The electrostatic view on M-theory LLM geometries
Aristomenis Donos, Joan Simon
TL;DR
The work provides a concrete electrostatic reformulation of the LLM sector in M-theory, recasting the non-linear Toda system as Laplace’s equation under a U(1) isometry and formulating a boundary-value problem for both regular and superstar-like geometries. It identifies the building blocks of regular vacua as semi-infinite line charges plus conducting disks (or planes) and derives explicit flux quantisation conditions that fix AdS radii and M2/M5 charges, yielding finite-$L$ masses consistent with BPS bounds. The paper then extends to excited states via multi-disk configurations, derives mass formulas $M_4 = \frac{1}{2L_4}\sum_{i}\sum_{j=1}^{i} N_2^{j} N_5^{i}$ and $M_7 = \frac{2}{L_7}\sum_{i}\sum_{j=1}^{i} N_2^{j} N_5^{i}$, and shows a clear connection between continuous disk distributions and superstar singularities. Overall, the results provide a precise dictionary between electrostatic data, flux quantisation, and gravitational masses for half-BPS M-theory geometries, clarifying the microstate interpretation of both regular and singular LLM configurations.
Abstract
We describe the geometry of the R x SO(3) x SO(6) x U(1) invariant half-BPS M-theory configurations considered in LLM in terms of their electrostatic variables. We discuss both regular configurations, such as AdS_4 x S^7 and AdS_7 x S^4 vacua or simple excited solutions, and singular ones such as the superstar geometries. This allows us to identify the appropriate boundary conditions describing the most general smooth and superstar-like singular configurations. We also compute their masses, matching the expected result from their microscopic interpretation, but now at finite radius of curvature.
