AbstractGiving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatron data still allow the lightest supersymmetric Higgs to have a large branching fraction into invisible neutralinos. Such a Higgs may be difficult to discover at the LHC and is practically unreachable at the Tevatron. We argue that, for some of these models to be compatible with the relic density, light sleptons with masses not far above the current limits are needed. There are, however, models that allow for larger sleptons masses without being in conflict with the relic density constraint. This is possible because these neutralinos can annihilate efficiently through a Z pole. We also find that many of these models can nicely account...
In supersymmetric models where the magnitude of the GUT scale gaugino mass parameter M3 is suppresse...
Motivated by recent data from CoGeNT and the DAMA annual modulation signal, we discuss collider cons...
In natural supersymmetry models, Higgsinos are always light because μ2 cannot be much larger than [?...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
AbstractGiving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP an...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
In view of the latest LEP data we consider the effects of charginos and neutralinos on the two-photo...
We discuss effects of the light sparticles on decays of the lightest Higgs in a supersymmetric model...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In supersymmetric models where the magnitude of the GUT scale gaugino mass parameter M3 is suppresse...
Motivated by recent data from CoGeNT and the DAMA annual modulation signal, we discuss collider cons...
In natural supersymmetry models, Higgsinos are always light because μ2 cannot be much larger than [?...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
AbstractGiving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP an...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatr...
In view of the latest LEP data we consider the effects of charginos and neutralinos on the two-photo...
We discuss effects of the light sparticles on decays of the lightest Higgs in a supersymmetric model...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In view of the latest LEP data we consider the effects of charginos andneutralinos on the two-photon...
In supersymmetric models where the magnitude of the GUT scale gaugino mass parameter M3 is suppresse...
Motivated by recent data from CoGeNT and the DAMA annual modulation signal, we discuss collider cons...
In natural supersymmetry models, Higgsinos are always light because μ2 cannot be much larger than [?...