Khan, Sarif

[["dc.bibliographiccitation.artnumber","37"],["dc.bibliographiccitation.issue","7"],["dc.bibliographiccitation.journal","Journal of High Energy Physics"],["dc.bibliographiccitation.volume","2022"],["dc.contributor.author","Biswas, Anirban"],["dc.contributor.author","Khan, Sarif"],["dc.date.accessioned","2022-08-04T12:00:08Z"],["dc.date.available","2022-08-04T12:00:08Z"],["dc.date.issued","2022-07-06"],["dc.date.updated","2022-07-25T11:18:47Z"],["dc.description.abstract","The quest for new physics beyond the Standard Model is boosted by the recently observed deviation in the anomalous magnetic moments of muon and electron from their respective theoretical prediction. In the present work, we have proposed a suitable extension of the minimal Lμ − Lτ model to address these two experimental results as the minimal model is unable to provide any realistic solution. In our model, a new Yukawa interaction involving first generation of leptons, a singlet vector like fermion (χ±) and a scalar (either an SU(2)L doublet Φ 4 ′ $ {\\Phi}_4^{\\prime } $ or a complex singlet Φ 4 ′ $ {\\Phi}_4^{\\prime } $ ) provides the additional one loop contribution to ae only on top of the usual contribution coming from the Lμ − Lτ gauge boson (Zμτ) to both electron and muon. The judicious choice of Lμ − Lτ charges to these new fields results in a strongly interacting scalar dark matter in O $ \\mathcal{O} $ (MeV) range after taking into account the bounds from relic density, unitarity and self interaction. The freeze-out dynamics of dark matter is greatly influenced by 3 → 2 scatterings while the kinetic equilibrium with the SM bath is ensured by 2 → 2 scatterings with neutrinos where Zμτ plays a pivotal role. The detection of dark matter is possible directly through scatterings with nuclei mediated by the SM Z bosons. Moreover, our proposed model can also be tested in the upcoming e+e− colliders by searching opposite sign di-electron and missing energy signal i.e. at the final state."],["dc.identifier.citation","Journal of High Energy Physics. 2022 Jul 06;2022(7):37"],["dc.identifier.doi","10.1007/JHEP07(2022)037"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/112642"],["dc.language.iso","en"],["dc.rights","CC BY 4.0"],["dc.rights.holder","The Author(s)"],["dc.subject","Cosmology of Theories BSM"],["dc.subject","Early Universe Particle Physics"],["dc.subject","Particle Nature of Dark Matter"],["dc.subject","Specific BSM Phenomenology"],["dc.title","(g − 2)e, μ and strongly interacting dark matter with collider implications"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.subtype","original_ja"],["dspace.entity.type","Publication"]]