The volume of the hive polytope (or polytope of honeycombs) associated with a Littlewood–Richardson coefficient of SU, or with a given admissible triple of highest weights, is expressed, in the generic case, in terms of the Fourier transform of a convolution product of orbital measures. Several properties of this function – a function of three non-necessarily integral weights or of three multiplets of real eigenvalues for the associated Horn problem – are already known. In the integral case it can be thought of as a semi-classical approximation of Littlewood–Richardson coefficients. We prove that it may be expressed as a local average of a finite number of such coefficients. We also relate this function to the Littlewood–Richardson polynomials (stretching polynomials) i.e. to the Ehrhart polynomials of the relevant hive polytopes. Several SU examples, for , are explicitly worked out.
Cite this article
Robert Coquereaux, Jean-Bernard Zuber, From orbital measures to Littlewood–Richardson coefficients and hive polytopes. Ann. Inst. Henri Poincaré Comb. Phys. Interact. 5 (2018), no. 3, pp. 339–386DOI 10.4171/AIHPD/57