PreprintCC BY 4.0arXiv
Exotic gravity theory in topologically non-trivial spacetimes
Abstract
An exotic linearised theory of superconformal gravity in D=6, (4,0) superspace has been proposed by C.M. Hull. In this note we discuss the bosonic sector of this model in topologically non-trivial spaces. Roughly speaking, Hull's model can be thought of as a square of the H=dB theory, although not all Hull fields can be so presented. We also briefly discuss the form sector of D=11 supergravity.
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BibTeX
@misc{howe2026exotic,
title = {{Exotic gravity theory in topologically non-trivial spacetimes}},
author = {P. S. Howe and U. Lindström},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.35253},
eprint = {2609.35253},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.35253},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Exotic gravity theory in topologically non-trivial spacetimes
AU - P. S. Howe
AU - U. Lindström
PY - 2026
DA - 2026/09/28
PB - arXiv
DO - 10.48550/arxiv.2609.35253
UR - https://arxiv.org/abs/2609.35253
AB - An exotic linearised theory of superconformal gravity in D=6, (4,0) superspace has been proposed by C.M. Hull. In this note we discuss the bosonic sector of this model in topologically non-trivial spaces. Roughly speaking, Hull's model can be thought of as a square of the H=dB theory, although not all Hull fields can be so presented. We also briefly discuss the form sector of D=11 supergravity.
ER -