This equation appears to be based on finding the relativistic mass, which if I've understood the book's symbology correctly, the author calls \rho_0(r) as a function of r.
Unfortunately, as I noted earlier:
The correct formulation for the i'th component of momentum in flat space-time is
P^i = \int T^{0i} dV
where T^{ij} is the stress-energy tensor. The 0'th component of the momentum is the energy.
This is based on the fact that one of the interpretations of the stress-energy tensor is that T \cdot u gives the density of energy-momentum in a region, where T is the stress-energy tensor and u is the 4-velocity, see for instance MTW's "Gravitation". (You'll probably find similar remarks in Rindler as well with different notation.)
To deal with spherical coordinates in flat-space-time it might be useful to note that one would more generally write:
P^i = \int \sqrt{\left| T^{0i}\,T_{0i} \right| }\, dV
(I believe this is correct, but it's from fallible memory, not directly from a textbook).
The issue of how to deal with non-flat space-times gets much more involved, but hopefully we don't need to get into that. I'll just point out that one needs certain preconditions to even *define* the total energy or total momentum in a non-flat space-time.
Because the stress terms in the stress-energy tensor do affect the momentum, one would need a complete material model, including the stresses, to find the answer. The issue is complicated by the non-existence of a Born-rigid spherical spinning body, see for instance the sci.physics.faq, so it's not clear that the notion of a rigid sphere spinning at light speed at its periphery makes any physical sense.
See
The rigid rotating disk in relativity for a popular discussion and some references. The result for the non-existence of a spinning Born-rigid sphere is due to Ehrenfest, and is the well-known Ehrenfest paradox which Chris Hillman talked about.
The associated faq entry is: