Physics Lab

Unit 5: Rotational Mechanics

Rotational mechanics is the single highest-yield topic in JEE Advanced mechanics, often supplying a multi-part problem worth 8–12 marks. JEE Main typically has 2–3 questions on moment of inertia, rolling motion, angular momentum conservation. The unit synthesizes everything from earlier units (forces, energy, momentum) with the new concept of rotation.

Typical question types:

  • JEE Main: moment of inertia of standard bodies (with parallel/perpendicular axis theorems), pure rolling down an incline, angular momentum conservation (skater, planet).
  • JEE Advanced: rotational collisions (bullet stuck in hinged rod), rolling with slipping, instantaneous axis of rotation, toppling vs sliding, combined translation + rotation problems.

Concept Map

  • Centre of Mass
    • Discrete systems
    • Continuous bodies (rod, arc, plate, hemisphere)
    • Properties (motion of CM, external forces only)
  • Rotational Kinematics
    • ω,α\omega, \alpha; analogues of linear motion
    • Rotation about fixed axis
  • Moment of Inertia (MoI)
    • Definition, standard bodies (with derivations)
    • Parallel & perpendicular axis theorems
    • Radius of gyration
  • Torque and Angular Momentum
    • Definitions; relation τ⃗=dL⃗/dt\vec\tau = d\vec L/dt
    • Conservation of angular momentum
  • Combined Translation + Rotation
    • Pure rolling condition; KE decomposition
    • Rolling on incline; slipping vs rolling
    • Direction of friction in rolling
  • Instantaneous Axis of Rotation
  • Angular Momentum about a Point (for a moving particle)
  • Toppling vs Sliding
  • Rotational Collisions

Topic 1: Centre of Mass

Sub-topic A: Discrete systems

For nn particles at positions r⃗i\vec r_i with masses mim_i:

R⃗cm=∑mir⃗iM,M=∑mi.\vec R_{cm} = \frac{\sum m_i \vec r_i}{M},\quad M = \sum m_i.

If F⃗ext\vec F_{ext} is the net external force, F⃗ext=Ma⃗cm\vec F_{ext} = M\vec a_{cm}. Internal forces (e.g. those in a collision) cancel pairwise (Newton's third law).

Sub-topic B: Continuous bodies — derivations

Uniform rod (length LL, mass MM). Choose origin at one end. Linear mass density λ=M/L\lambda = M/L.

xcm=1M∫0Lx λ dx=1M⋅λL22=L2.x_{cm} = \frac{1}{M}\int_0^L x\,\lambda\,dx = \frac{1}{M}\cdot\lambda\frac{L^2}{2} = \frac{L}{2}.

So CM at the midpoint. (For a rod of varying density λ(x)\lambda(x), the integral gives a different location.)

Semicircular wire (radius RR, uniform). Parametrize θ∈[0,π]\theta\in[0,\pi], x=Rcos⁡θx=R\cos\theta, y=Rsin⁡θy=R\sin\theta, ds=R dθds = R\,d\theta. Linear density λ=M/(πR)\lambda = M/(\pi R).

ycm=1M∫0πRsin⁡θ⋅λR dθ=R2λM∫0πsin⁡θ dθ=R2πR⋅2=2Rπ.y_{cm} = \frac{1}{M}\int_0^\pi R\sin\theta\cdot \lambda R\,d\theta = \frac{R^2\lambda}{M}\int_0^\pi \sin\theta\,d\theta = \frac{R^2}{\pi R}\cdot 2 = \frac{2R}{\pi}.

xcm=0x_{cm} = 0 by symmetry. So CM is at (0,2R/π)(0, 2R/\pi).

Semicircular disc (radius RR, mass MM). σ=M/(12πR2)\sigma = M/(\tfrac12\pi R^2). Use strips parallel to the diameter at height yy width dydy, length 2R2−y22\sqrt{R^2-y^2}:

ycm=1M∫0Ry⋅σ⋅2R2−y2 dy.y_{cm} = \frac{1}{M}\int_0^R y\cdot \sigma\cdot 2\sqrt{R^2-y^2}\,dy.

Let u=R2−y2u = R^2-y^2, du=−2y dydu = -2y\,dy, y dy=−du/2y\,dy = -du/2:

ycm=2σM∫R20u⋅(−12)du=σM∫0R2u du=σM⋅23R3=2R3σ3M.y_{cm} = \frac{2\sigma}{M}\int_{R^2}^0 \sqrt u\cdot(-\tfrac12)du = \frac{\sigma}{M}\int_0^{R^2}\sqrt u\,du = \frac{\sigma}{M}\cdot\frac{2}{3}R^3 = \frac{2R^3 \sigma}{3M}.

With σ=2M/(πR2)\sigma = 2M/(\pi R^2):

ycm=2R33M⋅2MπR2=4R3π.y_{cm} = \frac{2R^3}{3M}\cdot\frac{2M}{\pi R^2} = \frac{4R}{3\pi}.

Triangular plate (uniform). CM at the centroid: (x1+x2+x3)/3,(y1+y2+y3)/3(x_1+x_2+x_3)/3, (y_1+y_2+y_3)/3.

