Intuition The one-line idea
A triple integral ∭ E f d V \iiint_E f\,dV ∭ E f d V adds up the value of f f f over every tiny chunk d V dV d V of a 3D region E E E . The whole game is: (1) chop the region into boxes, (2) pick coordinates that make the boxes and the region easy to describe. ==Cartesian= straight walls=, ==cylindrical= round in one plane + straight axis=, ==spherical= round in all directions=.
Definition Triple integral (Riemann definition)
Partition a solid E E E into N N N tiny boxes of volume Δ V k \Delta V_k Δ V k , pick a sample point ( x k ∗ , y k ∗ , z k ∗ ) (x_k^*,y_k^*,z_k^*) ( x k ∗ , y k ∗ , z k ∗ ) in each, and form
∭ E f ( x , y , z ) d V = lim N → ∞ ∑ k = 1 N f ( x k ∗ , y k ∗ , z k ∗ ) Δ V k . \iiint_E f(x,y,z)\,dV \;=\; \lim_{N\to\infty}\sum_{k=1}^{N} f(x_k^*,y_k^*,z_k^*)\,\Delta V_k. ∭ E f ( x , y , z ) d V = lim N → ∞ ∑ k = 1 N f ( x k ∗ , y k ∗ , z k ∗ ) Δ V k .
WHAT it computes:
If f = 1 f=1 f = 1 : ∭ E d V = Volume ( E ) \iiint_E dV = \text{Volume}(E) ∭ E d V = Volume ( E ) .
If f = ρ ( x , y , z ) f=\rho(x,y,z) f = ρ ( x , y , z ) (density): ∭ E ρ d V = Mass \iiint_E \rho\,dV = \text{Mass} ∭ E ρ d V = Mass .
General f f f : total "amount" of a quantity distributed in space.
WHY it converges to something useful: each term f ⋅ Δ V k f\cdot\Delta V_k f ⋅ Δ V k = (value)×(little volume) = a little "amount". Summing all little amounts and refining the mesh gives the total exactly — same logic as a 1D area sum, lifted to 3D.
HOW to set the limits (the only skill that matters):
Innermost (z z z ): freeze x , y x,y x , y . Shoot a vertical arrow up. It enters E E E at z = z 1 ( x , y ) z=z_1(x,y) z = z 1 ( x , y ) and exits at z = z 2 ( x , y ) z=z_2(x,y) z = z 2 ( x , y ) . These (functions of x , y x,y x , y ) are the inner limits.
Middle (y y y ): project the shadow of E E E onto the x y xy x y -plane. Sweep y y y between the boundary curves y 1 ( x ) , y 2 ( x ) y_1(x),y_2(x) y 1 ( x ) , y 2 ( x ) .
Outer (x x x ): the constant range [ x 1 , x 2 ] [x_1,x_2] [ x 1 , x 2 ] covering the shadow.
Common mistake "Why are my outer limits functions of the inner variable?"
It feels natural to write ∫ 0 x … d x \int_0^x \dots dx ∫ 0 x … d x . The fix: outer limits must be constants , and each limit may only depend on variables outside it. Reason: you integrate inside-out; by the time you hit the outer integral, all other variables are gone, so a number is all that's left.
Worked example Volume of the tetrahedron
x , y , z ≥ 0 , x + y + z ≤ 1 x,y,z\ge 0,\; x+y+z\le 1 x , y , z ≥ 0 , x + y + z ≤ 1
Step 1 — inner z z z . Arrow up: enters z = 0 z=0 z = 0 , exits the plane z = 1 − x − y z=1-x-y z = 1 − x − y . Why? The slanted face is x + y + z = 1 x+y+z=1 x + y + z = 1 .
∫ 0 1 − x − y d z = 1 − x − y \int_0^{1-x-y} dz = 1-x-y ∫ 0 1 − x − y d z = 1 − x − y
Step 2 — middle y y y . Shadow on x y xy x y -plane is the triangle x , y ≥ 0 , x + y ≤ 1 x,y\ge0,\,x+y\le1 x , y ≥ 0 , x + y ≤ 1 , so y y y runs 0 → 1 − x 0\to 1-x 0 → 1 − x . Why? Set z = 0 z=0 z = 0 in the constraint.
