1.5.3Rotational Mechanics

Relation to linear quantities - v = rω, a_t = rα, a_c = rω²

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WHY do we even need a bridge?


Setting up: arc length is the seed of everything

WHY radians matter: the relation s=rθs = r\theta only works if θ\theta is in radians. If you used degrees, you'd need ugly factors of π/180\pi/180. Radians are designed so arc length = radius × angle, cleanly.


Deriving v=rωv = r\omega from scratch

Derivation (HOW): Start from arc length s=rθs = r\theta. For a rigid body, rr is constant in time (the point doesn't drift closer to the axis). Differentiate with respect to time: dsdt=rdθdt\frac{ds}{dt} = r\frac{d\theta}{dt} Now dsdt=v\dfrac{ds}{dt} = v (speed = rate of change of distance along the path) and dθdt=ω\dfrac{d\theta}{dt} = \omega (angular velocity). Therefore: v=rω\boxed{v = r\omega}

  • Why this step? We could differentiate because rr is constant — pull it out of the derivative. If rr changed, we'd get an extra term.
  • WHAT it means: vv is the tangential speed — it points along the circle, perpendicular to the radius.

Deriving at=rαa_t = r\alpha (tangential acceleration)

Derivation (HOW): Take v=rωv = r\omega and differentiate again (rigid body r\Rightarrow r constant): dvdt=rdωdtat=rα\frac{dv}{dt} = r\frac{d\omega}{dt} \quad\Rightarrow\quad a_t = r\alpha where α=dω/dt\alpha = d\omega/dt is the angular acceleration.

  • Why this step? ata_t is the rate of change of speed. It exists only when the rotation is speeding up or slowing down. If ω\omega is constant, α=0\alpha = 0 and at=0a_t = 0.
  • WHAT it does: ata_t changes the magnitude of velocity, not its direction.

Deriving ac=rω2a_c = r\omega^2 (centripetal acceleration)

Derivation (HOW) — first principles: Even at constant speed, a point on a circle is accelerating because its velocity direction keeps changing. Write the position vector: r=r(cosθ, sinθ),θ=ωt\vec{r} = r(\cos\theta,\ \sin\theta), \qquad \theta = \omega t Velocity (differentiate, ω\omega constant): v=rω(sinθ, cosθ)\vec{v} = r\omega(-\sin\theta,\ \cos\theta) Acceleration (differentiate again): a=rω2(cosθ, sinθ)=ω2r\vec{a} = r\omega^2(-\cos\theta,\ -\sin\theta) = -\omega^2 \vec{r} The minus sign means a\vec{a} points toward the center (opposite to r\vec r). Its magnitude: ac=rω2\boxed{a_c = r\omega^2} Using v=rωω=v/rv = r\omega \Rightarrow \omega = v/r, substitute: ac=r(v/r)2=v2/ra_c = r(v/r)^2 = v^2/r. ✓

  • Why this step? We differentiated the vector, not just the speed — that's how we captured the direction change, which is the whole source of centripetal acceleration.
Figure — Relation to linear quantities -  v = rω, a_t = rα, a_c = rω²

Dual Coding: the geometry

The diagram shows a point on a rotating disk with v\vec v tangent, at\vec a_t tangent (along/against vv), and ac\vec a_c pointing to the center. Bigger rr → longer v\vec v arrow for the same ω\omega.


Worked Examples


Forecast-then-Verify

Recall Before reading on, predict: if you double

ω\omega keeping rr fixed, by what factor do vv, ata_t (with fixed α\alpha), and aca_c change?

  • v=rωv = r\omega → doubles (×2\times 2).
  • at=rαa_t = r\alphaunchanged (doesn't depend on ω\omega at all!).
  • ac=rω2a_c = r\omega^2quadruples (×4\times 4). Did you catch that ata_t doesn't move? That's the trap.