Hemispherical solid (radius RR, mass MM). Use shells of radius rr, thickness drdr... or disks of radius R2−y2\sqrt{R^2-y^2} at height yy.

Volume element: disk of radius R2−y2\sqrt{R^2-y^2}, area π(R2−y2)\pi(R^2-y^2), thickness dydy. ρ=M/(23πR3)\rho = M/(\tfrac23\pi R^3).

ycm=1M∫0Ry⋅ρπ(R2−y2) dy=ρπM∫0R(R2y−y3)dy=ρπM⋅R44.y_{cm} = \frac{1}{M}\int_0^R y\cdot \rho\pi(R^2-y^2)\,dy = \frac{\rho\pi}{M}\int_0^R(R^2 y - y^3)dy = \frac{\rho\pi}{M}\cdot\frac{R^4}{4}.

=πR4/4(2πR3/3)=3R8.= \frac{\pi R^4/4}{(2\pi R^3/3)} = \frac{3R}{8}.

Hemispherical shell (thin, radius RR, mass MM). Use rings at height yy width R dθR\,d\theta at polar angle θ\theta:

y=Rcos⁡θy = R\cos\theta, ring radius Rsin⁡θR\sin\theta, area = 2πRsin⁡θ⋅R dθ=2πR2sin⁡θ dθ2\pi R\sin\theta\cdot R\,d\theta = 2\pi R^2\sin\theta\,d\theta.

σ=M/(2πR2)\sigma = M/(2\pi R^2).

ycm=1M∫0π/2Rcos⁡θ⋅σ⋅2πR2sin⁡θ dθ=2πR3σM∫0π/2sin⁡θcos⁡θ dθ=2πR3σM⋅12=πR3σM.y_{cm} = \frac{1}{M}\int_0^{\pi/2} R\cos\theta\cdot \sigma\cdot 2\pi R^2\sin\theta\,d\theta = \frac{2\pi R^3\sigma}{M}\int_0^{\pi/2}\sin\theta\cos\theta\,d\theta = \frac{2\pi R^3\sigma}{M}\cdot \frac{1}{2}=\frac{\pi R^3\sigma}{M}.

=πR3⋅M/(2πR2M)=R/2= \pi R^3\cdot M/(2\pi R^2 M) = R/2.

Sub-topic C: Centre of mass with cavity

If a body of mass MM has a cavity (small piece removed), treat the cavity as a negative mass and use the formula for the CM of two objects.

R⃗cm(body with cavity)=MR⃗cm(full)−mR⃗cm(cavity)M−m.\vec R_{cm}^{(\text{body with cavity})} = \frac{M\vec R_{cm}^{(\text{full})} - m\vec R_{cm}^{(\text{cavity})}}{M - m}.

Sub-topic D: Motion of CM

F⃗ext=Ma⃗cm,P⃗sys=Mv⃗cm.\vec F_{ext} = M\vec a_{cm},\quad \vec P_{sys} = M\vec v_{cm}.

Internal forces don't affect CM motion. Example: when a shell explodes in mid-air, its CM continues on the original projectile trajectory.

Worked Examples (JEE Main level)

Example 1.1. Find CM of a system of three particles at (0,0)(0,0), (1,0)(1,0), (0,1)(0,1) m, masses 1,2,31, 2, 3 kg.

xcm=(0+2+0)/6=1/3x_{cm} = (0+2+0)/6 = 1/3. ycm=(0+0+3)/6=1/2y_{cm} = (0+0+3)/6 = 1/2. So (1/3,1/2)(1/3, 1/2) m.

Example 1.2. A uniform disc of radius RR has a circular hole of radius R/2R/2 centred at R/2R/2 from the centre. Find the CM of the remainder.

Treat hole as negative mass. Original CM at 00 with mass MM. Hole mass M/4M/4 (area ratio 14\tfrac14). Hole CM at R/2R/2.

xcm=M⋅0−(M/4)(R/2)M−M/4=−MR/83M/4=−R6.x_{cm} = \frac{M\cdot 0 - (M/4)(R/2)}{M - M/4} = \frac{-MR/8}{3M/4} = -\frac{R}{6}.

(Opposite side of the hole, distance R/6R/6 from centre.)

Worked Examples (JEE Advanced level)

Example 1.A1. A boat of mass MM and length LL is at rest on still water. A man of mass mm walks from one end to the other. Displacement of the boat (no friction with water)?

CM stays put (no external horizontal force). Let boat shift by xx. Man's displacement in ground frame: L−xL - x (in opposite direction effectively, but let's set up coords: man moves +ı^+\hat\imath in the boat by LL, boat moves −ı^-\hat\imath by xx, so man's ground displacement is L−xL - x.)

0=m(L−x)+M(−x)⇒x=mLm+M.0 = m(L - x) + M(-x)\Rightarrow x = \dfrac{mL}{m+M}.


Topic 2: Rotational Kinematics

Sub-topic A: Definitions

For rotation about a fixed axis:

  • θ(t)\theta(t) = angular position, ω=dθ/dt\omega = d\theta/dt, α=dω/dt=d2θ/dt2\alpha = d\omega/dt = d^2\theta/dt^2.
  • Linear quantities for a point at distance rr from axis: v=rωv = r\omega, at=rαa_t = r\alpha, ac=rω2a_c = r\omega^2.