∫ 0 1 − x ( 1 − x − y ) d y = [ ( 1 − x ) y − y 2 2 ] 0 1 − x = ( 1 − x ) 2 2 \int_0^{1-x}(1-x-y)\,dy = \Big[(1-x)y-\tfrac{y^2}{2}\Big]_0^{1-x}=\tfrac{(1-x)^2}{2} ∫ 0 1 − x ( 1 − x − y ) d y = [ ( 1 − x ) y − 2 y 2 ] 0 1 − x = 2 ( 1 − x ) 2
Step 3 — outer x x x : x : 0 → 1 x:0\to1 x : 0 → 1 .
∫ 0 1 ( 1 − x ) 2 2 d x = 1 2 ⋅ 1 3 = 1 6 \int_0^1 \tfrac{(1-x)^2}{2}\,dx = \tfrac12\cdot\tfrac{1}{3}=\boxed{\tfrac16} ∫ 0 1 2 ( 1 − x ) 2 d x = 2 1 ⋅ 3 1 = 6 1
Sanity check: a tetra with three perpendicular edges of length 1 has volume 1 6 \tfrac16 6 1 . ✓
d V dV d V must carry a stretch factor
When you switch from ( x , y , z ) (x,y,z) ( x , y , z ) to new coords ( u , v , w ) (u,v,w) ( u , v , w ) , a tiny coordinate box d u d v d w du\,dv\,dw d u d v d w maps to a warped parallelepiped. Its volume = (volume of the box) × (local stretch). That stretch is ∣ J ∣ |J| ∣ J ∣ , the Jacobian determinant .
x = r cos θ , y = r sin θ , z = z , r ≥ 0 , 0 ≤ θ < 2 π . x=r\cos\theta,\quad y=r\sin\theta,\quad z=z,\qquad r\ge0,\ 0\le\theta<2\pi. x = r cos θ , y = r sin θ , z = z , r ≥ 0 , 0 ≤ θ < 2 π .
Use it when: the region or integrand has rotational symmetry about an axis (cylinders, cones, paraboloids).
Worked example Volume of cylinder
r ≤ a r\le a r ≤ a , 0 ≤ z ≤ h 0\le z\le h 0 ≤ z ≤ h
=\int_0^{2\pi}\!\!d\theta\int_0^a r\,dr\int_0^h dz
=2\pi\cdot\tfrac{a^2}{2}\cdot h=\pi a^2 h.\ \checkmark$$
**Why split into a product?** Limits are all constants and the integrand factors, so Fubini lets us multiply 1D integrals.
x = ρ sin ϕ cos θ , y = ρ sin ϕ sin θ , z = ρ cos ϕ , x=\rho\sin\phi\cos\theta,\quad y=\rho\sin\phi\sin\theta,\quad z=\rho\cos\phi, x = ρ sin ϕ cos θ , y = ρ sin ϕ sin θ , z = ρ cos ϕ ,
with ρ ≥ 0 \rho\ge0 ρ ≥ 0 (distance from origin), 0 ≤ ϕ ≤ π 0\le\phi\le\pi 0 ≤ ϕ ≤ π (angle from + z +z + z axis), 0 ≤ θ < 2 π 0\le\theta<2\pi 0 ≤ θ < 2 π (around z z z ).
Common mistake Forgetting
sin ϕ \sin\phi sin ϕ (or writing sin θ \sin\theta sin θ )
It feels like by analogy with cylindrical you only need one extra factor. Fix: there are two angular arc-lengths in spherical. The latitude circles shrink to points at the poles (ϕ = 0 , π \phi=0,\pi ϕ = 0 , π ), and sin ϕ → 0 \sin\phi\to0 sin ϕ → 0 encodes exactly that shrinking. Use ϕ \phi ϕ (polar angle), never θ \theta θ .
Worked example Volume of a ball of radius
a a a
=\underbrace{\int_0^{2\pi}d\theta}_{2\pi}\;\underbrace{\int_0^\pi\sin\phi\,d\phi}_{2}\;\underbrace{\int_0^a\rho^2 d\rho}_{a^3/3}
=2\pi\cdot2\cdot\tfrac{a^3}{3}=\tfrac{4}{3}\pi a^3.\ \checkmark$$
**Why this is the 80/20 example:** it simultaneously checks all three factors and lands on the famous $\frac43\pi a^3$.
∭ E z d V \iiint_E z\,dV ∭ E z d V over the upper half ball ρ ≤ a , z ≥ 0 \rho\le a,\ z\ge0 ρ ≤ a , z ≥ 0
z = ρ cos ϕ z=\rho\cos\phi z = ρ cos ϕ , and z ≥ 0 ⇒ ϕ ∈ [ 0 , π / 2 ] z\ge0\Rightarrow \phi\in[0,\pi/2] z ≥ 0 ⇒ ϕ ∈ [ 0 , π /2 ] .
