Abstract.
A representation of spatial infinity based on the properties of conformal geodesics is used to obtain asymptotic expansions of the gravitational field near the region where null infinity touches spatial infinity. These expansions show that generic time symmetric initial data with an analytic conformal metric at infinity will give rise to developments with a certain type of logarithmic singularities at the points where null infinity and spatial infinity meet. These logarithmic singularities produce a non-smooth null infinity. The sources of the logarithmic singularities are traced back down to the initial data. It is shown that if the parts of the initial data responsible for the non-regular behaviour of the solutions are not present, then the initial data is static to a certain order. On the basis of these results it is conjectured that the only time symmetric data sets with developments having a smooth null infinity are those which are static in a neighbourhood of infinity. This conjecture generalises a previous conjecture regarding time symmetric, conformally flat data. The relation of these conjectures to Penrose’s proposal for the description of the asymptotic gravitational field of isolated bodies is discussed.
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Communicated by G.W. Gibbons
Acknowledgements I would like to thank H. Friedrich who introduced me to this research topic and has provided me with invaluable advice. I also acknowledge several enriching and helpful discussions with R. Beig, S. Dain and J. Winicour. I also thank an anonymous referee for a careful reading of the manuscript and an important observation leading to Lemma 4. This work is funded by a Lise Meitner fellowship (M690-N02 and M814-N02) of the Fonds zur Forderung der Wissenschaftlichen Forschung (FWF), Austria. The computer algebra calculations here described have been performed in the computer facilities of the Albert Einstein Institute, Max Planck Institute für Gravitationsphysik, Golm, Germany.
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Kroon, J. Does Asymptotic Simplicity Allow for Radiation Near Spatial Infinity?. Commun. Math. Phys. 251, 211–234 (2004). https://doi.org/10.1007/s00220-004-1174-8
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DOI: https://doi.org/10.1007/s00220-004-1174-8