Arbitrary output shifts of Grassmannian ASP permutations #
The once-marked census may be normalized to degree g, but the full
transmission theory naturally uses every shift chi. This file derives that
family from the shift-zero Grassmannian constructor without reconstructing its
inversion set a second time.
The Grassmannian permutation of lambda with ASP shift chi.
Equations
- Utilities.shiftedGrassmannianPerm lambda chi = Utilities.outputShift (Utilities.grassmannianPermOfYoungDiagram lambda) chi
Instances For
An ASP permutation is uniquely determined by its inversion set and shift.
Thus any externally presented Grassmannian permutation with the Ferrers
inversion set of lambda is definitionally the canonical shifted constructor
used in this library.
The usual shifted Grassmannian formula on nonnegative inputs.
Every partition row retains its exact slipface value after translating
the first coordinate by -chi.
Output normalization does not change existence of the associated
transmission locus; witnesses differ by chi chips at the first mark.
Conditional-on-the-explicit-Ferrers-envelope form of the arbitrary-shift Grassmannian/once-marked dictionary. The output shift changes the normalized degree of a transmission witness but not its existence problem.
Arbitrary output normalization of the unconditional Grassmannian/ once-marked dictionary.
Presentation-independent dictionary. Any ASP permutation whose inversion
set is the Ferrers set of lambda and whose shift is chi has exactly the
once-marked transmission locus, even if it was not built with the canonical
constructor.