Abstract

Abstract In previous work we have shown that the equivariant index of multi-centered $ \mathcal{N}=2 $ black holes localizes on collinear configurations along a fixed axis. Here we provide a general algorithm for enumerating such collinear configurations and computing their contribution to the index. We apply this machinery to the case of black holes described by quiver quantum mechanics, and give a systematic prescription — the Coulomb branch formula — for computing the cohomology of the moduli space of quiver representations. For quivers without oriented loops, the Coulomb branch formula is shown to agree with the Higgs branch formula based on Reineke’s result for stack invariants, even when the dimension vector is not primitive. For quivers with oriented loops, the Coulomb branch formula parametrizes the Poincaré polynomial of the quiver moduli space in terms of single-centered (or pure-Higgs) BPS invariants, which are conjecturally independent of the stability condition (i.e. the choice of Fayet-Iliopoulos parameters) and angular-momentum free. To facilitate further investigation we provide a Mathematica package “CoulombHiggs.m” implementing the Coulomb and Higgs branch formulae.

Highlights

  • This comparison is complicated by the fact that on the macroscopic side, contributions to the index Ω(γ) originate from single centered black holes with charge γ, and from multi-centered black holes with constituents carrying charges {αi} such that γ = αi [4,5,6,7]

  • In previous work we have shown that the equivariant index of multi-centered N = 2 black holes localizes on collinear configurations along a fixed axis

  • We apply this machinery to the case of black holes described by quiver quantum mechanics, and give a systematic prescription — the Coulomb branch formula — for computing the cohomology of the moduli space of quiver representations

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Summary

A formula for the Coulomb index of multi-centered black holes

We establish a recursive algorithm for computing the Coulomb index gCoulomb({α1, · · · αn}; {c1, · · · cn}; y) for general charge configurations αi, away from the walls of marginal stability in the space of FI parameters ci. For this we first deform all the vanishing αij’s to non-zero values in such a way that the deformed quiver does not have any oriented loop To see that this is always possible, let us carry out the deformation one link at a time. If so let us flip the sign of αij of the deformed link In this case C together with the added link no longer forms an oriented loop. We can repeat the argument and show that all the vanishing αij’s can be made non-zero and for appropriate choice of sign of the deformed αij’s the new quiver does not have any oriented loop.

Generic Abelian quivers with all αij non-zero
An inductive formula for the index of collinear solutions
An inductive formula for the index of scaling collinear solutions
Coulomb index for 3 and 4 centers
Quiver invariants
Quiver Poincare-Laurent polynomial from Coulomb index: a review
Coulomb index for non-generic charges
Reineke’s formula for quivers without loops
Abelian quivers without loops
Non-Abelian quivers with primitive dimension vector and without loops
Non-primitive dimension vector
A The Mathematica package “CoulombHiggs”
Symbols
Environment variables
Coulomb index
Coulomb branch formula
Higgs branch formula
Utilities
Full Text
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