WHY a cross product? Because only the part of the motion that "goes around" the origin counts. Motion straight toward or away fromO produces zero turning — and the cross product automatically kills the parallel component.
∣L∣=rpsinθ=p⋅(rsinθ)=p⋅r⊥
where r⊥=rsinθ is the perpendicular distance (the "lever arm") from O to the line of motion.
Setup. Take a rigid body rotating about a fixed axis (say the z-axis). Pick particle i at perpendicular distance ri from the axis. Since it's rigid, every particle has the same angular speed ω.
Step 1 — speed of particle i. It travels in a circle of radius ri, so
vi=ωri.Why this step? For circular motion, tangential speed = radius × angular speed.
Step 2 — its momentum is tangential, pi=mivi=miωri. The velocity is perpendicular to the radius vector from the axis, so θ=90∘ and sinθ=1.
Step 3 — its angular momentum about the axis.Li,z=ripisin90∘=ri(miωri)=miri2ω.Why this step? We use the component along the axis, which is the physically conserved/relevant one for fixed-axis spin.
Step 4 — sum over all particles (the axis component adds up):
Lz=∑imiri2ω=(∑imiri2)ω.
Step 5 — recognise the bracket as the moment of inertiaI=∑imiri2:
vi=ωri, then Li=miri2ω, sum gives L=(∑miri2)ω
Why I appears
I=∑miri2 is the moment of inertia about the axis
When is L=Iω valid
rigid body about a fixed/symmetry axis only
Units of angular momentum
kgm2s−1=Js
Relation between torque and L
τext=dL/dt
Condition for conservation of L
net external torque =0
Skater spin-up explanation
I1ω1=I2ω2; smaller I ⇒ larger ω
Is L always parallel to ω?
No — only for principal/symmetry axes; in general I is a tensor
Recall Feynman: explain to a 12-year-old
Imagine spinning on a swivel chair holding heavy books with your arms stretched out. You're turning slowly. Now pull the books to your chest — you suddenly spin faster, like magic! Nothing pushed you; you just moved the weight closer to the middle. "Angular momentum" is the spinning version of how-hard-it-is-to-stop. Nature keeps it the same number when nobody twists you from outside. Bring the weight in (small spread = small I) and to keep the number the same, the spin speed ω jumps up. Stretch out again and you slow down. That single rule explains skaters, divers, and even why planets sweep faster when close to the Sun.
Dekho, angular momentum basically "ghoomne wali cheez ko rokna kitna mushkil hai" ka measure hai — jaise linear momentum p=mv seedhi line wali motion ke liye hota hai. Single particle ke liye general definition hai L=r×p. Yahan cross product isliye aata hai kyunki sirf wahi motion count hoti hai jo origin ke "around" ghoom rahi hai. Agar particle seedha origin ki taraf ja raha hai to koi swirl nahi, L=0. Magnitude nikalo to L=pr⊥, jahan r⊥ lever arm (perpendicular distance) hai — yaad rakho, full r mat use karo, sirf perpendicular part.
Ab L=Iω koi alag formula nahi hai — yeh wahi r×p hai jo rigid body ke har particle pe sum kiya gaya hai. Har particle ka vi=ωri, uska Li=miri2ω, sabko jod do to bracket me ∑miri2 ban jaata hai jise hum moment of inertiaI bolte hain. Bas, L=Iω ready! Lekin yeh sirf tab valid hai jab axis fixed/symmetry axis ho.
Sabse mast application: conservation. Agar bahar se koi torque nahi (τext=0), to L constant rehta hai. Isliye skater jab apne haath andar khinchti hai, uska I chhota ho jaata hai, aur ω tezi se badh jaata hai — I1ω1=I2ω2. Energy conserve nahi hoti (muscles kaam karti hain), par L conserve hota hai. Yahi rule planets, divers, sab pe lagta hai. Exam me bas yaad rakho: r⊥ use karo, axis check karo, aur torque zero hai to L same.