Shear-free Null Quasi-Spherical Spacetimes
Robert Bartnik

TL;DR
This paper investigates the residual gauge freedom in null quasi-spherical spacetimes, providing explicit formulas for key solutions, which aids in numerical relativity testing.
Contribution
It characterizes the gauge freedom in shear-free null foliations and derives explicit formulas for important spacetime solutions.
Findings
Explicit formulas for gauge transformations in Minkowski, Schwarzschild, Robinson-Trautman spacetimes
Identification of boost and rotation freedoms at each sphere
Application to numerical relativity test metrics
Abstract
The residual gauge freedom within the null quasi-spherical coordinate condition is studied, for spacetimes admitting an expanding, shear-free null foliation. The freedom consists of a boost and rotation at each coordinate sphere, corresponding to a specification of inertial frame at each sphere. Explicit formulae involving arbitrary functions of two variables are obtained for the accelerated Minkowski, Schwarzschild, and Robinson-Trautman spacetimes. These examples will be useful as test metrics in numerical relativity.
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