Sub-topic B: Constant α\alpha equations

ω=ω0+αt,θ=ω0t+12αt2,ω2=ω02+2αθ.\omega = \omega_0 + \alpha t,\quad \theta = \omega_0 t + \tfrac12\alpha t^2,\quad \omega^2 = \omega_0^2 + 2\alpha\theta.

Analogous to linear kinematics.

Worked Examples (JEE Main level)

Example 2.1. A wheel starts from rest with α=2\alpha = 2 rad/s². Angular speed after 55 s and angle covered?

ω=10\omega = 10 rad/s. θ=12⋅2⋅25=25\theta = \tfrac12\cdot 2\cdot 25 = 25 rad.


Topic 3: Moment of Inertia

Sub-topic A: Definition

For a system of particles, the moment of inertia about an axis is

I=∑miri2,orI=∫r2 dm,I = \sum m_i r_i^2,\quad\text{or}\quad I = \int r^2\,dm,

where rir_i is the perpendicular distance from particle ii to the axis.

Sub-topic B: Derivations for standard bodies

1. Thin rod, axis through centre perpendicular to length.

λ=M/L\lambda = M/L. I=∫−L/2L/2x2λ dx=λ⋅23(L/2)3=ML212.I = \int_{-L/2}^{L/2} x^2 \lambda\,dx = \lambda\cdot \tfrac{2}{3}(L/2)^3 = \dfrac{ML^2}{12}.

2. Thin rod, axis through one end perpendicular.

I=∫0Lx2λ dx=ML23I = \int_0^L x^2\lambda\,dx = \dfrac{ML^2}{3}. (Or via parallel axis: ML2/12+M(L/2)2=ML2/3ML^2/12 + M(L/2)^2 = ML^2/3.)

3. Thin ring, axis through centre perpendicular.

All mass at distance RR: I=MR2I = MR^2.

4. Disc, axis through centre perpendicular.

Use rings of radius rr width drdr. dm=σ⋅2πr drdm = \sigma\cdot 2\pi r\,dr, σ=M/(πR2)\sigma = M/(\pi R^2). I=∫0Rr2⋅σ2πr dr=2πσR4/4=MR22.I = \int_0^R r^2\cdot \sigma 2\pi r\,dr = 2\pi\sigma R^4/4 = \dfrac{MR^2}{2}.

5. Disc, axis along a diameter.

By perpendicular axis theorem: Iz=Ix+IyI_z = I_x + I_y. By symmetry Ix=IyI_x = I_y. So Id=Iz/2=MR2/4I_d = I_z/2 = MR^2/4.

6. Solid sphere, axis through centre.

Use spherical shells of radius rr thickness drdr. Mass dm=4πr2ρ drdm = 4\pi r^2 \rho\,dr. MoI of a thin spherical shell about its diameter is 23mr2\tfrac23 m r^2.

Total: I=∫0R23⋅4πr2ρ⋅r2 dr=8πρ3⋅R5/5=8πR515ρI = \int_0^R \tfrac23\cdot 4\pi r^2\rho\cdot r^2\,dr = \tfrac{8\pi\rho}{3}\cdot R^5/5 = \tfrac{8\pi R^5}{15}\rho.

With ρ=3M/(4πR3)\rho = 3M/(4\pi R^3): I=8πR515⋅3M4πR3=2MR25.I = \tfrac{8\pi R^5}{15}\cdot \tfrac{3M}{4\pi R^3} = \dfrac{2MR^2}{5}.

7. Thin spherical shell, axis through centre.

I=23MR2I = \tfrac{2}{3}MR^2.

(Quick derivation: use rings at polar angle θ\theta, radius Rsin⁡θR\sin\theta, mass dm=σ⋅2πRsin⁡θ⋅R dθdm = \sigma\cdot 2\pi R\sin\theta\cdot R\,d\theta. MoI of ring about axis =dm⋅R2sin⁡2θ= dm\cdot R^2\sin^2\theta. Integrate over θ∈[0,π]\theta\in[0,\pi].)

8. Cylinder (solid, length LL, radius RR), axis along length.

Like a disc: I=MR2/2I = MR^2/2.

9. Hollow cylinder (thin, radius RR), axis along length.

I=MR2I = MR^2.

10. Rectangular plate (a×ba\times b, mass MM), axis through CM perpendicular to plane.

By perp. axis: Iz=Ix+Iy=Mb2/12+Ma2/12=M(a2+b2)/12I_z = I_x + I_y = M b^2/12 + M a^2/12 = M(a^2+b^2)/12.

Sub-topic C: Theorems

Parallel axis theorem. If IcmI_{cm} is MoI about an axis through the CM, then MoI about a parallel axis at distance dd is

I=Icm+Md2.I = I_{cm} + Md^2.

Perpendicular axis theorem (for plane laminas). For a plane lamina, MoI about an axis perpendicular to the plane equals the sum of MoIs about two perpendicular axes in the plane intersecting at the same point:

Iz=Ix+Iy.I_z = I_x + I_y.

Sub-topic D: Radius of gyration

I=Mk2I = M k^2 defines the radius of gyration kk. For a solid sphere, k=R2/5k = R\sqrt{2/5}.

