Domain Walls in Massive Supergravities
Abstract
We show how toroidally-compactified eleven-dimensional supergravity can be consistently truncated to yield a variety of maximally-supersymmetric ``massive'' supergravities in spacetime dimensions . The mass terms arise as a consequence of making a more general ansatz than that in usual Kaluza-Klein dimensional reduction, in which one or more axions are given an additional linear dependence on one of the compactification coordinates. The lower-dimensional theories are nevertheless consistent truncations of eleven-dimensional supergravity. Owing to the fact that the generalised reduction commutes neither with U-duality nor with ordinary dimensional reduction, many different massive theories can result. The simplest examples arise when just a single axion has the additional linear coordinate dependence. We find five inequivalent such theories in D=7, and 71 inequivalent ones in D=4. The massive theories admit no maximally-symmetric vacuum solution, but they do admit -brane solutions, i.e. domain walls, which preserve half the supersymmetry. We present examples of these solutions, and their oxidations to D=11. Some of the latter are new solutions of D=11 supergravity.
Cite
@article{arxiv.hep-th/9608173,
title = {Domain Walls in Massive Supergravities},
author = {P. M. Cowdall and H. Lu and C. N. Pope and K. S. Stelle and P. K. Townsend},
journal= {arXiv preprint arXiv:hep-th/9608173},
year = {2009}
}
Comments
latex, 32 papes, no figures, further comments and references added