  In the lowest nonlinear approximation I compare two gravitational wave
equations,- those of Weinberg and Papapetrou. The first one is simply a form of
Einstein equation and the second is claimed to be yet another field theoretical
form in which the energy-momentum tensor is obtained by Belinfante or Rosenfeld
method. I show that for interacting gravitational field these methods lead to
different energy-momentum tensors. Both these tensors need to be complemented
"by hand" with some interaction energy-momentum tensors in order that the
conservation laws of the total energy-momentum tensor give equation of motion
for particles in agreement with general relativity. In approximation considered
by Thirring, the Papapetrou wave equation must coincide with that of Thirring.
But they differ because Thirring inserted the necessary interaction term. I
show that Thirring wave equation is equivalent to Weinberg's one. Hence the
Papapetrou equation is not yet another form of Einstein equation.