Worked Examples (JEE Main level)

Example 3.1. MoI of a rod (L=1L=1 m, M=2M=2 kg) about an axis through one end perpendicular?

I=ML2/3=2/3I = ML^2/3 = 2/3 kg·m².

Example 3.2. MoI of a uniform disc of mass MM and radius RR about an axis tangent to the disc in its plane?

Through diameter: MR2/4MR^2/4. Parallel axis (distance RR): I=MR2/4+MR2=5MR2/4I = MR^2/4 + MR^2 = 5MR^2/4.

Example 3.3. MoI of a thin ring about a tangent in its plane?

Diameter: MR2/2MR^2/2 (by perp. axis, Iz=MR2=Ix+Iy=2Ix⇒Ix=MR2/2I_z=MR^2=I_x+I_y=2I_x\Rightarrow I_x = MR^2/2). Tangent: MR2/2+MR2=3MR2/2MR^2/2 + MR^2 = 3MR^2/2.

Worked Examples (JEE Advanced level)

Example 3.A1. A uniform rod of length LL and mass MM has MoI I0I_0 about a perpendicular axis through one end. A small mass mm is added at the other end. New MoI?

I0=ML2/3I_0 = ML^2/3. With added mass: I=ML2/3+mL2I = ML^2/3 + mL^2.

Example 3.A2. MoI of a uniform solid cone (semi-vertical angle α\alpha, height hh, mass MM) about its axis.

Volume element: disc at height zz from apex, radius ztan⁡αz\tan\alpha, thickness dzdz.

dV=πz2tan⁡2α dzdV = \pi z^2\tan^2\alpha\,dz. ρ=M/V=M/(13πh3tan⁡2α)\rho = M/V = M/(\tfrac13\pi h^3\tan^2\alpha).

MoI of disc about axis: 12dm⋅r2=12ρπz2tan⁡2α⋅z2tan⁡2α dz=12ρπz4tan⁡4α dz\tfrac12 dm\cdot r^2 = \tfrac12\rho\pi z^2\tan^2\alpha\cdot z^2\tan^2\alpha\,dz = \tfrac12\rho\pi z^4\tan^4\alpha\,dz.

Integrate 00 to hh: I=ρπtan⁡4α2⋅h55=ρπh5tan⁡4α10I = \tfrac{\rho\pi\tan^4\alpha}{2}\cdot \tfrac{h^5}{5} = \tfrac{\rho\pi h^5\tan^4\alpha}{10}.

Substituting ρ\rho: I=3Mh2tan⁡2α10=3MR210I = \dfrac{3 M h^2\tan^2\alpha}{10} = \dfrac{3MR^2}{10}, where R=htan⁡αR = h\tan\alpha is the base radius.


Topic 4: Torque and Angular Momentum

Sub-topic A: Torque

About a point OO, the torque of a force F⃗\vec F applied at position r⃗\vec r (from OO) is

τ⃗=r⃗×F⃗,∣τ∣=rFsin⁡θ=F⋅r⊥.\vec\tau = \vec r\times\vec F,\quad |\tau| = rF\sin\theta = F\cdot r_\perp.

For rotation about a fixed axis with MoI II:

τext=Iα.\tau_{ext} = I\alpha.

Sub-topic B: Angular momentum

For a single particle, L⃗=r⃗×p⃗=mr⃗×v⃗\vec L = \vec r\times\vec p = m\vec r\times\vec v.

For a rigid body rotating about a fixed axis with ω\omega: L=IωL = I\omega.

Theorem: τ⃗ext=dL⃗/dt\vec\tau_{ext} = d\vec L/dt (Newton's 2nd law for rotation).

Sub-topic C: Conservation of angular momentum

If τ⃗ext=0⃗\vec\tau_{ext} = \vec 0, then L⃗=\vec L = const.

Classic examples:

  • Ice skater pulling arms in: II decreases, ω\omega increases.
  • Planet in elliptic orbit: gravity is central → torque about Sun is zero → LL conserved → Kepler's 2nd law (equal areas in equal times).
  • Top with no friction: spin axis precession is via gravity torque.

Sub-topic D: Angular momentum about a point (moving particle)

For a particle moving with velocity v⃗\vec v at position r⃗\vec r relative to OO,

L⃗=mr⃗×v⃗.\vec L = m\vec r\times\vec v.

Magnitude: L=mvrsin⁡θ=mv⋅dL = mvr\sin\theta = mv\cdot d where dd is the perpendicular distance from OO to the line of v⃗\vec v.

For a particle moving in a straight line (constant v⃗\vec v): the perpendicular distance from a fixed point to the line is constant → LL is constant about that point (even though the particle moves).

Worked Examples (JEE Main level)

Example 4.1. A force F⃗=(3ı^+4ȷ^)\vec F = (3\hat\imath + 4\hat\jmath) N acts at position r⃗=(2ı^−ȷ^)\vec r = (2\hat\imath - \hat\jmath) m. Torque about origin?

τ⃗=r⃗×F⃗=(2ı^−ȷ^)×(3ı^+4ȷ^)=8k^+3k^=11k^\vec\tau = \vec r\times\vec F = (2\hat\imath - \hat\jmath)\times(3\hat\imath+4\hat\jmath) = 8\hat k + 3\hat k = 11\hat k N·m.

