  A stress-energy tensor for linear gravity adapted to the harmonic gauge was
recently proposed by Butcher, Hobson and Lasenby. By removing gauge constraints
and imposing full metrical GR, we find a natural generalisation to the
pseudotensor of Einstein. M{\o}ller's pseudotensor is an alternative to that of
Einstein formulated using tetrads. We obtain the pseudotensor of M{\o}ller for
gauge theory gravity (GTG) using a variational approach, identifying a
potentially interesting recipe for constructing conserved currents in that
theory. We show that in static, spherical spacetimes with a central
gravitational mass M{\o}ller's pseudotensor describes gravitational
stress-energy as if the gravitational potential were a scalar (i.e.
Klein-Gordon) field coupled to a gravitational mass density on the Minkowski
background. The old Newtonian formula successfully describes the potential of
even strong fields in this picture. The Newtonian limit of this effect was
previously observed in the tensor of Butcher; we recover a local virial theorem
in this limit. We demonstrate using the `Schwarzschild star' solution for an
incompressible perfect fluid ball.
