1, vuv-v \le u \le v:

01 ⁣vveu/v12dudv=1201v(ee1)dv=ee14=e214e0.5876.\int_0^1\!\int_{-v}^{v} e^{u/v}\,\tfrac12\,du\,dv = \tfrac12\int_0^1 v\,(e - e^{-1})\,dv = \frac{e - e^{-1}}{4} = \frac{e^2 - 1}{4e} \approx 0.5876.

The slanted boundaries xy=constx - y = \text{const} and x+y=constx + y = \text{const} became horizontal and vertical lines in uvuv — that straightening is the whole reason to change variables.

Worked example · WE-3 · non-linear, the chapter's teeth

Find the area of the region bounded by xy=1xy = 1, xy=2xy = 2, y=xy = x, and y=4xy = 4x. The boundaries are products and ratios held constant, so substitute u=xyu = xy, v=y/xv = y/x. Inverting, x=u/vx = \sqrt{u/v}, y=uvy = \sqrt{uv}, and the Jacobian works out (via the shortcut, (u,v)(x,y)=2y/x=2v\tfrac{\partial(u,v)}{\partial(x,y)} = 2y/x = 2v) to

J=12v.|J| = \frac{1}{2v}.

The four curves become four straight lines: 1u21 \le u \le 2, 1v41 \le v \le 4. So

Area=14 ⁣1212vdudv=1412vdv=12ln4=ln20.6931.\text{Area} = \int_1^4\!\int_1^2 \frac{1}{2v}\,du\,dv = \int_1^4 \frac{1}{2v}\,dv = \tfrac12\ln 4 = \ln 2 \approx 0.6931.

Notice J=12v|J| = \tfrac{1}{2v} is not constant — it changes across the region. That is exactly what makes the non-linear case harder than WE-1, and exactly where marks are lost: you cannot pull a varying Jacobian out of the integral.

End of sitting 1 — you can now write down a Jacobian, use the reciprocal shortcut, and straighten a region with both a linear and a non-linear substitution. After the break: the Gaussian, paid in full, then the Jacobian Predictor to drill the one skill that matters, and the exam-shaped practice set.

Applications · the payoff

Cashing the hook: the Gaussian, in full

Now we earn the π\sqrt{\pi}. The trick is to compute I2I^2 instead of II, because a product of two single integrals is a double integral over the plane:

Worked example · WE-4 · the polar payoff

Let I=ex2dxI = \displaystyle\int_{-\infty}^{\infty} e^{-x^2}\,dx. Writing the second copy in the variable yy,

I2=(ex2dx)(ey2dy)=R2e(x2+y2)dA.I^2 = \left(\int_{-\infty}^{\infty} e^{-x^2}\,dx\right) \left(\int_{-\infty}^{\infty} e^{-y^2}\,dy\right) = \iint_{\mathbb{R}^2} e^{-(x^2+y^2)}\,dA.

Over the whole plane, switch to polar: x2+y2=r2x^2 + y^2 = r^2, and dA=rdrdθdA = r\,dr\,d\theta — the Jacobian J=r|J| = r is what makes this work:

I2=02π ⁣0er2rdrdθ=02π[12er2]0dθ=02π12dθ=2π12=π.I^2 = \int_0^{2\pi}\!\int_0^{\infty} e^{-r^2}\,r\,dr\,d\theta = \int_0^{2\pi}\Big[-\tfrac12 e^{-r^2}\Big]_0^{\infty} d\theta = \int_0^{2\pi}\tfrac12\,d\theta = 2\pi\cdot\tfrac12 = \pi.

So I2=πI^2 = \pi, and since I>0I > 0,  I=π\ \mathbf{I = \sqrt{\pi}}. The rr that made the inner integral elementary — er2re^{-r^2}\,r integrates instantly, while ex2e^{-x^2} never could — is the Jacobian. It is the same rr you were told never to drop in Chapter 10, now revealed as the hero of the whole calculation.