Example 4.2. A flywheel of MoI 0.50.5 kg·m² spins at 2020 rad/s. Torque to stop in 44 s?

τ=Iα=0.5⋅(20/4)=2.5\tau = I\alpha = 0.5\cdot(20/4) = 2.5 N·m.

Worked Examples (JEE Advanced level)

Example 4.A1. A bullet of mass mm moving at speed vv hits and embeds in the free end of a rod (mass MM, length LL) pivoted at the other end. Angular speed of the system just after collision?

Conserve angular momentum about pivot (the impulsive reaction at pivot has zero moment arm):

mvL=IωmvL = I\omega, where I=ML2/3+mL2I = ML^2/3 + mL^2.

ω=mvL(M/3+m)L2=mv(M/3+m)L.\omega = \frac{mvL}{(M/3 + m)L^2} = \frac{mv}{(M/3 + m)L}.

Example 4.A2. A planet moves in an elliptic orbit; at perihelion distance r1r_1 its speed is v1v_1. Find speed at aphelion (r2r_2).

LL conserved: mv1r1=mv2r2⇒v2=v1r1/r2m v_1 r_1 = m v_2 r_2\Rightarrow v_2 = v_1 r_1/r_2 (with both velocities perpendicular to position at these extremes).


Topic 5: Rolling Motion

Sub-topic A: Pure rolling condition

For a body of radius RR rolling without slipping on a surface:

vcm=ωR,acm=αR.v_{cm} = \omega R,\quad a_{cm} = \alpha R.

The point of contact is instantaneously at rest.

Sub-topic B: KE decomposition

Total KE = translational KE of CM + rotational KE about CM:

KE=12Mvcm2+12Icmω2.KE = \tfrac12 M v_{cm}^2 + \tfrac12 I_{cm}\omega^2.

For pure rolling: KE=12Mv2(1+Icm/(MR2))KE = \tfrac12 M v^2(1 + I_{cm}/(MR^2)).

For a solid sphere (I=2MR2/5I=2MR^2/5): KE=(7/10)Mv2KE = (7/10)Mv^2. For a disc/cylinder (I=MR2/2I=MR^2/2): KE=(3/4)Mv2KE = (3/4)Mv^2. For a ring (I=MR2I=MR^2): KE=Mv2KE = Mv^2.

Sub-topic C: Rolling on an incline

A body of mass MM, radius RR, MoI I=βMR2I = \beta M R^2 (so β=2/5,1/2,1\beta = 2/5, 1/2, 1 for solid sphere, disc, ring).

Newton's 2nd law along incline: Mgsin⁡θ−f=MaMg\sin\theta - f = Ma.

Torque about CM (friction at the contact point): fR=Iα=βMR2⋅a/R=βMRa⇒f=βMaf R = I\alpha = \beta M R^2\cdot a/R = \beta M R a\Rightarrow f = \beta M a.

So Mgsin⁡θ−βMa=Ma⇒a=gsin⁡θ1+β.Mg\sin\theta - \beta M a = M a\Rightarrow a = \dfrac{g\sin\theta}{1+\beta}.

Friction needed: f=βMa=βMgsin⁡θ1+βf = \beta M a = \dfrac{\beta M g\sin\theta}{1+\beta}.

For no slipping, need f≤μsMgcos⁡θf\le \mu_s M g\cos\theta:

μs≥βtan⁡θ1+β.\boxed{\mu_s \ge \frac{\beta\tan\theta}{1+\beta}.}

If incline is steeper, body rolls AND slips, and friction becomes kinetic μkMgcos⁡θ\mu_k Mg\cos\theta.

Race down an incline. From a=gsin⁡θ/(1+β)a = g\sin\theta/(1+\beta), smaller β\beta wins: solid sphere >> disc >> ring. Speed at the bottom (from v2=2aLv^2 = 2a L, where LL = incline length, h=Lsin⁡θh=L\sin\theta):

v=2gh1+β.v = \sqrt{\frac{2gh}{1+\beta}}.

Sub-topic D: Direction of friction in rolling

  • Body initially rolling on smooth surface: no friction needed; rolls forever.
  • Body rolling on rough surface, no other force: no slipping tendency, so no friction.
  • Pure translation on rough surface (e.g. a ball placed on belt or kicked): friction acts on the bottom backward (opposing slip), provides torque to start rolling.
  • Body rolling down incline: friction acts up the incline (provides torque to keep angular acceleration positive).
  • Body being pushed/pulled at the centre on rough surface: friction acts backward (opposes slip tendency at contact).
  • Body being pushed/pulled at the top: depends on geometry. Trick: write the torque equation about the bottom contact point to find net rotational effect; friction adjusts accordingly.

Sub-topic E: Slipping → rolling transition

A ball is given pure translation v0v_0 on a rough horizontal surface (μk\mu_k). Find time at which pure rolling begins.

Friction μkmg\mu_k mg backward decelerates: v(t)=v0−μkgtv(t) = v_0 - \mu_k g t.

