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Implications of the Higgs discovery for the MSSM. [PDF]
Eur Phys J C Part Fields, 2014 Djouadi A.
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Search for chargino-neutralino production in p anti-p collisions at s**(1/2) = 1.96-TeV
, 2007 Not Available
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Two-body decays of neutralinos and charginos
Physical Review D, 1988We give explicit formulas for the two-body decays of the neutralinos and charginos of the minimal model of supersymmetry. There are two possible classes of two-body final states: (i) neutralino or chargino plus a W, Z, or Higgs boson; and (ii) channels involving squarks or sleptons.
, Gunion, , Haber
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Measuring the chargino parameters
Pramana, 2000After the supersymmetric particles have been discovered, the priority will be to determine independently the fundamental parameters to reveal the structure of the underlying supersymmetric theory. In my talk I discuss how the chargino sector can be reconstructed completely by measuring the cross-sections with polarized beams at e + e − collider ...
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Stop-Chargino Production at LHC
2008If Supersymmetry (SUSY) is a symmetry of nature, and the SUSY scale is around the 1TeV, the Large Hadron Collider is expected to be able to produce at least some of the new particles predicted by the supersymmetric models.
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2019
The lighter chargino (chi1) is a prime candidate to be thenext-to-lightest SUSY particle (the NLSP). Several analyses have beendone of chi1 pair-production at the ILC, at specific model-points,showing that detection and property-determination is possible, even forvery difficult cases.
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The lighter chargino (chi1) is a prime candidate to be thenext-to-lightest SUSY particle (the NLSP). Several analyses have beendone of chi1 pair-production at the ILC, at specific model-points,showing that detection and property-determination is possible, even forvery difficult cases.
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2019
The lighter chargino (chi1) is a prime candidate to be thenext-to-lightest SUSY particle (the NLSP). Several analyses have beendone of chi1 pair-production at the ILC, at specific model-points,showing that detection and property-determination is possible, even forvery difficult cases.
openaire +1 more source
The lighter chargino (chi1) is a prime candidate to be thenext-to-lightest SUSY particle (the NLSP). Several analyses have beendone of chi1 pair-production at the ILC, at specific model-points,showing that detection and property-determination is possible, even forvery difficult cases.
openaire +1 more source