∫ 0 2 π ∫ 0 π / 2 ∫ 0 a ( ρ cos ϕ ) ρ 2 sin ϕ d ρ d ϕ d θ \int_0^{2\pi}\!\!\int_0^{\pi/2}\!\!\int_0^a (\rho\cos\phi)\,\rho^2\sin\phi\,d\rho\,d\phi\,d\theta ∫ 0 2 π ∫ 0 π /2 ∫ 0 a ( ρ cos ϕ ) ρ 2 sin ϕ d ρ d ϕ d θ
Step why: integrand becomes ρ 3 cos ϕ sin ϕ \rho^3\cos\phi\sin\phi ρ 3 cos ϕ sin ϕ .
=2\pi\cdot\tfrac12\cdot\tfrac{a^4}{4}=\tfrac{\pi a^4}{4}.$$
Used $\int_0^{\pi/2}\sin\phi\cos\phi\,d\phi=\tfrac12$.
Region / symmetry
Best coords
d V dV d V
Box, planes, slanted faces
Cartesian
d x d y d z dx\,dy\,dz d x d y d z
Circle/cylinder/cone/paraboloid about an axis
Cylindrical
r d r d θ d z r\,dr\,d\theta\,dz r d r d θ d z
Sphere, ball, x 2 + y 2 + z 2 x^2+y^2+z^2 x 2 + y 2 + z 2 in integrand
Spherical
ρ 2 sin ϕ d ρ d ϕ d θ \rho^2\sin\phi\,d\rho\,d\phi\,d\theta ρ 2 sin ϕ d ρ d ϕ d θ
Common mistake Using Cartesian on a sphere
It feels safe (no Jacobian to remember). But limits like z = ± a 2 − x 2 − y 2 z=\pm\sqrt{a^2-x^2-y^2} z = ± a 2 − x 2 − y 2 create ugly nested square roots. Fix: if you see x 2 + y 2 + z 2 x^2+y^2+z^2 x 2 + y 2 + z 2 , go spherical — the boundary becomes the single constant ρ = a \rho=a ρ = a .
Recall Test yourself (hide answers)
What is d V dV d V in each coordinate system?
Where does the r r r in cylindrical come from, geometrically?
Why ρ 2 sin ϕ \rho^2\sin\phi ρ 2 sin ϕ and not ρ 2 \rho^2 ρ 2 ?
Why must outer limits be constants?
Recall Feynman: explain to a 12-year-old
Imagine filling a shape with tiny sugar cubes and counting how much "stuff" (sweetness) is in each cube. Add them all up — that's a triple integral. If the shape is a box, use square cubes (Cartesian). If it's a tin can, slice it into curved tiles that fan out — the tiles far from the center are wider , so we multiply by how far out they are (r r r ). If it's a ball, the tiles also get shorter near the top and bottom poles, so we multiply by sin ϕ \sin\phi sin ϕ too. The extra multipliers just make sure we don't pretend warped tiles are the same size as flat ones.
d V dV d V factors
"Cylinders carry ONE r r r , Spheres squeeze with ρ 2 sin ϕ \rho^2\sin\phi ρ 2 sin ϕ ."
Spherical mantra: "rho-squared sine-phi" — two ρ \rho ρ 's (radial + two arcs) and the sin ϕ \sin\phi sin ϕ that kills the poles .
What is d V dV d V in Cartesian coordinates? What is d V dV d V in cylindrical coordinates? r d r d θ d z r\,dr\,d\theta\,dz r d r d θ d z What is d V dV d V in spherical coordinates? ρ 2 sin ϕ d ρ d ϕ d θ \rho^2\sin\phi\,d\rho\,d\phi\,d\theta ρ 2 sin ϕ d ρ d ϕ d θ Why does the cylindrical Jacobian equal r r r ? A polar pixel has area
r d r d θ r\,dr\,d\theta r d r d θ (arc length
r d θ r\,d\theta r d θ times width
d r dr d r ); times
d z dz d z gives volume.
