Abstract

The form factors of the Lambda _{b} rightarrow N^*ell ^+ ell ^- decay are calculated in the framework of the light cone QCD sum rules. In the calculations the contribution of the negative parity Lambda _b^* baryon is eliminated by constructing the sum rules for different Lorentz structures. Furthermore the branching ratio of the semileptonic Lambda _b rightarrow N^*ell ^+ ell ^- decay is calculated. The numerical study for the branching ratio of the Lambda _{b} rightarrow N^*ell ^+ ell ^- decay indicates that it is quite large and could be measurable at future planned experiments to be conducted at LHCb.

Highlights

  • N is eliminated by constructing the sum rules for different Lorentz structures

  • The numerical study for the branching ratio of the b → N ∗ + − decay indicates that it is quite large and could be measurable at future planned experiments to be conducted at LHCb

  • In order to derive the light cone QCD sum rules method (LCSR) for these form factors we introduce the correlation function μj ( p, q) = i d4xeiqx 0 | T {η b (0) Jμj (x)} | N ∗( p), (4)

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Summary

Introduction

Decay in the framework of the LCSR method. The paper is organized as follows: In Sect. 2 the LCSR for the relevant form factors appearing in the b(. In the present section we derive the LCSR for the transition form factors of the b( ∗b) → N ∗ + − decay. Xq2 + x x xm Equating the coefficients of the structures pμγ, pμq/ γ5, γμγ, γμq/ γ5, qμγ, and qμq/ γ5 we get the following sum rules for the invariant functions of the transition current (bγμd),. Using the heavy quark symmetry and the soft collinear effective theory in [13,14,15] it is obtained that the matrix element for b → N ∗ transition can be in terms of only one universal function ξ( pv). For a complete description of the heavy-to-light baryon transition form factors, it is necessary to take into account non-factorizable contributions. We calculate only factorizable contributions and we plan to present a detailed analysis of the non-factorizable contributions elsewhere in future

Numerical analysis
Conclusion
16 Q 2 β T4
Q 2 T1
14 Q 2 β T5

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