The anchor — why you actually care

That π\sqrt{\pi} is not a curiosity. The normal distribution is 1σ2πe(xμ)2/2σ2\dfrac{1}{\sigma\sqrt{2\pi}}\,e^{-(x-\mu)^2/2\sigma^2}, and the 2π\sqrt{2\pi} downstairs is there for exactly one reason: to make the total probability integrate to 11. That constant is a rescaled version of the integral you just did. Every time a dataset is modelled as "normally distributed" — heights, measurement errors, exam scores, noise in a signal — the bell curve normalises because ex2dx=π\int_{-\infty}^{\infty} e^{-x^2}\,dx = \sqrt{\pi}. You have just derived the cornerstone of statistics with a coordinate change.

Interactive playground

The Jacobian Predictor

One rule: commit your prediction of J|J| before the area-scale renders. Pick a substitution, watch the uvuv-grid map to its warped xyxy-image, then commit what you think the local area-scaling factor is. Only then does the answer light up. Committing — even to a wrong factor — is what installs the reflex; recognising J|J| once you are shown it is not the same skill.

The Jacobian Predictor
What to notice
  • Linear maps scale by a constant. The shear halves every cell (J=12|J| = \tfrac12); the stretch enlarges by 2×3=62 \times 3 = 6. The grid stays made of identical parallelograms.
  • Polar and multiplicative maps scale differently at different places. J=r|J| = r grows as you move out; J=12v|J| = \tfrac{1}{2v} shrinks as vv grows. The image cells are visibly unequal.
  • The absolute value is not optional. Commit a negative value and the Predictor stops you: a negative determinant flips orientation, it does not make area negative.
  • The dropped factor is the classic loss. Predict 11 for the polar map and you have made the exact Chapter 10 mistake — the rr is the Jacobian.
Retrieval gauntlet

Test yourself before moving on

Commit to an answer before reading the feedback. These interleave computation with decision-only items on purpose — knowing which Jacobian a problem wants is half the skill.

Quiz 1 · polar, through the Jacobian

R(x2+y2)dA\displaystyle\iint_R (x^2 + y^2)\,dA over the unit disk x2+y21x^2 + y^2 \le 1 equals:

Quiz 2 · the reciprocal trap

Find the area of the xyxy-region that maps to the rectangle 0u40 \le u \le 4, 1v71 \le v \le 7 under u=x2yu = x - 2y, v=3xyv = 3x - y.

Predict the next step. You can read (u,v)(x,y)\dfrac{\partial(u,v)}{\partial(x,y)} straight off u=x2yu = x - 2y, v=3xyv = 3x - y. Which determinant is that — and what must you do to it before it multiplies dudvdu\,dv?

Easy determinant first. uu and vv are given in terms of x,yx, y, so (u,v)(x,y)\dfrac{\partial(u,v)}{\partial(x,y)} is immediate:

(u,v)(x,y)=1231=(1)(1)(2)(3)=5.\frac{\partial(u,v)}{\partial(x,y)} = \begin{vmatrix} 1 & -2 \\ 3 & -1 \end{vmatrix} = (1)(-1) - (-2)(3) = 5.

Reciprocate to get the factor that multiplies dudvdu\,dv:  (x,y)(u,v)=15\ \left|\dfrac{\partial(x,y)}{\partial(u,v)}\right| = \dfrac{1}{5}. The region is a rectangle of area 4×6=244 \times 6 = 24 in uvuv, so

Area=S15dudv=1524=245.\text{Area} = \iint_S \frac{1}{5}\,du\,dv = \frac15\cdot 24 = \frac{24}{5}.
Quiz 3 · name the substitution — do not integrate

For each, which substitution makes it cleanest?  (i) the disk x2+y29x^2+y^2 \le 9 with integrand e(x2+y2)e^{-(x^2+y^2)};  (ii) the region bounded by xy=1, xy=4, y=x, y=3xxy=1,\ xy=4,\ y=x,\ y=3x;  (iii) the parallelogram with sides x+2y=constx+2y=\text{const}, 3xy=const3x-y=\text{const}.

