BMN Vacua, Superstars and Non-Abelian T-duality
Abstract
Acting with non-Abelian T-duality on the inside the subspace of with units of flux, we generate a new half-BPS solution with symmetry that belongs to the Lin-Lunin-Maldacena class of geometries. The analysis of the asymptotics, quantised charges and probe branes in this geometry suggests an interpretation as the gravity dual to the Berenstein-Maldacena-Nastase Plane Wave Matrix Model, in a particular vacuum associated to a partition of , in which the multiplicity of each irreducible representation is equal to its dimension. This vacuum is interpreted in M-theory in terms of giant gravitons backreacting in the maximally supersymmetric pp-wave geometry. Consistently with this, we show that the non-Abelian T-dual solution exactly agrees with the Penrose limit of the superstar solution in . This suggests an interesting global completion of the non-Abelian T-dual solution in terms of an M5-brane geometry.
Keywords
Cite
@article{arxiv.1703.00417,
title = {BMN Vacua, Superstars and Non-Abelian T-duality},
author = {Yolanda Lozano and Carlos Nunez and Salomon Zacarias},
journal= {arXiv preprint arXiv:1703.00417},
year = {2017}
}
Comments
28 pages, discussion in section 5.1 improved, results unchanged, reference added. Matches published version