Stability conditions and related filtrations for (G,h)-constellations

Abstract

Given an infinite reductive algebraic group G, we consider G-equivariant coherent sheaves with prescribed multiplicities, called (G,h)-constellations, for which two stability notions arise. The first one is analogous to the θ-stability defined for quiver representations by King and for G-constellations by Craw and Ishii, but depending on infinitely many parameters. The second one comes from Geometric Invariant Theory in the construction of a moduli space for (G,h)-constellations, and depends on some finite subset D of the isomorphy classes of irreducible representations of G. We show that these two stability notions do not coincide, answering negatively a question raised in [BT15]. Also, we construct Harder-Narasimhan filtrations for (G,h)-constellations with respect to both stability notions (namely, the μθ-HN and μD-HN filtrations). Even though these filtrations do not coincide in general, we prove that they are strongly related: the μθ-HN filtration is a subfiltration of the μD-HN filtration, and the polygons of the μD-HN filtrations converge to the polygon of the μθ-HN filtration when D grows.

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