Torque about CM (friction at contact, lever arm RR): τ=μkmgR=Iα=(2/5)mR2α⇒α=(5μkg)/(2R)\tau = \mu_k mg R = I\alpha = (2/5) mR^2\alpha\Rightarrow \alpha = (5\mu_k g)/(2R).

ω(t)=αt=5μkgt/(2R)\omega(t) = \alpha t = 5\mu_k g t/(2R).

Pure rolling when v=ωRv = \omega R:

v0−μkgt=(5/2)μkgt⇒t=2v07μkg.v_0 - \mu_k g t = (5/2)\mu_k g t\Rightarrow t = \frac{2 v_0}{7\mu_k g}.

Speed at this instant: v=v0−μkg⋅2v0/(7μkg)=5v0/7v = v_0 - \mu_k g\cdot 2v_0/(7\mu_k g) = 5 v_0/7.

Worked Examples (JEE Main level)

Example 5.1. A solid sphere rolls down a 30∘30^\circ incline. Acceleration (g=10g=10)?

a=gsin⁡θ/(1+β)=10⋅0.5/(1+2/5)=5/(7/5)=25/7≈3.57a = g\sin\theta/(1+\beta) = 10\cdot 0.5/(1+2/5) = 5/(7/5) = 25/7\approx 3.57 m/s².

Example 5.2. Min μ\mu for a disc to roll without slipping on a 45∘45^\circ incline?

μ≥βtan⁡θ/(1+β)=(1/2)⋅1/(3/2)=1/3\mu\ge \beta\tan\theta/(1+\beta) = (1/2)\cdot 1/(3/2) = 1/3.

Worked Examples (JEE Advanced level)

Example 5.A1. A solid sphere is set spinning at ω0\omega_0 in place (no translation) on a rough horizontal surface (μ\mu). Find time and position when pure rolling starts.

Friction acts on the bottom contact; bottom is moving backward (since sphere spins forward), so friction is forward. This accelerates the CM: a=μga = \mu g (forward). Torque about CM (friction acts at contact, magnitude μmg\mu mg, lever arm RR): τ=μmgR\tau = \mu mg R, opposite to spin → decelerates: α=−5μg/(2R)\alpha = -5\mu g/(2R).

v(t)=μgtv(t) = \mu g t. ω(t)=ω0−5μgt/(2R)\omega(t) = \omega_0 - 5\mu g t/(2R).

Pure rolling: v=ωR⇒μgt=ω0R−5μgt/2⇒t=2ω0R7μgv = \omega R\Rightarrow \mu g t = \omega_0 R - 5\mu g t/2\Rightarrow t = \dfrac{2\omega_0 R}{7\mu g}.

Distance covered =12μgt2=μg⋅2ω02R2/(49μ2g2)=2ω02R2/(49μg)= \tfrac12 \mu g t^2 = \mu g\cdot 2\omega_0^2 R^2/(49\mu^2 g^2) = 2\omega_0^2 R^2/(49\mu g).

Final speed v=2ω0R/7v = 2\omega_0 R/7.

Example 5.A2. A sphere of radius rr rolls in the inside of a hemisphere of radius RR. Period of small oscillations?

The CM moves on a circle of radius R−rR-r. Equation of motion (SHM with effective "gg" depending on rolling): T=2π(R−r)/geffT = 2\pi\sqrt{(R-r)/g_{\text{eff}}}, where geff=g/(1+β)=5g/7g_{\text{eff}} = g/(1+\beta) = 5g/7. So T=2π7(R−r)/(5g)T = 2\pi\sqrt{7(R-r)/(5g)}.


Topic 6: Instantaneous Axis of Rotation (IAR)

Sub-topic A: Definition

In a rigid body undergoing combined translation and rotation, at any instant there is an axis (possibly external to the body) about which the body appears to be in pure rotation. The point on the body coinciding with this axis has zero velocity.

For pure rolling, the contact point is the IAR.

Sub-topic B: KE about IAR

If IIARI_{IAR} is MoI about the instantaneous axis,

KE=12IIARω2.KE = \tfrac12 I_{IAR}\omega^2.

For a wheel rolling on the ground with vcm=ωRv_{cm} = \omega R: IIAR=Icm+MR2I_{IAR} = I_{cm} + MR^2. KE=12(Icm+MR2)ω2=12Icmω2+12Mv2KE = \tfrac12 (I_{cm}+MR^2)\omega^2 = \tfrac12 I_{cm}\omega^2 + \tfrac12 M v^2. ✓

Sub-topic C: Useful for finding velocities of various points

Velocity of point PP on a rolling body: v⃗P=ω⃗×r⃗P\vec v_P = \vec\omega\times\vec r_P where r⃗P\vec r_P is from IAR. Magnitude =ω⋅∣rP∣= \omega\cdot \vert r_P\vert .

  • Top of wheel: 2vcm2v_{cm}.
  • Bottom: 00.
  • Any point: depends on its distance from contact point.

Worked Examples

Example 6.1. A wheel of radius 0.50.5 m rolls at vcm=10v_{cm}=10 m/s. Velocity of the topmost point?

2vcm=202v_{cm} = 20 m/s.

Example 6.2. A ladder of length LL slides such that its bottom moves on the floor with velocity vv and top moves down the wall. Find angular velocity when the ladder makes angle θ\theta with the floor.

