The inertia tensor originates from the study of (discrete or continuous) rigid systems, which are systems that preserve relative distances among their parts.
The inertia tensor does not involve any dynamical consideration (forces and torques) in its definition. It is simply a powerful tool to calculate both kinetic energy and angular momentum of a rigid system.
This tensor extends the concept of mass to rotating systems; mass determines how much speed you will gain when you transfer a certain (linear) momentum, inertia tensor determines what angular speed you will attain by trasfering a certain angular momentum:
p=m
v
L=
Iw
(Consider anyway that angular momentum depends on a prefixed pole and so will the inertia tensor; the problem can be simplified by breaking the motion into two parts one relative to the the center of mass the other treating the whole system as concentrated in the center of mass)
What characterizes a (3D real symmetric) tensor is that there are three direction of space mutually orthogonal that make the tensor diagonal. Hence a (3D real symmetric) tensor can always be thought as the rotation of these diagonal tensor. The way the diagonal tensor acts on the components of a vector is really simple since it simply multiplies each of the components for a simple number. The three numbers (principal inertia moments in our case) usually differ from each other; a scalar multiplying a vector can be simply thought as a tensor with three identical principal components.
To go back to the comparison with mass and velocity/momentum, there are conditions in which the (effective) mass will be different dipending on the direction of momentum (e.g. in many crystals) and these can be represented by an (effective) mass tensor. The same happens with many physical objects usually considered as scalars such as conductivity, index of refraction, etc.
The simplest way to see how each component contributes to the inertia tensor is by using a system constituted by a single mass rotating around a prefixed axis with (variable) angular velocity
ω
Let us consider the origin as the pole for momentum calculation and a rotation axis passing through the origin/pole
L=
OPxm
v=
OPxm(
ωx
OP)=m(|
OP|^2-
OPOP)
ω=
Iω
Now if you want to extend the concept to a system of masses you need to have a system in which the velocity of each mass point can be written as a vector product of the SAME angular velocity and position.
In general this is possible for rigid systems only after separating the contribution of the center of mass.
Mathworld link for angular momentum (
http://scienceworld.wolfram.com/physics/AngularMomentum.html) could help but beware that it is full of little mistakes and it does not even mention that its calculation of the inertia tensor works only for rigid systems.
Hope this helps, Dario