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Fully automated precision predictions for heavy neutrino production mechanisms at hadron colliders

Céline DegrandeInstitute for Particle Physics Phenomenology, Department of Physics, Durham University, Durham DH1 3LE, United KingdomOlivier MattelaerInstitute for Particle Physics Phenomenology, Department of Physics, Durham University, Durham DH1 3LE, United KingdomRichard RuízInstitute for Particle Physics Phenomenology, Department of Physics, Durham University, Durham DH1 3LE, United KingdomJessica TurnerInstitute for Particle Physics Phenomenology, Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
2016en
ABI

Аннотация

Motivated by TeV-scale neutrino mass models, we propose a systematic treatment of heavy neutrino ($N$) production at hadron colliders. Our simple and efficient modeling of the vector boson fusion (VBF) ${W}^{\ifmmode\pm\else\textpm\fi{}}\ensuremath{\gamma}\ensuremath{\rightarrow}N{\ensuremath{\ell}}^{\ifmmode\pm\else\textpm\fi{}}$ and $N{\ensuremath{\ell}}^{\ifmmode\pm\else\textpm\fi{}}+nj$ signal definitions resolve collinear and soft divergences that have plagued past studies, and is applicable to other color-singlet processes, e.g., associated Higgs $({W}^{\ifmmode\pm\else\textpm\fi{}}h)$, sparticle $({\stackrel{\texttildelow{}}{\ensuremath{\ell}}}^{\ifmmode\pm\else\textpm\fi{}}\stackrel{\texttildelow{}}{{\ensuremath{\nu}}_{\ensuremath{\ell}}})$, and charged Higgs $({h}^{\ifmmode\pm\else\textpm\fi{}\ifmmode\pm\else\textpm\fi{}}{h}^{\ensuremath{\mp}})$ production. We present, for the first time, a comparison of all leading $N$ production modes, including both gluon fusion (GF) $gg\ensuremath{\rightarrow}{Z}^{*}/{h}^{*}\ensuremath{\rightarrow}N\stackrel{(\ensuremath{-})}{{\ensuremath{\nu}}_{\ensuremath{\ell}}}$ and VBF. We obtain fully differential results up to next-to-leading order (NLO) in QCD accuracy using a Monte Carlo tool chain linking feynrules, nloct, and madgraph5_amc@nlo. Associated model files are publicly available. At the 14 TeV LHC, the leading order GF rate is small and comparable to the NLO $N{\ensuremath{\ell}}^{\ifmmode\pm\else\textpm\fi{}}+1j$ rate; at a future 100 TeV Very Large Hadron Collider, GF dominates for ${m}_{N}=300--1500\text{ }\text{ }\mathrm{GeV}$, beyond which VBF takes the lead.

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Цитирований: 3Использованных источников: 0