Why does spherical d V dV d V contain sin ϕ \sin\phi sin ϕ ? The latitude-circle arc has radius
ρ sin ϕ \rho\sin\phi ρ sin ϕ , so its arc length is
ρ sin ϕ d θ \rho\sin\phi\,d\theta ρ sin ϕ d θ ; this shrinks to 0 at the poles.
In spherical coords, what are the ranges of ρ , ϕ , θ \rho,\phi,\theta ρ , ϕ , θ ? ρ ≥ 0 \rho\ge0 ρ ≥ 0 ,
0 ≤ ϕ ≤ π 0\le\phi\le\pi 0 ≤ ϕ ≤ π (polar, from
+ z +z + z ),
0 ≤ θ < 2 π 0\le\theta<2\pi 0 ≤ θ < 2 π (azimuth).
Volume of a ball of radius a a a via spherical integral? ∫ 0 2 π ∫ 0 π ∫ 0 a ρ 2 sin ϕ d ρ d ϕ d θ = 4 3 π a 3 \int_0^{2\pi}\!\int_0^\pi\!\int_0^a \rho^2\sin\phi\,d\rho\,d\phi\,d\theta=\frac43\pi a^3 ∫ 0 2 π ∫ 0 π ∫ 0 a ρ 2 sin ϕ d ρ d ϕ d θ = 3 4 π a 3 .
Volume of cylinder radius a a a , height h h h ? ∫ 0 2 π ∫ 0 a ∫ 0 h r d z d r d θ = π a 2 h \int_0^{2\pi}\!\int_0^a\!\int_0^h r\,dz\,dr\,d\theta=\pi a^2 h ∫ 0 2 π ∫ 0 a ∫ 0 h r d z d r d θ = π a 2 h .
How do you choose the innermost (z z z ) Cartesian limits? Freeze
x , y x,y x , y , shoot a vertical arrow: it enters at
z 1 ( x , y ) z_1(x,y) z 1 ( x , y ) and exits at
z 2 ( x , y ) z_2(x,y) z 2 ( x , y ) .
Why must the outermost integration limits be constants? You integrate inside-out; by the outer step all other variables are gone, so only numbers remain.
When should you prefer spherical coordinates? When the region is a sphere/ball or the integrand contains
x 2 + y 2 + z 2 = ρ 2 x^2+y^2+z^2=\rho^2 x 2 + y 2 + z 2 = ρ 2 .
General change-of-variables formula for d V dV d V ? d V = ∣ det ∂ ( x , y , z ) / ∂ ( u , v , w ) ∣ d u d v d w dV=\left|\det\partial(x,y,z)/\partial(u,v,w)\right|\,du\,dv\,dw d V = ∣ det ∂ ( x , y , z ) / ∂ ( u , v , w ) ∣ d u d v d w .
What does ∭ E 1 d V \iiint_E 1\,dV ∭ E 1 d V compute? Cartesian-to-spherical: what is z z z ? z = ρ cos ϕ z=\rho\cos\phi z = ρ cos ϕ .
Triple integral iiint f dV
Vertical arrow enter exit
Intuition Hinglish mein samjho
Triple integral ka matlab simple hai: kisi 3D shape ke andar har chhote cube ka "amount" (jaise density ya bas volume) nikaalo aur sabko jod do. Jaise 1D mein area aur 2D mein double integral, waise hi 3D mein hum poore solid ko tiny boxes mein todte hain, har box ka contribution f ⋅ d V f\cdot dV f ⋅ d V lete hain, aur infinite chhote boxes ka sum lete hain. Agar f = 1 f=1 f = 1 rakho to seedha volume mil jaata hai.
Asli skill hai sahi coordinate choose karna. Agar shape ke walls seedhe hain (box, slanted planes) to Cartesian best — d V = d x d y d z dV=dx\,dy\,dz d V = d x d y d z , aur limits aise lagao: inner z z z ke liye ek arrow upar maaro, jahan enter kare wahan se jahan exit kare. Outer limits hamesha constant hone chahiye, yeh galti sabse zyada hoti hai. Agar shape kisi axis ke around round hai (cylinder, cone) to cylindrical use karo, aur yaad rakho ek extra r r r aata hai — kyunki door wali wedge t