The motivation of course comes from physics: under suitable simplifying assumptions, a Lorentzian spacetime is locally $(M \times \mathbb R,g - dt^2)$ for $(M,g)$ a Riemannian 3-manifold, and the local mass density $T_{tt}$ of the stress-energy tensor is equal to the scalar curvature of $g$. Thus the assumption of non-negative scalar curvature of $(M,g)$ in the the positive mass theorem corresponds to the weak energy condition for the spacetime. In colloquial terms, the total energy must be non-negative if the local energy density is non-negative everywhere.
You should be able to find detailed discussion of this matter in many texts on general relativity - I won't try to go in to detail because my physics is very rusty, and there are a lot of subtleties when trying to define local energy. (The root of this is the lack of any well-defined notion of "gravitational energy density" in GR.) My first recommendation would be Chapter 11 of Wald's book.
Maybe something shorter to start: I wrote a little about this in the first chapter of my undergraduate thesis a few years ago. I wouldn't vouch for its accuracy or depth, but hopefully it gives a decent picture of the intuition for the ADM mass and the difficulties in defining local energy.