Stellar kinetic-energy tensor
= Stellar kinetic-energy tensor
{title2=$T_{ij}=\tfrac12\int\rho u_iu_j\,d^3x$}
This tensor records the ordered <kinetic energy> of the <streaming velocity> $u_i=\langle v_i\rangle$. It excludes random motion; its vanishing is compatible with a nonzero <stellar pressure-energy tensor>.