In view of the recent interest in the pMSSM with light third generation squarks, we consider a hitherto neglected scenario where the lighter bottom squark ((b) over tilde (1)) is the next lightest supersymmetric particle (NLSP) which co-annihilates with the lightest supersymmetric particle (LSP), the dark matter (DM) candidate. Since the co-annihilation cross section receives contributions from both electroweak and strong vertices, it is relatively large. As a result relatively large NLSP-LSP mass difference (25-35GeV) is consistent with the PLANCK data. This facilitates the LHC signatures of this scenario. We consider several variants of the sbottom NLSP scenario with and without light stops and delineate the parameter space allowed by the PLANCK data. We point out several novel signal (e.g., (t) over tilde (1) -> (b) over tilde W-1) which are not viable in the stop NLSP scenario of DM production. Finally, we consider gluino ((g) over tilde) decays in this scenario and using the current ATLAS data in the jets (with or without b-tagging) + is not an element of(T) channel, obtain new limits in the m((b) over tilde1) - m((g) over tilde) mass plane. We find that for m((b) over tilde1) upto 500GeV, m((g) over tilde) >= 1.1-1.2 TeV in this scenario.
机构:
Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
Chinese Acad Sci, Inst Theoret Phys, KITPC, Beijing 100190, Peoples R China
Univ Delaware, Dept Phys & Astron, Bartol Res Inst, Newark, DE 19716 USAChinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
Raza, Shabbar
Shafi, Qaisar
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Univ Delaware, Dept Phys & Astron, Bartol Res Inst, Newark, DE 19716 USAChinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
Shafi, Qaisar
Un, Cem Salih
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Univ Delaware, Dept Phys & Astron, Bartol Res Inst, Newark, DE 19716 USA
Uludag Univ, Dept Phys, TR-16059 Bursa, TurkeyChinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China