The IAR is the point such that horizontal velocity of the bottom matches and vertical velocity of the top matches. Bottom: (xB,0)(x_B, 0), velocity (v,0)(v, 0). Top: (0,yT)(0, y_T), velocity (0,−vT)(0, -v_T).

The IAR is at (xB,yT)(x_B, y_T) — i.e. the corner of the rectangle. ω=v/yT=v/(Lsin⁡θ)\omega = v/y_T = v/(L\sin\theta).


Topic 7: Toppling vs Sliding

A block of width ww, height hh on a rough floor pushed horizontally at the top.

Sliding condition: F>μmgF > \mu mg.

Toppling condition: torque about the front edge (front edge is pivot) exceeds the restoring torque from gravity. Fh>mg(w/2)F h > mg(w/2), i.e. F>mgw/(2h)F > mgw/(2h).

Whichever condition is satisfied first as FF increases determines whether the block slides or topples.

  • If μmg<mgw/(2h)\mu mg < mgw/(2h), i.e. μ<w/(2h)\mu < w/(2h): sliding first.
  • If μ>w/(2h)\mu > w/(2h): toppling first.

(For force applied at height h0h_0 instead of top, replace hh by h0h_0 in the toppling condition.)

Worked Examples (JEE Advanced level)

Example 7.A1. A cube of side aa on a rough floor is pushed by a horizontal force at the top edge. μ=0.5\mu = 0.5. What happens?

Toppling at F=mga/(2a)=mg/2F = mga/(2a) = mg/2. Sliding at F=μmg=mg/2F = \mu mg = mg/2. They're equal — both occur simultaneously.


Topic 8: Rotational Collisions

Sub-topic A: Impulse and angular impulse

For a collision with a hinged body, angular impulse = change in angular momentum:

∫τ dt=ΔL.\int \tau\,dt = \Delta L.

About the pivot, the impulsive hinge force has zero moment arm, so doesn't contribute. Use this to find ω\omega after collision.

Sub-topic B: Examples

Bullet–rod (hinged at one end): mvL=Iω=(ML2/3+mL2)ωmvL = I\omega = (ML^2/3 + mL^2)\omega.

Bullet–free rod: Conserve linear momentum AND angular momentum about CM. Bullet embeds at end → final body has CM somewhere between original rod CM and the embedding point. Find vcmv_{cm} from linear momentum, ω\omega from angular momentum about CM.

Worked Examples (JEE Advanced level)

Example 8.A1. A rod of mass MM, length LL lies on a smooth horizontal table. A ball of mass mm moves perpendicular to the rod with speed vv and hits the end of the rod, sticking. Find CM speed and angular speed of the system after collision.

Linear momentum: mv=(M+m)vcm⇒vcm=mv/(M+m)mv = (M+m)v_{cm}\Rightarrow v_{cm} = mv/(M+m).

Locate new CM: original rod CM at centre, mass MM; ball at end (distance L/2L/2 from rod CM), mass mm. New CM at distance mL/(2(M+m))mL/(2(M+m)) from original rod CM, toward the end where the ball stuck.

MoI about new CM: Inew=Irod,cm+Md12+md22I_{new} = I_{rod,cm} + M d_1^2 + m d_2^2, where d1=mL/(2(M+m))d_1 = mL/(2(M+m)) and d2=ML/(2(M+m))d_2 = ML/(2(M+m)).

Inew=ML2/12+M(mL2(M+m))2+m(ML2(M+m))2I_{new} = ML^2/12 + M\left(\dfrac{mL}{2(M+m)}\right)^2 + m\left(\dfrac{ML}{2(M+m)}\right)^2.

Simplify: =ML2/12+MmL2(m+M)4(M+m)2⋅11=ML2/12+MmL24(M+m)= ML^2/12 + \dfrac{Mm L^2 (m + M)}{4(M+m)^2}\cdot \dfrac{1}{1} = ML^2/12 + \dfrac{Mm L^2}{4(M+m)}.

Angular momentum about new CM: the ball had momentum mvmv at distance d2=ML/(2(M+m))d_2 = ML/(2(M+m)) from CM perpendicular to its motion.

L0=mv⋅d2=mMvL2(M+m)L_0 = mv\cdot d_2 = \dfrac{m M v L}{2(M+m)}.

After: L0=Inewω⇒ω=L0/InewL_0 = I_{new}\omega\Rightarrow \omega = L_0/I_{new}.


Problem-Solving Heuristics

  1. For CM problems, use the formula straightforwardly; for bodies with cavities, use negative mass trick.
  2. Choose the axis of MoI carefully — usually the CM or the contact point. Use parallel axis to shift.
  3. For a plane lamina, perpendicular axis theorem is your friend (Iz=Ix+IyI_z = I_x+I_y).
  4. For combined translation + rotation, always write two equations: ∑F=Macm\sum F = Ma_{cm} and ∑τcm=Icmα\sum\tau_{cm} = I_{cm}\alpha. Then use the rolling constraint a=αRa = \alpha R.
  5. Friction in rolling: not always at μN\mu N — only the maximum. For pure rolling, friction is whatever is needed (static); compute it, compare with μN\mu N to check.
  6. For rotational collisions with a hinged body: conserve angular momentum about the hinge; the impulsive hinge force is unknown but has zero moment arm.
  7. Angular momentum of a moving particle about a point: L=mv⋅d⊥L = mv\cdot d_\perp (perpendicular distance from the point to the line of motion).
  8. For two-body rotational problems on a smooth floor, conserve linear momentum, angular momentum about the new CM, and (if elastic) KE.
  9. Sphere rolling down: solid sphere wins the race, then disc/cylinder, then ring. Order is by β\beta — smaller β\beta, faster.
  10. Toppling vs sliding: compute the force needed for each; the smaller decides the outcome.

