دورية أكاديمية

Hunting ewinos and a light scalar of Z 3-NMSSM with a bino-like dark matter in top squark decays at the LHC

التفاصيل البيبلوغرافية
العنوان: Hunting ewinos and a light scalar of Z 3-NMSSM with a bino-like dark matter in top squark decays at the LHC
المؤلفون: AseshKrishna Datta, Monoranjan Guchait, Arnab Roy, Subhojit Roy
المصدر: Journal of High Energy Physics, Vol 2023, Iss 11, Pp 1-38 (2023)
بيانات النشر: SpringerOpen, 2023.
سنة النشر: 2023
المجموعة: LCC:Nuclear and particle physics. Atomic energy. Radioactivity
مصطلحات موضوعية: Dark Matter at Colliders, Supersymmetry, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
الوصف: Abstract We explore a possible signal of the presence of relatively light electroweakinos (ewinos) and a singlet-like scalar (a S ) of the Z 3-symmetric Next-to-Minimal Supersymmetric Standard Model (Z 3-NMSSM) in the cascade decays of not so heavy top squarks ( m t ~ 1 $$ {m}_{{\tilde{t}}_1} $$ ≲ 1.5 TeV) that may be produced in pairs at the Large Hadron Collider LHC. We work in a scenario where the lightest (next-to-lightest) SUSY particle is bino (singlino)-like with its mass below 100 GeV and is mildly tempered with higgsino and singlino admixtures. The singlet-like scalar provides an annihilation funnel for the bino-like states such that the latter could act as a viable dark matter candidate, unlike what is now highly constrained in the MSSM. We consider a pair of immediately heavier neutralinos and the lighter chargino which all are higgsino-like with masses in the range ~ 0.5–1 TeV and are still compatible with all experimental constraints. While these states may not be accessible in their direct searches at the LHC in our present scenario, such ewinos could still be traced in the decays of the top squarks of the above-mentioned kind. We consider the signal final state at the LHC. We find that while a usual cut-based analysis (CBA) of LHC data worth 300 fb −1 would be unable to discover such excitations, a multivariate analysis (MVA) can be reasonably sensitive to higgsino-like ewinos having masses ≳ 650 GeV when m t ~ 1 $$ {m}_{{\tilde{t}}_1} $$ ≳ 1 TeV. On the other hand, with 3000 fb −1 of data, these masses become accessible in a CBA while even an MVA on such a data set is unlikely to find these ewinos with masses around 1 TeV when m t ~ 1 $$ {m}_{{\tilde{t}}_1} $$ hits ∼ 1.5 TeV.
نوع الوثيقة: article
وصف الملف: electronic resource
اللغة: English
تدمد: 1029-8479
Relation: https://doaj.org/toc/1029-8479
DOI: 10.1007/JHEP11(2023)081
URL الوصول: https://doaj.org/article/2c1d641a64724516a75d78e3f85f7b4a
رقم الأكسشن: edsdoj.2c1d641a64724516a75d78e3f85f7b4a
قاعدة البيانات: Directory of Open Access Journals
الوصف
تدمد:10298479
DOI:10.1007/JHEP11(2023)081