Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University
In: WSPC - Proceedings (2010)
Boost-rotation symmetric spacetimes are exceptional as they are the only exact asymp-
totically flat solutions to the Einstein equations describing spatially bounded sources
(“point-like” particles, black holes) undergoing non-trivial motion (“uniform accelera-
tion”) with radiation. We construct the Newtonian limit of these spacetimes: it yields
fields of uniformly accelerated sources in classical mechanics. We also study the special-
relativistic limit of
boost-rotation symmetry, C-metric, Newtonian limit
@inproceedings{UTF472,
author = {Kofroň, D. and Bičák, J.},
title = {{CLASSICAL LIMITS OF BOOST-ROTATION SYMMETRIC SPACETIMES}},
booktitle = {WSPC - Proceedings},
year = {2010},
}