On asymptotically flat algebraically special spacetimes in higher dimensions
Marcello Ortaggio, Vojtech Pravda, Alena Pravdova

TL;DR
This paper investigates the asymptotic structure of higher-dimensional vacuum spacetimes with special algebraic properties, showing they lack gravitational radiation and establishing the uniqueness of higher-dimensional Schwarzschild solutions.
Contribution
It provides a detailed analysis of asymptotic flatness and Weyl tensor behavior in higher dimensions, revealing differences from four-dimensional cases and proving uniqueness results.
Findings
Higher-dimensional algebraically special spacetimes do not exhibit peeling-off behavior.
These spacetimes do not contain gravitational radiation.
The Schwarzschild-Tangherlini metric is unique in the non-twisting case.
Abstract
We analyze asymptotic properties of higher-dimensional vacuum spacetimes admitting a "non-degenerate" geodetic multiple WAND. After imposing a fall-off condition necessary for asymptotic flatness, we determine the behaviour of the Weyl tensor as null infinity is approached along the WAND. This demonstrates that these spacetimes do not "peel-off" and do not contain gravitational radiation (in contrast to their four-dimensional counterparts). In the non-twisting case, the uniqueness of the Schwarzschild-Tangherlini metric is also proven.
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