Rotational Motion, Torque, and Dynamics

Torque & Rotational Dynamics

  • Torque (τ\tau): Defined as the tendency of an applied force to rotate an object about an axis of rotation.

  • Influencing Factors:

    • Magnitude of the applied force (FF).

    • Position/distance from the axis of rotation (rr).

    • Angle (θ\theta) between the position vector and the line of action of the force.

  • Torque Formula:   τ=rFsin⁡(θ)=Fd=r⊥F\tau = r F \sin(\theta) = F d = r_\perp F

    • The lever arm (dd or r⊥r_\perp) is the perpendicular distance from the axis of rotation to the line along which the force acts: d=rsin⁡(θ)d = r \sin(\theta).

  • Angular Limits:

    • θ=0∘\theta = 0^\circ or 180∘180^\circ: Torque is zero (τ=0\tau = 0) because the force is parallel to the position vector.

    • θ=90∘\theta = 90^\circ or 270∘270^\circ: Torque achieves maximum magnitude.

  • Units & Sign Convention:

    • SI Unit: N⋅m\text{N}\cdot\text{m}

    • Counterclockwise (anticlockwise) torque: Positive (+τ+\tau).

    • Clockwise torque: Negative (−τ-\tau).


Sign conventions for rotational torque

Moment of Inertia (Rotational Inertia)

  • Definition: The tendency of a body to resist angular acceleration; represents rotational inertia.

  • Governing Factors:

    • Mass of the body (MM or mm).

    • Distribution of mass relative to the axis of rotation.

    • Selection/location of the axis of rotation.


Effect of rotation axis location on difficulty of spinning a rod
  • Mathematical Definitions:

    • Single point mass: I=mr2I = m r^2

    • Discrete collection of particles: I=∑imiri2=m1r12+m2r22+m3r32+…I = \sum_i m_i r_i^2 = m_1 r_1^2 + m_2 r_2^2 + m_3 r_3^2 + \dots

    • Continuous mass distribution: I=∫r2 dmI = \int r^2\,dm

    • SI Unit: kg⋅m2\text{kg}\cdot\text{m}^2

  • Formulas for Common Geometries:

    • Hoop / thin-walled cylinder (about cylinder axis): I=MR2I = M R^2

    • Annular cylinder / ring (about cylinder axis): I=12M(R12+R22)I = \frac{1}{2} M (R_1^2 + R_2^2)

    • Solid cylinder or disk (about cylinder axis): I=12MR2I = \frac{1}{2} M R^2

    • Solid cylinder or disk (about central diameter): I=14MR2+112Ml2I = \frac{1}{4} M R^2 + \frac{1}{12} M l^2

    • Thin rod (axis through center, perpendicular to length): I=112Ml2I = \frac{1}{12} M l^2

    • Thin rod (axis through one end, perpendicular to length): I=13Ml2I = \frac{1}{3} M l^2

    • Solid sphere (about any diameter): I=25MR2I = \frac{2}{5} M R^2

    • Thin spherical shell (about any diameter): I=23MR2I = \frac{2}{3} M R^2

    • Hoop (about any diameter): I=12MR2I = \frac{1}{2} M R^2

    • Flat slab (perpendicular axis through center): I=112M(a2+b2)I = \frac{1}{12} M (a^2 + b^2)


Moments of inertia for various standard geometric objects

Newton's Second Law for Rotation

  • Rotational Formulation:   τnet=Iα\tau_{\text{net}} = I \alpha   α=τnetI\alpha = \frac{\tau_{\text{net}}}{I}

    • Angular acceleration (α\alpha) is directly proportional to net torque (τnet\tau_{\text{net}}) and inversely proportional to rotational inertia (II).

  • Derivation from Linear Dynamics:

    • Linear tangential form: FT=maT=m(rα)F_T = m a_T = m(r \alpha)

    • Multiplying both sides by rr:     FTr=mr2α  ⟹  τ=IαF_T r = m r^2 \alpha \implies \tau = I \alpha

  • Equilibrium State Independence:

    • A system can have zero net translational force (Fnet=0\mathbf{F}_{\text{net}} = 0) while experiencing a non-zero net rotational torque (τnet≠0\boldsymbol{\tau}_{\text{net}} \neq 0).

  • Problem-Solving Framework:

    • Draw free-body diagrams showing points of application for each force.

