Physics by Lamhi: Not Your Boring Physics

CLASS 11 · CHAPTER 6 · MECHANICS

QUICK REVISION

System of Particles & Rotational Motion

Every key result from this chapter, boxed and ready for a last look before the exam. No derivations here, just what to recall and when to use it — for the full explanation, see the detailed notes.

1. Centre of Mass

R=1M∑imiriFext=Macm\mathbf{R} = \dfrac{1}{M}\sum_i m_i\mathbf{r}_i \qquad \mathbf{F}_{ext} = M\mathbf{a}_{cm}

The CM moves exactly as if the whole mass were concentrated there and the whole external force acted there — internal forces always cancel in pairs (Newton’s third law).

2. Torque and Angular Momentum

τ=r×FL=r×pτext=dLdt\boldsymbol{\tau} = \mathbf{r}\times\mathbf{F} \qquad \mathbf{L} = \mathbf{r}\times\mathbf{p} \qquad \boldsymbol{\tau}_{ext} = \dfrac{d\mathbf{L}}{dt}

Both τ\boldsymbol{\tau} and L\mathbf{L} are defined only relative to a chosen origin. τ=rFsin⁡θ\tau = rF\sin\theta, direction by the right-hand rule.

3. Moment of Inertia — Standard Results

I=∑imiri2=MK2I = \sum_i m_ir_i^2 = MK^2
  • Ring about central (symmetry) axis: I=MR2I = MR^2
  • Disc about central axis: I=12MR2I = \tfrac{1}{2}MR^2
  • Solid sphere about a diameter: I=25MR2I = \tfrac{2}{5}MR^2
  • Thin rod about centre, ⊥ to length: I=112ML2I = \tfrac{1}{12}ML^2

rir_i is the perpendicular distance from the axis; KK (radius of gyration) is where all the mass would sit, as a point, to give the same II.

4. Perpendicular and Parallel Axes Theorems

Iz=Ix+IyI=Icm+Md2I_z = I_x + I_y \qquad I = I_{cm} + Md^2
  1. Perpendicular axes: planar lamina only; x,yx,y in the plane, zz through their intersection, normal to the plane.
  2. Parallel axes: any rigid body; IcmI_{cm} is the minimum over all parallel axes — moving away only adds Md2≥0Md^2 \ge 0.

5. Conservation of Angular Momentum

L=constantwhenτext=0I1ω1=I2ω2\mathbf{L} = \text{constant} \quad\text{when}\quad \boldsymbol{\tau}_{ext}=0 \qquad I_1\omega_1 = I_2\omega_2
KE=12Iω2=L22IKE = \tfrac{1}{2}I\omega^2 = \dfrac{L^2}{2I}
  1. Skater pulls arms in: II drops, ω\omega shoots up to keep LL fixed, and KEKE rises — that extra energy comes from muscular work, not for free.

6. Rolling — Kinetic Energy Split

vcm=ωRv_{cm} = \omega R
KE=12Mvcm2+12Iω2=12Mvcm2(1+K2R2)KE = \tfrac{1}{2}Mv_{cm}^2 + \tfrac{1}{2}I\omega^2 = \tfrac{1}{2}Mv_{cm}^2\left(1+\dfrac{K^2}{R^2}\right)

7. Rolling Down an Incline — Key Result

vcm=2gh1+K2/R2v_{cm} = \sqrt{\dfrac{2gh}{1+K^2/R^2}}
  1. Smaller K2/R2K^2/R^2 (mass closer to the axis) needs less energy budget to spin up, so more is left for translation — it arrives faster, regardless of mass or radius.
  2. Solid sphere (K2/R2=2/5)(K^2/R^2=2/5) beats a hollow cylinder (K2/R2=1)(K^2/R^2=1) down the same incline, every time.

Full derivations and worked examples: detailed notes →