Angular Momentum

Conservation of angular momentum, cross products, and applications

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Angular Momentum

Definition

For a particle: L=r×p=m(r×v)\vec{L} = \vec{r} \times \vec{p} = m(\vec{r} \times \vec{v})

Magnitude: L=rmvsinθ=rmv=mrvL = rmv\sin\theta = r_{\perp}mv = mrv_{\perp}

For rotation about fixed axis: L=IωL = I\omega

Relationship to Torque

τ=dLdt\vec{\tau} = \frac{d\vec{L}}{dt}

(Rotational analog of F=dpdt\vec{F} = \frac{d\vec{p}}{dt})

For fixed axis with constant II: τ=Idωdt=Iα\tau = I\frac{d\omega}{dt} = I\alpha

Conservation of Angular Momentum

When τext=0\vec{\tau}_{ext} = 0:

L=constant\vec{L} = \text{constant}

Iiωi=IfωfI_i\omega_i = I_f\omega_f

Example: Figure Skater

Skater pulls arms in, reducing moment of inertia:

Iiωi=IfωfI_i\omega_i = I_f\omega_f

If If<IiI_f < I_i, then ωf>ωi\omega_f > \omega_i (spins faster)

Energy changes: KEi=12Iiωi2,KEf=12Ifωf2KE_i = \frac{1}{2}I_i\omega_i^2, \quad KE_f = \frac{1}{2}I_f\omega_f^2

KEf=12If(IiIfωi)2=IiIf12Iiωi2=IiIfKEiKE_f = \frac{1}{2}I_f\left(\frac{I_i}{I_f}\omega_i\right)^2 = \frac{I_i}{I_f}\cdot\frac{1}{2}I_i\omega_i^2 = \frac{I_i}{I_f}KE_i

Energy increases! (Work done by internal forces)

Angular Momentum of System

Ltotal=iLi=iri×pi\vec{L}_{total} = \sum_i \vec{L}_i = \sum_i \vec{r}_i \times \vec{p}_i

About center of mass: L=Lcm+Lorbital\vec{L} = \vec{L}_{cm} + \vec{L}_{orbital}

where:

  • Lcm=Icmω\vec{L}_{cm} = I_{cm}\vec{\omega} (spin)
  • Lorbital=rcm×Mvcm\vec{L}_{orbital} = \vec{r}_{cm} \times M\vec{v}_{cm} (orbital)

Central Force Motion

For central force (directed toward/away from fixed point):

τ=r×F=0\vec{\tau} = \vec{r} \times \vec{F} = 0

(because F\vec{F} parallel to r\vec{r})

Therefore: L\vec{L} = constant

Consequences:

  1. Motion confined to a plane
  2. Areal velocity constant (Kepler's second law)
  3. r2θ˙=Lmr^2\dot{\theta} = \frac{L}{m} = constant

Areal Velocity

Area swept out per unit time:

dAdt=12r2dθdt=12r2ω=L2m\frac{dA}{dt} = \frac{1}{2}r^2\frac{d\theta}{dt} = \frac{1}{2}r^2\omega = \frac{L}{2m}

(Constant for central forces)

Collisions and Angular Momentum

For collision, if τext=0\vec{\tau}_{ext} = 0 about some point, then L\vec{L} conserved about that point.

Example: Putty Ball Hitting Rod

Ball of mass mm, speed vv hits rod of length LL, mass MM at distance dd from pivot.

Before: Li=mvdL_i = mvd (ball's angular momentum)

After: Lf=ItotalωL_f = I_{total}\omega

where Itotal=13ML2+md2I_{total} = \frac{1}{3}ML^2 + md^2 (rod + stuck ball)

mvd=(13ML2+md2)ωmvd = \left(\frac{1}{3}ML^2 + md^2\right)\omega

ω=mvd13ML2+md2\omega = \frac{mvd}{\frac{1}{3}ML^2 + md^2}

Precession

Spinning top with angular momentum L\vec{L} tilted at angle θ\theta:

Gravitational torque: τ=mgrsinθ\tau = mgr\sin\theta

This causes precession (axis rotates) with angular velocity:

Ω=τLsinθ=mgrL=mgrIω\Omega = \frac{\tau}{L\sin\theta} = \frac{mgr}{L} = \frac{mgr}{I\omega}

Gyroscopic Motion

Gyroscope resists changes in orientation due to angular momentum conservation.

Applied torque τ\vec{\tau} causes change: ΔL=τΔt\Delta\vec{L} = \vec{\tau}\Delta t

Direction of ΔL\Delta\vec{L} perpendicular to both L\vec{L} and τ\vec{\tau}, causing precession.

Angular Impulse

t1t2τdt=ΔL\int_{t_1}^{t_2} \vec{\tau} \, dt = \Delta\vec{L}

Analog of linear impulse Fdt=Δp\int \vec{F} \, dt = \Delta\vec{p}

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