    • Apply translational equations: Fnet=∑Fi=ma\mathbf{F}_{\text{net}} = \sum \mathbf{F}_i = m \mathbf{a}

    • Apply rotational equations about a common axis: τnet=∑τi=Iα\boldsymbol{\tau}_{\text{net}} = \sum \boldsymbol{\tau}_i = I \boldsymbol{\alpha}

    • Use constraint conditions (such as aT=rαa_T = r \alpha) to link translational and rotational variables.

Angular Momentum & Conservation

  • Angular Momentum (LL):

    • Defined as the rotational equivalent of linear momentum:     L=IωL = I \omega

    • For a point particle moving at radius rr: L=mr2ωL = m r^2 \omega

    • SI Unit: kg⋅m2/s\text{kg}\cdot\text{m}^2/\text{s}

  • Torque and Rate of Change:   τnet=ΔLΔt=dLdt\tau_{\text{net}} = \frac{\Delta L}{\Delta t} = \frac{dL}{dt}

  • Law of Conservation of Angular Momentum:

    • If the net external torque acting on a rotating system is zero (τnet=0\tau_{\text{net}} = 0), the total angular momentum remains constant:     dLdt=0  ⟹  Li=Lf\frac{dL}{dt} = 0 \implies L_i = L_f     I0ω0=IωI_0 \omega_0 = I \omega

    • Decreasing the moment of inertia (II) results in a proportional increase in angular velocity (ω\omega).

Rotational Kinetic Energy & Energy Conservation

  • Kinetic Energy Formulations:

    • Translational Kinetic Energy: Ktrans=12mv2K_{\text{trans}} = \frac{1}{2} m v^2

    • Rotational Kinetic Energy: Krot=12Iω2K_{\text{rot}} = \frac{1}{2} I \omega^2

    • Total Mechanical Kinetic Energy for an object rolling without slipping (v=rωv = r \omega):     Ktotal=12mv2+12Iω2K_{\text{total}} = \frac{1}{2} m v^2 + \frac{1}{2} I \omega^2

  • Conservation of Mechanical Energy:   Ei=EfE_i = E_f   Ui+Klinear,initial+Krotational,initial=Uf+Klinear,final+Krotational,finalU_i + K_{\text{linear,initial}} + K_{\text{rotational,initial}} = U_f + K_{\text{linear,final}} + K_{\text{rotational,final}}

  • Objects Rolling Down an Incline of Height hh:   mgh=12mv2+12I(vr)2m g h = \frac{1}{2} m v^2 + \frac{1}{2} I \left(\frac{v}{r}\right)^2


Comparative race of shapes rolling down an incline
  • Velocities at Bottom of Incline:

    • Frictionless sliding box: v=2ghv = \sqrt{2 g h}

    • Solid sphere (I=25mr2I = \frac{2}{5} m r^2): v=107gh≈1.20ghv = \sqrt{\frac{10}{7} g h} \approx 1.20 \sqrt{g h}

    • Solid cylinder (I=12mr2I = \frac{1}{2} m r^2): v=43gh≈1.15ghv = \sqrt{\frac{4}{3} g h} \approx 1.15 \sqrt{g h}

    • Hoop / hollow cylinder (I=mr2I = m r^2): v=gh=1.00ghv = \sqrt{g h} = 1.00 \sqrt{g h}

  • Speed Ranking: Sliding Box > Solid Sphere > Solid Cylinder > Hollow Cylinder / Hoop. Objects with a smaller fraction of inertia concentrate less potential energy into rotational motion and reach the bottom faster.

Linear vs. Rotational Analogues

  • Displacement: ss (Linear) ⟷\longleftrightarrow θ\theta (Rotational)

  • Velocity: vv (Linear) ⟷\longleftrightarrow ω\omega (Rotational)

  • Acceleration: aa (Linear) ⟷\longleftrightarrow α\alpha (Rotational)

  • Inertia / Mass: mm (Linear) ⟷\longleftrightarrow II (Rotational)

  • Dynamic Cause: Force F=maF = m a (Linear) ⟷\longleftrightarrow Torque τ=Iα\tau = I \alpha (Rotational)

  • Momentum: p=mvp = m v (Linear) ⟷\longleftrightarrow Angular Momentum L=IωL = I \omega (Rotational)

  • Kinetic Energy: K=12mv2K = \frac{1}{2} m v^2 (Linear) ⟷\longleftrightarrow KR=12Iω2K_R = \frac{1}{2} I \omega^2 (Rotational)

  • Work: W=F⋅sW = F \cdot s (Linear) ⟷\longleftrightarrow W=τ⋅θW = \tau \cdot \theta (Rotational)