Stringent limits are set on the long-lived lepton-like sector of the phenomenological minimal supersymmetric standard model (pMSSM) and the anomaly-mediated supersymmetry breaking (AMSB) model. The limits are derived from the results presented in a recent search for long-lived charged particles in protonâproton collisions, based on data collected by the CMS detector at a centre-of-mass energy of 8Â TeV at the Large Hadron Collider. In the pMSSM parameter sub-space considered, 95.9Â % of the points predicting charginos with a lifetime of at least 10Â ns are excluded. These constraints on the pMSSM are the first obtained at the LHC. Charginos with a lifetime greater than 100Â ns and masses up to about 800Â GeV in the AMSB model are also excluded. The method described can also be used to set constraints on other models.
Constraints on the pMSSM, AMSB model and on other models from the search for long-lived charged particles in protonâproton collisions at âs = 8 TeV
ALBERGO, Sebastiano Francesco;CAPPELLO, GIGI;COSTA, Salvatore;GIORDANO, FERDINANDO;POTENZA, Renato Carlo;TRICOMI, Alessia Rita;TUVE', Cristina Natalina;
2015-01-01
Abstract
Stringent limits are set on the long-lived lepton-like sector of the phenomenological minimal supersymmetric standard model (pMSSM) and the anomaly-mediated supersymmetry breaking (AMSB) model. The limits are derived from the results presented in a recent search for long-lived charged particles in protonâproton collisions, based on data collected by the CMS detector at a centre-of-mass energy of 8Â TeV at the Large Hadron Collider. In the pMSSM parameter sub-space considered, 95.9Â % of the points predicting charginos with a lifetime of at least 10Â ns are excluded. These constraints on the pMSSM are the first obtained at the LHC. Charginos with a lifetime greater than 100Â ns and masses up to about 800Â GeV in the AMSB model are also excluded. The method described can also be used to set constraints on other models.File | Dimensione | Formato | |
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Constraints on the pMSSM, AMSB model and on other models.pdf
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