Quiz 4 · the sign that isn't an error

A student uses u=yu = y, v=xv = x, correctly finds (x,y)(u,v)=1\dfrac{\partial(x,y)}{\partial(u,v)} = -1, writes the area element as 1dudv-1\,du\,dv, and gets a negative area. What is the fix?

Exam translator — six cold problems

Exam shapes

In standard Indian engineering-math papers, and likely in MCC201A unless your class notes differ, change-of-variables wears four costumes — each one you have now seen worked:

  • "Evaluate using polar coordinates" → the Jacobian is rr; dA=rdrdθdA = r\,dr\,d\theta (WE-4, Q1). The dropped rr is the classic lost mark.
  • "Evaluate using the transformation u=, v=u = \ldots,\ v = \ldots" → compute J|J|, rewrite ff and the region (WE-2). Often a linear map straightening a slanted region.
  • "Find the area of the region bounded by \ldots" → the curves name the substitution; Jdudv\iint |J|\,du\,dv (WE-3). Products/ratios ⇒ u=xy,v=y/xu=xy,\,v=y/x.
  • "Evaluate ex2dx\int_{-\infty}^{\infty} e^{-x^2}dx" / a normal-distribution constant → square it, go polar, π\sqrt{\pi} (WE-4).

Worked solutions are complete; nothing points off this page. Do them as listed — interleaved on purpose — not blocked by method. Two of them, PR3 and PR4 (the non-constant and scaled Jacobians), open with a faded bridge: part of the work is set out, the key step left for you to predict.

PR1 · a radial integrand

Shape · disk + radial integrand ⇒ polar; |J| = r

PR1. Evaluate Rx2+y2dA\displaystyle\iint_R \sqrt{x^2+y^2}\,dA over the disk x2+y24x^2 + y^2 \le 4.

Polar. x2+y2=r\sqrt{x^2+y^2} = r, the disk is 0r20 \le r \le 2, 0θ2π0 \le \theta \le 2\pi, and dA=rdrdθdA = r\,dr\,d\theta:

02π ⁣02rrdrdθ=02π83dθ=16π3.\int_0^{2\pi}\!\int_0^{2} r\cdot r\,dr\,d\theta = \int_0^{2\pi}\frac{8}{3}\,d\theta = \frac{16\pi}{3}.

The integrand rr times the Jacobian rr gives r2r^2 — drop the Jacobian and you would integrate rr alone and get 8π...\tfrac{8\pi}{...} wrong.

PR2 · a linear straightening

Shape · slanted parallel edges ⇒ linear map; |J| = ½

PR2. Evaluate R(x+y)dA\displaystyle\iint_R (x+y)\,dA, where RR is bounded by x+y=1x+y=1, x+y=2x+y=2, xy=0x-y=0, xy=1x-y=1. Use u=x+yu = x+y, v=xyv = x-y.

Set up. J=12|J| = \tfrac12 (as in WE-1), the integrand x+y=ux+y = u, and the region is the rectangle 1u21 \le u \le 2, 0v10 \le v \le 1:

12 ⁣01u12dvdu=1212udu=1232=34.\int_1^{2}\!\int_0^{1} u\cdot\tfrac12\,dv\,du = \tfrac12\int_1^{2} u\,du = \tfrac12\cdot\frac{3}{2} = \frac{3}{4}.

Four slanted lines became four sides of a rectangle — the integral is then trivial.

PR3 · faded bridge · the multiplicative classic

Shape · products and ratios constant ⇒ u = xy, v = y/x; |J| varies

PR3. Find the area of the region bounded by xy=1xy = 1, xy=3xy = 3, y=xy = x, y=2xy = 2x.

