Generalised Holonomy for Higher-Order Corrections to Supersymmetric Backgrounds in String and M-Theory
H. Lu, C.N. Pope, K.S. Stelle

TL;DR
This paper explores how higher-order string and M-theory corrections modify the structure and holonomy groups in supergravity backgrounds, enabling supersymmetry to persist despite the breakdown of traditional Riemannian holonomy.
Contribution
It introduces the concept of generalized holonomy groups accounting for higher-order corrections, extending the understanding of supersymmetric backgrounds in string and M-theory.
Findings
Higher-order corrections enlarge structure and holonomy groups.
Corrected equations can induce non-zero form fields, further enlarging groups.
Generalized holonomies preserve supersymmetry beyond Riemannian limits.
Abstract
The notion of {\it generalised structure groups} and {\it generalised holonomy groups} has been introduced in supergravity, in order to discuss the spinor rotations generated by commutators of supercovariant derivatives when non-vanishing form fields are included, with their associated gamma-matrix structures that go beyond the usual \Gamma_{MN} of the Riemannian connection. In this paper we investigate the generalisations to the usual Riemannian structure and holonomy groups that result from the inclusion of higher-order string or M-theory corrections in the supercovariant derivative. Even in the absence of background form fields, these corrections introduce additional terms \Gamma_{M_1... M_6} in the supercovariant connection, and hence they lead to enlarged structure and holonomy groups. In some cases, the corrected equations of motion force form fields to become non-zero too, which…
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