IIB Soliton Spectra with All Fluxes Activated
Jarah Evslin
TL;DR
This work addresses the absence of a fully S-duality covariant charge classification in type IIB string theory and proposes a generalized AHSS-like framework to compute conserved RR and NS charges, conjectured to form a K-theory of dual pairs. It tests the approach by applying the Maldacena–Moore–Seiberg framework to branes on $S^3$ with both NS and RR fluxes and comparing the results to the baryon spectrum in $AdS^5\times \mathbf{RP}^5$, finding consistency in the predicted spectra and their dependence on flux quanta. The analysis reveals that charge groups can change under Brown–Teitelboim–like phase transitions, highlighting the need for a dynamic, flux-aware extension of K-theory and its extension maps. The paper also explores dielectric D9-branes and speculates about a K-theory of dual pairs that may refine conventional K-theory by encoding dual gauge data, outlining concrete directions for a complete, duality-consistent classification of IIB solitons.
Abstract
Building upon an earlier proposal for the classification of fluxes, a sequence is proposed which generalizes the AHSS by computing type IIB string theory's group of conserved RR and also NS charges, which is conjectured to be a K-theory of dual pairs. As a test, the formalism of Maldacena, Moore and Seiberg (hep-th/0108100) is applied to classify D-branes, NS5-branes, F-strings and their dielectric counterparts in IIB compactified on a 3-sphere with both NS and RR background fluxes. The soliton spectra on the 3-sphere are then compared with the output of the sequence, as is the baryon spectrum in Witten's non-spin^c example, AdS^5xRP^5. The group of conserved charges is seen to change during Brown-Teitelboim-like phase transitions which change the effective cosmological constant.
