Isgur-Wise functions and unitary representations of the Lorentz group : the baryon case j = 0

TL;DR

This paper introduces a group theoretical approach to analyze Isgur-Wise functions in heavy baryon decays, providing new bounds and insights by decomposing the light cloud's Lorentz group representations.

Contribution

It develops a formalism based on unitary Lorentz group representations to derive constraints on Isgur-Wise functions, especially for the j=0 case in baryon decays, connecting sum rules with representation theory.

Findings

Recovered the curvature bound for the IW function xi_Lambda(w).

Derived new bounds for higher derivatives of the IW function.

Determined the IW function explicitly when the curvature bound is saturated.

Abstract

We propose a group theoretical method to study Isgur-Wise functions. A current matrix element splits into a heavy quark matrix element and an overlap of the initial and final clouds, related to the IW functions, that contain the long distance physics. The light cloud belongs to the Hilbert space of a unitary representation of the Lorentz group. Decomposing into irreducible representations one obtains the IW function as an integral formula, superposition of irreducible IW functions with positive measures, providing positivity bounds on its derivatives. Our method is equivalent to the sum rule approach, but sheds another light on the physics and summarizes and gives all its possible constraints. We expose the general formalism, thoroughly applying it to the case j = 0 for the light cloud, relevant to the semileptonic decay Lambda_b -> Lambda_c + l + nu. In this case, the principal series of the representations contribute, and also the supplementary series. We recover the bound for the curvature of the j = 0 IW function xi_Lambda (w) that we did obtain from the sum rule method, and we get new bounds for higher derivatives. We demonstrate also that if the lower bound for the curvature is saturated, then xi_Lambda (w) is completely determined, given by an explicit elementary function. We give criteria to decide if any ansatz for the Isgur-Wise function is compatible or not with the sum rules. We apply the method to some simple model forms proposed in the literature. Dealing with a Hilbert space, the sum rules are convergent, but this feature does not survive hard gluon radiative corrections.