Right-handed sneutrino dark matter in supersymmetric \(B - L\) model

DOI10.1007/JHEP07(2011)026zbMath1298.81420arXiv1102.4249OpenAlexW3105773247MaRDI QIDQ467327

Shaaban Khalil, Takashi Toma, Hiroshi Okada

Publication date: 3 November 2014

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1102.4249

zbMATH Keywords

supersymmetry phenomenology

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Supersymmetric field theories in quantum mechanics (81T60) Weak interaction in quantum theory (81V15)

Related Items (3)

A supersymmetric electroweak scale seesaw model ⋮ Right-handed sneutrino dark matter in \(\mathrm{U}(1)'\) seesaw models and its signatures at the LHC ⋮ Dark Matter inB–Lsupersymmetric Standard Model with inverse seesaw

Uses Software

• DarkSUSY

Cites Work

• Beyond the MSSM Higgs with \(d=6\) effective operators
• Heavy lepton pair production at LHC: model discrimination with multi-lepton signals
• Neutrino masses, dark matter and B-L symmetry at the LHC
• Electron EDM and soft leptogenesis in supersymmetric B-L extension of the Standard Model
• TeV scale see-saw mechanisms of neutrino mass generation, the Majorana nature of the heavy singlet neutrinos and \((\beta \beta)_{\text{0}\nu}\)-decay
• A gamma-ray determination of the Universe’s star formation history

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