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Physics LibreTexts

26.1: Angular Momentum and Angular Velocity

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In contrast to angular velocity, the angular momentum of a body depends on the point with respect to which it is defined. For now, we take it (following Landau, of course) as relative to the center of mass, but we denote it by L, following modern usage. This “intrinsic” angular momentum is like the Earth’s angular momentum from its diurnal rotation, as distinct from its orbital angular momentum in going around the Sun.

That is

L=nrn×mnvn=nrn×mn(Ω×rn)=nmn[r2nΩrn(rnΩ)]=IΩ

where I is the inertia tensor: this just means Li=IikΩk

Explicitly, taking the principal axes as the (x1,x2,x3) axes,

L1=I1Ω1,L2=I2Ω2,L3=I3Ω3

For anything with spherical inertial symmetry (such as a cube or a tetrahedron!) L=IΩ

Landau defines a rotator as a collection of massive particles all on a line. (I guess that includes diatomic molecules, and, for example, CO2, neglecting electrons and nuclear size). We know there are only two physical rotational degrees of freedom for these molecular rotators (thanks to quantum mechanics) and obviously the two principal axes are perpendicular to the line of masses, and degenerate. Again, then, L=IΩ.


This page titled 26.1: Angular Momentum and Angular Velocity is shared under a not declared license and was authored, remixed, and/or curated by Michael Fowler.

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