The basis of Goryachev's analysis [1] of conserved scalar phase-ordering dynamics, to apply only the global constraint ψdx = const., is incorrect. For physical conserved systems, which evolve by mass transport, the stronger local conservation law embodied by the continuity equationis the appropriate one to use [2]. Even as an approximation, the global constraint is inadequate [3]. The standard evolution equation for systems with conserved dynamics iswhere2 is the effective free energy. These dynamics satisfy the local conservation law (1), and are motivated phenomenologically by a current j = −∇δF/δψ. At very early times after a quench from a disordered state, gradients will be large and higher order gradient terms will be needed. Other disagreements with (2) can stem, for example, from hydrodynamic, thermal, and stress relaxation effects. These indicate important extensions needed to (2) and F [ψ], however the local conservation (1) will still apply in all of these cases.A special initial condition emphasizes the differences in the microscopic evolution of local vs. global conservation, where we only require that the dissipative dynamics be invariant under ψ → −ψ and that F [ψ] is minimized by ψ = ±1 everywhere. Consider two half spaces, antisymmetric about a static flat domain wall, one of which has ψ = 1 everywhere except for a small sphere where ψ = −1, the other of which has ψ = +1 and −1 respectively. For spheres far from the domain wall, under local conserved dynamics the total magnetization of each half space will be constant as the spheres evolve. However with only global conservation, always satisfied by the symmetry of the problem, the dynamics are identical to non-conserved dynamics and the magnetization of each half-space will evolve in time and will eventually saturate. This is clearly inconsistent with a local conservation law.The differences between the global constraint and a local conservation law is also made clear by a class of dynamics introduced by Onuki [4] that includes both cases. In Fourier space we havewhere σ = 2 is the locally conserved dynamics of (2), σ → 0 + imposes the global constraint discussed by Goryachev, and σ = 0 is non-conserved dynamics. The differences between local and global conservation laws can be clearly seen in the late time behavior after a quench, which must be governed by the same non-linear dynamics as the early-time behavior. As discussed in a unified treatment [5] of (3), and in agreement with previous results [2], the growth laws are L(t) ∼ t 1/3 for (locally) conserved scalar quenches, and L(t) ∼ t 1/2 for non-conserved and globally constrained quenches, where t is the time since the quench. L(t) also describes the radius of the spheres in the previous paragraph, evolving by (3), where t is the time to annihilation.We can also consider long-range interactions within the effective free-energy F [ψ]. These are relevant both for attractive [5] and for repulsive [6], or competing, interactions. The free-energy should enter into the dynamics the same way, indep...