Bridge: the curves say u=xyu = xy, v=y/xv = y/x, and the Jacobian is J=12v|J| = \tfrac{1}{2v} (not constant). Before revealing, predict the next step: what are the uu- and vv-limits, and why can't you pull J|J| out of the integral?

Limits. xy=1,31u3xy = 1,3 \Rightarrow 1 \le u \le 3; y/x=1,21v2y/x = 1,2 \Rightarrow 1 \le v \le 2. Since J=12v|J| = \tfrac{1}{2v} depends on vv, it stays inside:

Area=12 ⁣1312vdudv=1222vdv=121vdv=ln2.\text{Area} = \int_1^{2}\!\int_1^{3} \frac{1}{2v}\,du\,dv = \int_1^{2}\frac{2}{2v}\,dv = \int_1^{2}\frac{1}{v}\,dv = \ln 2.

The inner uu-integral contributed the width 31=23 - 1 = 2; the varying Jacobian turned the outer integral into a logarithm.

PR4 · faded bridge · scaled polar for an ellipse

Shape · an ellipse ⇒ scaled polar; the scale rides into |J|

PR4. Find the area of the ellipse x24+y291\dfrac{x^2}{4} + \dfrac{y^2}{9} \le 1 using x=2rcosθx = 2r\cos\theta, y=3rsinθy = 3r\sin\theta.

Bridge: this is polar with the axes pre-scaled, so the boundary is just r=1r = 1, 0θ2π0 \le \theta \le 2\pi. Before revealing, predict the next step: compute J|J| for x=2rcosθx = 2r\cos\theta, y=3rsinθy = 3r\sin\theta — how does the 2×32\times 3 scaling show up?

Jacobian.

J=2cosθ2rsinθ3sinθ3rcosθ=6rcos2θ+6rsin2θ=6r,J=6r.J = \begin{vmatrix} 2\cos\theta & -2r\sin\theta \\ 3\sin\theta & 3r\cos\theta \end{vmatrix} = 6r\cos^2\theta + 6r\sin^2\theta = 6r, \qquad |J| = 6r.

The 6=2×36 = 2\times 3 is the ordinary polar rr multiplied by the axis scaling. With 0r10 \le r \le 1:

Area=02π ⁣016rdrdθ=6122π=6π.\text{Area} = \int_0^{2\pi}\!\int_0^{1} 6r\,dr\,d\theta = 6\cdot\tfrac12\cdot 2\pi = 6\pi.

Sanity check: the ellipse x2a2+y2b21\tfrac{x^2}{a^2}+\tfrac{y^2}{b^2}\le 1 has area πab=π23=6π\pi a b = \pi\cdot 2\cdot 3 = 6\pi. ✓

PR5 · the probability payoff

Shape · square it, go polar, read off the Gaussian

PR5. Evaluate R2e(x2+y2)dA\displaystyle\iint_{\mathbb{R}^2} e^{-(x^2+y^2)}\,dA, and hence state ex2dx\displaystyle\int_{-\infty}^{\infty} e^{-x^2}\,dx.

Polar over the whole plane. x2+y2=r2x^2 + y^2 = r^2, dA=rdrdθdA = r\,dr\,d\theta:

02π ⁣0er2rdrdθ=02π12dθ=π.\int_0^{2\pi}\!\int_0^{\infty} e^{-r^2}\,r\,dr\,d\theta = \int_0^{2\pi}\tfrac12\,d\theta = \pi.

This double integral is (ex2dx)2\left(\int_{-\infty}^{\infty} e^{-x^2}dx\right)^2, so ex2dx=π\int_{-\infty}^{\infty} e^{-x^2}\,dx = \sqrt{\pi}.

