Birational geometry of quiver varieties and other GIT quotients
Gwyn Bellamy, Alastair Craw, Travis Schedler
TL;DR
This work provides a unified, geometry-driven framework for understanding the birational maps among GIT quotients and their resolutions. By establishing Condition GIT, the authors show that a large class of quotients are relative Mori Dream Spaces and that their movable cones are controlled by the GIT chamber structure via the linearisation map. They apply this to Nakajima quiver varieties, hypertoric varieties, and certain threefold quotient singularities, proving that crepant resolutions are themselves moduli-type spaces and describing how all such resolutions arise from variation of GIT quotients. This approach yields explicit descriptions of Mov(X/Y), the Namikawa–Weyl group action, and hyperplane arrangements, circumventing reliance on the BCHM machinery and offering constructive, combinatorial tools for birational classification in this setting.
Abstract
We prove that all projective crepant resolutions of Nakajima quiver varieties satisfying natural conditions are also Nakajima quiver varieties. More generally, we classify the small birational models of many Geometric Invariant Theory (GIT) quotients by introducing a sufficient condition for the GIT quotient of an affine variety $V$ by the action of a reductive group $G$ to be a relative Mori Dream Space. Two surprising examples illustrate that our new condition is optimal. When the condition holds, we show that the linearisation map identifies a region of the GIT fan with the Mori chamber decomposition of the relative movable cone of $V /\!/_θ G$. If $V/\!/_θ G$ is a crepant resolution of $Y\!\!:= V/\!/_{0} G$, then every projective crepant resolution of $Y$ is obtained by varying $θ$. Under suitable conditions, we show that this is the case for quiver varieties and hypertoric varieties. Similarly, for any finite subgroup $Γ\subset \mathrm{SL}(3,\mathbb{C})$ whose nontrivial conjugacy classes are all junior, we obtain a simple geometric proof of the fact that every projective crepant resolution of $\mathbb{C}^3/Γ$ is a fine moduli space of $θ$-stable $Γ$-constellations.