Common Traps & Mistakes

  • For a disc, the MoI about a diameter is MR2/4MR^2/4, not MR2/2MR^2/2 (that's about the perpendicular axis through centre).
  • For a rod, I=ML2/12I = ML^2/12 about centre, ML2/3ML^2/3 about end — students often invert.
  • Rolling without slipping is a constraint: vcm=ωRv_{cm}=\omega R. You can't assume this if there's slipping.
  • Friction in pure rolling is static, not kinetic. So ff can be any value up to μsN\mu_s N.
  • When a body slides and rolls (e.g. on a slippery incline), use kinetic friction; the constraint v=ωRv=\omega R does NOT hold.
  • Sphere on smooth surface kicked at centre: it slides without rolling (no friction → no torque). On rough surface, it eventually rolls.
  • A particle moving in a straight line at constant velocity has constant angular momentum about a fixed point (the perpendicular distance is constant).
  • The torque on a planet about the Sun is zero, so LL is conserved — but NOT the angular velocity (since the distance changes).
  • Negative mass for cavities: don't double-count!

Quick Revision Card

  • R⃗cm=∑mir⃗i/∑mi\vec R_{cm} = \sum m_i\vec r_i/\sum m_i; for continuous bodies use integrals.
  • I=∑miri2I = \sum m_i r_i^2; key results:
    • Rod about centre =ML2/12= ML^2/12, about end =ML2/3= ML^2/3
    • Ring about axis =MR2= MR^2, about diameter =MR2/2= MR^2/2
    • Disc about axis =MR2/2= MR^2/2, about diameter =MR2/4= MR^2/4
    • Solid sphere =2MR2/5= 2MR^2/5, shell =2MR2/3= 2MR^2/3
  • Parallel axis: I=Icm+Md2I = I_{cm} + Md^2.
  • Perp. axis (lamina): Iz=Ix+IyI_z = I_x + I_y.
  • τ=Iα\tau = I\alpha, L=IωL = I\omega, τext=dL/dt\tau_{ext} = dL/dt.
  • Pure rolling: v=ωRv = \omega R, KE=12Mv2(1+β)KE = \tfrac12 Mv^2(1+\beta).
  • Rolling down incline: a=gsin⁡θ/(1+β)a = g\sin\theta/(1+\beta), vbot=2gh/(1+β)v_{bot} = \sqrt{2gh/(1+\beta)}.
  • Min μ\mu for rolling: μ≥βtan⁡θ/(1+β)\mu \ge \beta\tan\theta/(1+\beta).
  • Bullet–hinged rod: mvL=(ML2/3+mL2)ωmvL = (ML^2/3 + mL^2)\omega.

Formula Sheet

BodyMoI (axis specified)
Rod (centre, perp.)ML2/12ML^2/12
Rod (end, perp.)ML2/3ML^2/3
Ring (centre, perp.)MR2MR^2
Ring (diameter)MR2/2MR^2/2
Disc (centre, perp.)MR2/2MR^2/2
Disc (diameter)MR2/4MR^2/4
Solid sphere (centre)2MR2/52MR^2/5
Spherical shell (centre)2MR2/32MR^2/3
Solid cylinder (axis)MR2/2MR^2/2
Hollow cylinder (axis)MR2MR^2
Rectangular plate (centre, perp.)M(a2+b2)/12M(a^2+b^2)/12
ConceptFormula
Parallel axisI=Icm+Md2I = I_{cm} + Md^2
Perpendicular axis (lamina)Iz=Ix+IyI_z = I_x + I_y
Radius of gyrationI=Mk2I = Mk^2
Torqueτ⃗=r⃗×F⃗\vec\tau = \vec r\times\vec F
Newton (rotation)τ=Iα\tau = I\alpha
Angular momentumL⃗=r⃗×p⃗\vec L = \vec r\times \vec p; for rigid body L=IωL = I\omega
Conservationτext=0⇒L=\tau_{ext} = 0\Rightarrow L = const
Pure rollingv=ωRv = \omega R
KE (rolling)12Mv2+12Iω2=12Mv2(1+β)\tfrac12 Mv^2 + \tfrac12 I\omega^2 = \tfrac12 Mv^2(1+\beta)
Acceleration rolling down inclinea=gsin⁡θ/(1+β)a = g\sin\theta/(1+\beta)
Min μ\mu rollingβtan⁡θ/(1+β)\beta\tan\theta/(1+\beta)
Time to start rolling (kicked)t=2v0/(7μg)t = 2v_0/(7\mu g)
Bullet–rod (hinged)ω=mvL/(ML2/3+mL2)\omega = mvL/(ML^2/3 + mL^2)

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