RICHARDSON ORBITS FOR REAL CLASSICAL GROUPS
PETER E. TRAPA
Abstract. For classical real Lie groups, we compute the annihilators and asso ciated vari-
eties of the derived functor mo dules cohomologically induced from the trivial representation.
(Generalizing the standard terminology for complex groups, the nilp otent orbits that arise
as such asso ciated varieties are called Richardson orbits.) We show that every complex
sp ecial orbit has a real form which is Richardson. As a consequence of the annihilator
calculations, we give many new in nite families of simple highest weight mo dules with ir-
reducible asso ciated varieties. Finally we sketch the analogous computations for singular
derived functor mo dules in the weakly fair range and, as an application, outline a metho d
to detect nonnormality of complex nilp otent orbit closures.
1. Introduction
Fix a complex reductive Lie group, and consider its adjoint action on its Lie algebra g.
If q = l u is a parab olic subalgebra, then the G saturation of u admits a unique dense
orbit, and the nilp otent orbits which arise in this way are called Richardson orbits (following
their initial study in [R]). They are the simplest kind of induced orbits, and they play an
imp ortant role in the representation theory of G.
It is natural to extend this construction to the case of a linear real reductive Lie group
G . Let g denote the Lie algebra of G , write g for its complexi cation, and G for the
R R R
complexi cation of G . Let denote the Cartan involution of G , write g = k p for
R R
the complexi ed Cartan decomp osition, and let K denote the corresp onding subgroup of G.
Instead of considering nilp otent orbits of G on g , we work on the other side of the Kostant-
R R
Sekiguchi bijection and consider nilp otent K orbits on p. (As a matter of terminology, we say
that such an orbit O is a K -form of its G saturation.) Fix a -stable parab olic subalgebra
K
q = l u of g. Then the K saturation of u \ p admits a unique dense orbit, and we call the
orbits that arise in this way Richardson. It is easy to check that this de nition reduces to
the one given ab ove if G is itself complex.
R
It is convenient to give a slightly more geometric formulation of this de nition. A -stable
parab olic q de nes a closed orbit K q of K on G=Q (where Q is the corresp onding parab olic