Is the notion of angular velocity $\boldsymbol{\omega}$ defined for arbitrary particle trajectories (e.g. a crazy one like $\textbf x(t)=(t^3\ln(t),\sqrt{t}\operatorname{erf}(2t),\cot^{42}(t))$) or only when the position and velocity vectors of the particle are constantly orthogonal (i.e. $\textbf x(t)\cdot\dot{\textbf x}(t)=0$ for all $t\geq 0$, which implies that the particle is constrained to move on a sphere)? Or even only when the particle engages in circular motion (i.e. it is constrained to travel on a great circle of the aforementioned sphere)? I have seen two conflicting definitions; for example, one can attempt to define angular velocity directly via the formula $$\boldsymbol{\omega}:=\frac{\textbf x\times{\dot{\textbf x}}}{\textbf x\cdot\textbf x}$$ which has the advantage that (as long as the particle never comes to the origin), the angular velocity at each moment in time $t\geq 0$ is completely well-defined, regardless of how sophisticated the trajectory $\textbf x$ is. This definition also has the property that at every moment $t\geq 0$ in time, $\boldsymbol \omega(t)\in(\operatorname{span}\{\textbf x(t),\dot{\textbf x}(t)\})^{\perp}$ is orthogonal to the instantaneous plane of the particle's rotation and does so in a right-handed way. One can check that its magnitude $||\boldsymbol \omega||$ also behaves in a reasonable manner. On the other hand, sometimes people seem to define the angular velocity $\boldsymbol \omega$ indirectly as the unique vector satisfying: $$\dot{\textbf x}=\boldsymbol \omega\times{\textbf x}$$ which also lies along "the axis of rotation". These definitions are incompatible with each other for a number of reasons, the obvious one being that in the latter we have already assumed a priori that $\textbf x\cdot\dot{\textbf x}=0$ (indeed, one can prove the following general result about $3$-dimensional Euclidean vector spaces: if $\textbf a\in{\textbf R^3}$ and $\textbf c\in{\textbf R^3\setminus{\{\textbf 0}}\}$ are two $3$-dimensional Euclidean vectors with $\textbf c$ not equal to the zero vector $\textbf 0$, then there exists a vector $\textbf b\in \textbf R^3$ such that $\textbf a=\textbf b\times\textbf c$ if and only if $\textbf a\cdot\textbf c=0$). So how should one conceptualize angular velocity (for a single point particle)?
2 Answers
The second equation $\dot{\boldsymbol x}=\boldsymbol\omega\times \boldsymbol x$ is the general definition of spin angular velocity, $\boldsymbol\omega\,,$ in space for a rotating rigid body (see Arnold's book on Classical Mechanics).
The first equation $\boldsymbol\omega=\boldsymbol x\times\dot{\boldsymbol x}/|{\boldsymbol x}|^2$ is the correct definition for orbital angular velocity for a single particle with trajectory $\boldsymbol{x}(t)\,.$
Because every point in a rotating rigid body is a single particle it is a natural question when both concepts agree.
Consider the single particle that moves such that $\boldsymbol x$ and $\dot{\boldsymbol x}$ are always orthogonal. Using the Grassmann identity $a\times(b\times c)=(a\cdot c)\,b-(a\cdot b)\,c$ it is easy to see that the orbital angular velocity satisfies the equation for spin angular velocity. However, the fully correct definition of spin angular velocity requires that the $\boldsymbol\omega$ must be the unique vector that satisfies $\dot{\boldsymbol x}=\boldsymbol\omega\times \boldsymbol x$ for all $\boldsymbol x$ in the rigid body.
For example consider the particles $$ {\boldsymbol x}(t)=\left(\begin{array}{c}\cos t\\ \sin t\\1\end{array}\right),~~ \dot {\boldsymbol x}(t)=\left(\begin{array}{c}-\sin t\\ \cos t\\0\end{array}\right),~~ {\boldsymbol\omega}_{\text orbital}(t)=\frac{1}{2}\left(\begin{array}{c}-\cos t\\ -\sin t\\1\end{array}\right)\,, $$
$$ {\boldsymbol y}(t)=\left(\begin{array}{c}-\sin t\\ \cos t\\1\end{array}\right),~~ \dot {\boldsymbol y}(t)=\left(\begin{array}{c}-\cos t\\ -\sin t\\0\end{array}\right),~~ {\boldsymbol\omega}_{\text orbital}(t)=\frac{1}{2}\left(\begin{array}{c}\sin t\\ -\cos t\\1\end{array}\right)\, $$ and assume they are part of the same rigid body. It is easy to see that both their orbital angular velocities satisfy $\dot{\boldsymbol x}=\boldsymbol\omega\times \boldsymbol x$, resp. $\dot{\boldsymbol y}=\boldsymbol\omega\times \boldsymbol y\,.$ The uniqe spin angular velocity that satisfies both these equations is however $$ {\boldsymbol\omega}_{spin}=\left(\begin{array}{c}0\\ 0 \\1\end{array}\right)\,. $$
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We consider that angular velocity ω (ω=dφ ̇/dτ) is the first derivative of angular displacement φ with respect to time τ. In a sense, a purely geometric point cannot be described using angular velocity ω. If one insists on describing angular velocity ω in terms of linear velocity v, it can be represented by half of the curl of the velocity in mathematical terms: 1/2 (∇×v)