Common Mistakes (Steel-manned)


Mnemonic


Feynman: explain to a 12-year-old

Recall Explain it simply

Picture a spinning disk like a vinyl record. Everyone on it goes around in the same time — same "turning speed." But a bug sitting near the edge has to travel a much bigger circle in that same time, so it must zoom faster than a bug near the middle. That's v=rωv = r\omega: edge bug (big rr) = fast. If the record speeds up, the bug feels a push forward — that's at=rαa_t = r\alpha. And just going in a circle, the bug always feels pulled toward the center (like being on a turning car seat) — that's ac=rω2a_c = r\omega^2, and it gets way stronger if you spin faster.


Flashcards

What is the relation between linear speed and angular speed?
v=rωv = r\omega (with ω\omega in rad/s)
Why must ω\omega be in radians for v=rωv=r\omega?
Because it comes from s=rθs=r\theta, which defines the radian (arc/radius); degrees would need extra factors.
Derive v=rωv=r\omega.
Differentiate s=rθs=r\theta with rr constant: ds/dt=rdθ/dtds/dt = r\,d\theta/dt, i.e. v=rωv = r\omega.
Two formulas for centripetal acceleration?
ac=v2/r=rω2a_c = v^2/r = r\omega^2.
What does tangential acceleration at=rαa_t=r\alpha physically change?
The magnitude (speed) of velocity, along the tangent.
What does centripetal acceleration change?
The direction of velocity; it points toward the center.
Do all points of a rigid rotating body share the same ω\omega?
Yes — ω,α,θ\omega,\alpha,\theta are common to the whole body; v,at,acv,a_t,a_c depend on rr.
If ω\omega doubles (fixed rr), how does aca_c change?
It quadruples (since acω2a_c\propto\omega^2).
How do you combine ata_t and aca_c into total acceleration?
They're perpendicular: a=at2+ac2a=\sqrt{a_t^2+a_c^2}.
At constant speed on a circle, is there acceleration?
Yes, centripetal ac=rω2a_c=r\omega^2, because direction changes.

Connections

Concept Map

same for all points

acts as dictionary

defines

differentiate in t

allows pulling r out

differentiate again

direction change

changes speed

changes direction

Angular quantities theta omega alpha

Linear quantities v at ac

Radius r

Arc length s = r theta

Radians required

v = r omega

a_t = r alpha

a_c = r omega squared

Rigid body r constant

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, jab koi rigid body ghoomti hai (jaise pankha ya disk), to uska angular part — yaani ω\omega (angular speed), α\alpha (angular acceleration), θ\theta (angle) — poore body ke liye ek hi hota hai. Center ho ya edge, sab ek hi time mein same angle ghoomte hain. Lekin har point ek circle banata hai, aur uski linear speed alag hoti hai. Edge wala point bahut tezi se ghoomta hai, center wala dheere. Yeh difference radius rr ki wajah se aata hai: v=rωv = r\omega. Jitna door axis se, utni zyada speed.

v=rωv=r\omega kaise aaya? Simple — arc length s=rθs = r\theta se. Time ke saath differentiate karo (kyunki rigid body mein rr constant rehta hai), to v=rωv = r\omega mil jaata hai. Phir wahi cheez dobara differentiate karo to at=rαa_t = r\alpha — yeh tangential acceleration hai jo speed ko badalta hai (sirf jab body tez ya dheere ho rahi ho). Yaad rakho: ω\omega hamesha radians mein, degrees mein nahi!

Ab ek interesting baat — circle pe chalte waqt, even agar speed constant ho, tab bhi acceleration hota hai! Kyunki velocity ek vector hai aur uski direction badal rahi hai. Yeh hai centripetal acceleration ac=rω2=v2/ra_c = r\omega^2 = v^2/r, jo hamesha center ki taraf point karta hai. Position vector ko do baar differentiate karoge to a=ω2r\vec a = -\omega^2 \vec r — minus sign matlab center ki taraf.

Yeh chize kyun important hai? Kyunki Newton ke laws, force, energy — sab linear language mein hain, par rotation angular language mein. rr inn dono ke beech ka translator hai. Exam tip: aca_c mein ω\omega ki power 2 hoti hai, isliye ω\omega double karo to aca_c char guna ho jaata hai — yeh trap hai, dhyan rakhna!

Go deeper — visual, from zero

Test yourself — Rotational Mechanics

Connections