Naturalness, Supersymmetry and Light Higgsinos: A Snowmass Whitepaper
arXiv:1306.2926
Abstract
We show that the electroweak fine-tuning parameter Δ_{\rm EW} derived from the well-known electroweak symmetry breaking condition written in terms of weak scale parameters leads to {\it a bound on fine-tuning in the MSSM} and explain its utility for phenomenological analyses. We argue that a small magnitude of the mu parameter, and the concomitant presence of light higgsinos, is the most basic consequence of naturalness in SUSY models, and list the resulting implications of this for experiments at the LHC and at future e^+e^- colliders.
3 page Snowmass whitepaper
Cited by in corpus (7)
- How conventional measures overestimate electroweak fine-tuning in supersymmetric theory
- Confronting Electroweak Fine-tuning with No-Scale Supergravity
- Post LHC8 SUSY benchmark points for ILC physics
- Snowmass whitepaper: Exploring natural SUSY via direct and indirect detection of higgsino-like WIMPs
- Leaving no stone unturned in the hunt for SUSY naturalness: A Snowmass whitepaper
- Identifying a Higgsino-like NLSP in the context of a keV-scale gravitino LSP
- The loop effects on the chargino decays in the MSSM