Twisted Homology
Andres Collinucci, Jarah Evslin
TL;DR
The paper argues that on a simply-connected six-manifold, twisted K-theory, which classifies D-branes, is isomorphic to twisted homology, a more computable and degree-flexible framework that also extends to M-branes. It introduces a geometric realization of twisted homology via cycles in a spacetime bundle $Q$ (and a simpler subbundle $P$ when available), and constructs a spectral sequence with differentials $d_{2i+1}$ that converges to twisted homology, capturing multistep brane decays such as MMS/KPV transitions. The authors provide a concrete cohomological computation using the Gysin sequence, giving an explicit formula for $H$-cohomology in terms of the total space $P$, and illustrate with examples: the SU(2) WZW model on $S^3$ and a lens space, showing how charges and anomalies align with twisted homology predictions. This framework yields a practical, bijective bridge between brane configurations, anomalies, and conserved charges, facilitating background-brane analyses in string phenomenology and extending naturally to M-theory contexts.
Abstract
D-branes are classified by twisted K-theory. Yet twisted K-theory is often hard to calculate. We argue that, in the case of a compactification on a simply-connected six manifold, twisted K-theory is isomorphic to a much simpler object, twisted homology. Unlike K-theory, homology can be twisted by a class of any degree and so it classifies not only D-branes but also M-branes. Twisted homology classes correspond to cycles in a certain bundle over spacetime, and branes may decay via Kachru-Pearson-Verlinde transitions only if this cycle is trivial. We provide a spectral sequence which calculates twisted homology, the kth step treats D(p-2k)-branes ending on Dp-branes.