PR6 · decision-only · name the move

Shape · no integration — choose the substitution and say why

PR6. For each, name the substitution and why — do not integrate. (a) (x2+y2)3/2dA\iint (x^2+y^2)^{3/2}\,dA over x2+y21x^2+y^2 \le 1; (b) the area bounded by xy=2, xy=5, y=3x, y=7xxy = 2,\ xy = 5,\ y = 3x,\ y = 7x; (c) fdA\iint f\,dA over the parallelogram with sides 2xy=const2x - y = \text{const}, x+y=constx + y = \text{const}.

(a) Polar. Circular region and a radial integrand (x2+y2)3/2=r3(x^2+y^2)^{3/2} = r^3 — both signals point polar; J=r|J| = r.

(b) Multiplicative. Boundaries are products xy=constxy = \text{const} and ratios y/x=consty/x = \text{const}, so u=xy, v=y/xu = xy,\ v = y/x straightens all four; J=12v|J| = \tfrac{1}{2v}.

(c) Linear. Slanted straight edges held constant ⇒ u=2xy, v=x+yu = 2x - y,\ v = x + y; J|J| is a constant you read off the determinant. No circular symmetry, so polar would only make it worse.

Three things to carry out of this chapter

  1. Change of variables re-grids the plane; the area element scales by J|J|. dA=JdudvdA = |J|\,du\,dv, absolute value always — rewrite the integrand and the region in u,vu, v too.
  2. Polar's rr was the Jacobian all along. Same factor, now from one general rule: x=rcosθ, y=rsinθJ=rx = r\cos\theta,\ y = r\sin\theta \Rightarrow |J| = r.
  3. Compute the easy determinant and reciprocate. (x,y)(u,v)=1(u,v)/(x,y)\dfrac{\partial(x,y)}{\partial(u,v)} = \dfrac{1}{\partial(u,v)/\partial(x,y)}.
Pre-flight checklist — run it before you integrate
1. Sketch drawn? Limits read off the sketch, not the statement?\textbf{1.}\ \text{Sketch drawn? Limits read off the sketch, not the statement?} 2. Outer limits constant? Inner limits depend only on the outer variable?\textbf{2.}\ \text{Outer limits constant? Inner limits depend only on the outer variable?} 3. Polar: is the r in dA=rdrdθ present?\textbf{3.}\ \text{Polar: is the } r \text{ in } dA = r\,dr\,d\theta \text{ present?} 4. Change of variables: is J present, and is it the absolute value?\textbf{4.}\ \text{Change of variables: is } |J| \text{ present, and is it the } \textit{absolute} \text{ value?} 5. Did you use (x,y)(u,v) — or reciprocate (u,v)(x,y) if that was the easy one?\textbf{5.}\ \text{Did you use } \tfrac{\partial(x,y)}{\partial(u,v)} \text{ — or reciprocate } \tfrac{\partial(u,v)}{\partial(x,y)} \text{ if that was the easy one?}
The anchor, one more time

Return to the bell curve. The π\sqrt{\pi} you derived is why the normal distribution normalises — the curve that sits under effectively every dataset she will model, from lab errors to exam marks. One coordinate change, and the cornerstone of statistics fell out. Re-do PR3 and PR4 from a blank page tomorrow — not re-read, re-do. Computing a Jacobian and keeping its absolute value is muscle memory, built with the pencil, not by recognising a finished solution.

What's next. Chapter 12 takes the same idea up a dimension — triple integrals, where the Jacobian becomes rr (cylindrical) and ρ2sinϕ\rho^2\sin\phi (spherical). The headline mark-loser there is the dropped sinϕ\sin\phi, the three-dimensional cousin of the dropped rr.

Same material, another voice

If a different explanation would help, this one maps one-to-one onto this chapter — free, from MIT OpenCourseWare:

  • Read / watch: MIT 18.02SC, Session 53 — Change of Variables — the general Jacobian with the same u=x+y/v=xyu=x+y/v=x-y and u=xyu=xy-type examples; Sessions 54–55 cover the polar Jacobian and a worked example if you want more.