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RESEARCH PRODUCT

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

Alfonso ZamoraRonan Terpereau

subject

Pure mathematicsGeneral Mathematics01 natural sciencesHarder–Narasimhan filtrationCoherent sheafModuliMathematics - Algebraic GeometryMathematics::Algebraic Geometry0103 physical sciencesFOS: MathematicsComputer Science::General Literature14D20 14L24Representation Theory (math.RT)0101 mathematicsAlgebraic Geometry (math.AG)MathematicsComputer Science::Information Retrieval010102 general mathematicsQuiverAstrophysics::Instrumentation and Methods for AstrophysicsGIT quotientComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)16. Peace & justiceModuli spaceGIT quotientStability conditionAlgebraic groupIrreducible representationMSC: 14D20 14L24010307 mathematical physicsGeometric invariant theory[MATH.MATH-AG]Mathematics [math]/Algebraic Geometry [math.AG]Mathematics - Representation Theory

description

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 $\theta$-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 $\mu_{\theta}$-HN and $\mu_D$-HN filtrations). Even though these filtrations do not coincide in general, we prove that they are strongly related: the $\mu_{\theta}$-HN filtration is a subfiltration of the $\mu_D$-HN filtration, and the polygons of the $\mu_D$-HN filtrations converge to the polygon of the $\mu_{\theta}$-HN filtration when $D$ grows.

10.1142/s0129167x17500987https://hal.archives-ouvertes.fr/hal-01620368v2/file/stability_of_constellations_final_version.pdf