Flux and charge quantization in 11-dimensional supergravity
Determine a fully consistent, non-perturbative flux- and charge-quantization law for the C-field in D=11, N=1 supergravity that fixes the global higher gauge field content (including torsion charges) and is compatible with the supergravity equations of motion.
References
In \S\ref{SuperFluxQuantization} we address the open problem of flux- and charge-quantization (see ) of $D=11$, $\mathcal{N}=1$ supergravity (11d SuGra , review in ), explaining how this is a necessary step towards the completion of 11d SuGra to the conjectured ``M-theory'' .
Especially in the presence of Romans mass, RR flux quantisation is a subtle problem. At the level of supergravity, one usually imposes Page flux quantisation , which in our conventions ($2\pi\sqrt{\alpha'}=1$), and in the gauge $B_2=0$ used here, amounts to requiring $\int_C F_4\in\mathbb Z$ for every integral 4-cycle $C\subset X_8$, i.e. $[F_4]\in H4(X_8,\mathbb Z)$. For a purely untwisted flux, we derive candidate Page quantisation conditions from the fourteen explicit orbifold coordinate cycles constructed below. Interpreting these conditions as Page quantisation conditions on the smooth resolution requires the additional assumption that these orbifold cycles lift to integral 4-cycles of $X_8$ and that the periods of the untwisted forms are unchanged under this lift. Nevertheless, more refined RR quantisation conditions have been formulated . Since we are unable to implement them explicitly for our toroidal example, we restrict ourselves to Page flux quantisation.
This proves an equality of local eight-form classes, while the corresponding global anomaly analysis is left for future work.