Warp factor and the gravitational wave spectrum
Abstract
A distinct signature of compact extra dimensions would be a Kaluza-Klein tower of gravitational waves. Motivated by this prospect, we compute the corresponding spectrum on a warped toroidal background. We evaluate in particular the impact of the warp factor on the spectrum. To that end, we use the complete warp factor H of standard string compactifications, generated by D-branes and orientifolds, thus connecting to recent works on stringy de Sitter constructions. The problematic region close to an orientifold where H < 0 leads to unphysical tachyonic modes in the spectrum. We develop tools that overcome this difficulty and lead to a tachyon-free spectrum. We show, in particular, that the warp factor can lower the first Kaluza-Klein mass by at least 69%.
Keywords
Cite
@article{arxiv.2103.09240,
title = {Warp factor and the gravitational wave spectrum},
author = {David Andriot and Paul Marconnet and Dimitrios Tsimpis},
journal= {arXiv preprint arXiv:2103.09240},
year = {2021}
}
Comments
v2: 38 pages, 11 figures, minor modifications and few additions, published version