NNLO QCD predictions of the asymmetry probe of the Z γ pair-production process

• Published in: Physica scripta Vol. 99; no. 2; pp. 25302 - 25319
• Main Author: Saygin, Kadir
• Format: Journal Article
• Language: English
• Published: IOP Publishing 01.02.2024
• Subjects: asymmetry in Z; hadron collider phenomenology; NNLO QCD predictions; pair production; process
• ISSN: 0031-8949; 1402-4896
• DOI: 10.1088/1402-4896/ad1860

Abstract The paper presents for the first time a novel idea of exploiting asymmetry between differential cross sections of the off-shell Z γ pair-production in proton-proton ( pp ) collisions for the final states of a charged-lepton pair plus a photon pp → Z γ → l + l − γ (leptonic decay) and of a neutrino pair plus a photon pp → Z γ → ν ν ¯ γ (invisible decay). Asymmetry between the leptonic and invisible decays of the Z γ process is investigated by using fixed-order predictions through inclusion of next-to-next-to-leading (NNLO) radiative corrections in quantum chromodynamics (QCD) perturbation theory. NNLO QCD predictions are presented at various pp -collision energies as functions of several key observables including transverse momenta and azimuthal-angle separation, regarding the Z γ decay products. The predicted distributions for the Z γ asymmetry are provided based on realistic fiducial phase-space requirements in line with the related hadron-collider measurements. The predicted distributions are assessed at various pp -collision energies and in different phase-space regions such as with higher lepton-pair invariant mass m l + l − or higher neutrino-pair transverse momentum p T ν ν ¯ requirements. The Z γ asymmetry is shown to be significantly sensitive in different regions of phase space including high- m l + l − and high- p T ν ν ¯ regions. The Z γ asymmetry can therefore be translated into an important quantity for probing deviation from the Standard Model (SM) predictions. In this regard, the asymmetry probe is proposed as a sensitive indicator for indirect searches for physics beyond the SM encompassing high-mass resonances and dark-matter sector.