  We adapt the post-Newtonian gravitational-radiation methods developed within
general relativity by Epstein and Wagoner to the gravitation theory with
torsion, recently proposed by Hehl et al., and show that the two theories
predict in this approximation the same gravitational radiation losses. Since
they agree also on the first post-Newtonian level, they are at the present time
- observationally - indistinguishable.
