Abstract

In this paper we deal with radiation from heavy quarks in the context of next-to-leading order calculations matched to parton shower generators. A new algorithm for radiation from massive quarks is presented that has considerable advantages over the one previously employed. We implement the algorithm in the framework of the POWHEG-BOX, and compare it with the previous one in the case of the hvq generator for bottom production in hadronic collisions, and in the case of the bb4l generator for top production and decay.

Highlights

  • The production and detection of bottom quarks play an important rôle in various contexts in LHC physics

  • The purpose of the present paper is twofold: we present a new algorithm for radiation from a heavy quark, that has proven superior to the old one; we perform a thorough investigation of the behaviour of this component of the POWHEG generator, by comparing the two methods, both in the framework of bottom quarks generated in top decay, and in inclusive bottom quark pair production

  • In this paper we have presented a method for implementing radiation from a heavy quark in the POWHEG framework

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Summary

Introduction

The production and detection of bottom quarks play an important rôle in various contexts in LHC physics. There are reasons to give an adequate treatment to final state radiation from a high transverse momentum bottom quark This radiation process is intimately related to the physics of the bottom fragmentation function, and may have important effects in processes of considerable interest, like for example in top decay. The purpose of the present paper is twofold: we present a new algorithm for radiation from a heavy quark, that has proven superior to the old one; we perform a thorough investigation of the behaviour of this component of the POWHEG generator, by comparing the two methods, both in the framework of bottom quarks generated in top decay, and in inclusive bottom quark pair production. The paper is organized as follows: in Sect. 2 we describe the new algorithm, in Sect. 3 we illustrate our phenomenological studies, and in Sect. 4 we give our conclusions

The POWHEG mapping for the massive emitter case
Mr2ec q 2
Inverse map
Full kinematic reconstruction of the real emission
Generation of radiation
Upper bound function
Integral of the upper bound function
We generate a uniform random number
Comparison in the bb4l case
Problematic regions
Conclusions
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