Event Details

The natural SUSY scenario requires light third generations while a 125 GeV higgs prefers heavy third generations. Dr. Huang will discuss a SUSY scenario, “Radiative Natural SUSY”, in which the contribution to fine-tuning from the Hu is driven radiatively to be small. This scenario features low electroweak fine-tuning, a 125 higgs and particles beyond the LHC limits. Then Dr. Huang will comment on the higgs couplings to SM particles in MSSM. In the end, Dr. Huang will discuss the LHC phenomenology of the Radiative Natural SUSY scenario.

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