### 5.4 Asymptotically static and stationary spacetimes

Update
By defining asymptotically static or stationary spacetimes as those asymptotically-flat spacetimes where
the asymptotic variables are ‘time’ independent, i.e., independent, we can look at our procedure
for transforming to the complex center of mass (or complex center of charge). This example,
though very special, has the huge advantage in that it can be done exactly, without the use of
perturbations [2].
Imposing time independence on the asymptotic Bianchi identities, Equations (56) – (58),

and reality condition
we have, using Equations (51) and (52) with , that
From Equation (252), we find (after a simple calculation) that the imaginary part of is determined
by the ‘magnetic’ [44] part of the Bondi shear (spin-weight ) and thus must contain harmonics only
of . But from Equation (250), we find that contains only the harmonic. From this it
follows that the ‘magnetic’ part of the shear must vanish. The remaining part of the shear, i.e., the ‘electric’
part, which by assumption is time independent, can be made to vanish by a supertranslation, via the Sachs
theorem:

In this Bondi frame, (i.e., frame with a vanishing shear), Equation (251), implies that
using the conventionally accepted physical identification of the complex gravitational dipole. (Since the
shear vanishes, this agrees with probably all the various attempted identifications.)
From the mass identification, becomes

Since the Bondi shear is zero, the asymptotically shear-free congruences are determined by the same GCFs
as in flat spaces, i.e., we have
Our procedure for the identification of the complex center of mass, namely setting in the
transformation, Equation (276),

leads, after using Equations (254), (249) and (257), to

From the time independence, , the spatial part of the world line is a constant vector. By a (real)
spatial Poincaré transformation (from the BMS group), the real part of can be made to vanish, while
by ordinary rotation the imaginary part of can be made to point in the three-direction. Using the the
gauge freedom in the choice of we set . Then pulling all these items together, we
have for the complex world line, the UCF, and the angular momentum, :

Thus, we have the complex center of mass on the complex world line, .
These results for the lower multipole moments, i.e., , are identical to those of the Kerr metric.
The higher moments are still present (appearing in higher terms in the Weyl tensor) and are not
affected by these results.