English

Supersymmetric Backgrounds and Generalised Special Holonomy

High Energy Physics - Theory 2016-07-07 v1 Differential Geometry

Abstract

We define intrinsic torsion in generalised geometry and use it to introduce a new notion of generalised special holonomy. We then consider generic warped supersymmetric flux compactifications of M theory and Type II of the form RD1,1×M\mathbb{R}^{D-1,1}\times M. Using the language of Ed(d)×R+E_{d(d)}\times\mathbb{R}^+ generalised geometry, we show that, for D4D\geq 4, preserving minimal supersymmetry is equivalent to the manifold MM having generalised special holonomy and list the relevant holonomy groups. We conjecture that this result extends to backgrounds preserving any number of supersymmetries. As a prime example, we consider N=1\mathcal{N}=1 in D=4D=4. The corresponding generalised special holonomy group is SU(7)SU(7), giving the natural M theory extension to the notion of a G2G_2 manifold, and, for Type II backgrounds, reformulating the pure spinor SU(3)×SU(3)SU(3)\times SU(3) conditions as an integrable structure.

Keywords

Cite

@article{arxiv.1411.5721,
  title  = {Supersymmetric Backgrounds and Generalised Special Holonomy},
  author = {André Coimbra and Charles Strickland-Constable and Daniel Waldram},
  journal= {arXiv preprint arXiv:1411.5721},
  year   = {2016}
}

Comments

33 pages

R2 v1 2026-06-22T07:06:40.119Z