Kerr-Schild spacetimes with (A)dS background
classification
🌀 gr-qc
hep-th
keywords
spacetimeskerr-schildbackgroundtypeweylallowsarbitraryboost
pith:HSY5YNBJ Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{HSY5YNBJ}
Prints a linked pith:HSY5YNBJ badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
General properties of Kerr-Schild spacetimes with (A)dS background in arbitrary dimension are studied. It is shown that the geodetic Kerr-Schild vector k is a multiple WAND of the spacetime. Einstein Kerr-Schild spacetimes with non-expanding k are shown to be of Weyl type N, while the expanding spacetimes are of type II or D. It is shown that this class of spacetimes obeys the optical constraint. This allows us to solve Sachs equation, determine r-dependence of boost weight zero components of the Weyl tensor and discuss curvature singularities.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.