1993
DOI: 10.1103/physrevd.48.1277
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Dynamical supersymmetry breaking at low energies

Abstract: Conventional approaches to supersymmetric model building suffer from several naturalness problems: they do not explain the large hierarchy between the weak scale and the Planck mass, and they require fine tuning to avoid large flavor changing neutral currents and particle electric dipole moments. The existence of models with dynamical supersymmetry breaking, which can explain the hierarchy, has been known for some time, but efforts to build such models have suffered from unwanted axions and difficulties with a… Show more

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Cited by 865 publications
(1,383 citation statements)
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References 21 publications
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“…The scale factors are close to unity (0.89-1.06, with uncertainties between 0.03 and 0.06) in the lowest p T bin (20)(21)(22)(23)(24)(25)(26)(27)(28)(29)(30), and decrease to between 0.5 and 0.6 at high p T [Oð100 GeVÞ].…”
Section: Nðlþmentioning
confidence: 99%
See 1 more Smart Citation
“…The scale factors are close to unity (0.89-1.06, with uncertainties between 0.03 and 0.06) in the lowest p T bin (20)(21)(22)(23)(24)(25)(26)(27)(28)(29)(30), and decrease to between 0.5 and 0.6 at high p T [Oð100 GeVÞ].…”
Section: Nðlþmentioning
confidence: 99%
“…Results are interpreted in terms of modelindependent limits on the event yields from new physics processes leading to the given signature, as well as in a variety of specific SUSY scenarios. These scenarios include RPV and RPC simplified models, which describe the interactions of a minimal set of particles, as well as models with general gauge-mediated SUSY breaking (GGM) [18,19], which is a generalization of gauge-mediated SUSY breaking theories (GMSB) [20][21][22][23][24][25] where the parametrization does not depend on the details of the SUSY breaking mechanism. This analysis updates and extends results presented previously by ATLAS [26].…”
Section: Introductionmentioning
confidence: 99%
“…The canonical models were first put forth in the older works of [111,112,113,12] but interest was renewed in the scenario by models of Dine, Nelson and collaborators [114,115,116].…”
Section: Gauge Mediated Supersymmetry Breakingmentioning
confidence: 99%
“…Moreover, unless both N 1 and N 2 are even, the R symmetry becomes trivial. 5 Thus, we expec that gaugino masses are generated by radiative corrections [21,22,23] for the entire gauge group G except for the diagonal U (1), for which q 12 , q 21 are neutral.…”
Section: Gaugino Masses and The Low Energy Limitmentioning
confidence: 99%