Status of Natural Supersymmetry from the GmSUGRA in Light of the current LHC Run-2 and LUX data
Waqas Ahmed, Xiao-Jun Bi, Tianjun Li, Jia Shu Niu, Shabbar Raza,, Qian-Fei Xiang, Peng-Fei Yin

TL;DR
This study explores natural supersymmetry within GmSUGRA, demonstrating compatibility with current experimental constraints, identifying viable dark matter scenarios, and analyzing collider detection prospects with a focus on electroweak fine-tuning.
Contribution
It provides a detailed analysis of low fine-tuning supersymmetric models in GmSUGRA, identifying parameter space consistent with dark matter and collider constraints, and presents benchmark points for future searches.
Findings
Viable dark matter scenarios include Z-pole, Higgs-pole, and Higgsino LSP.
Current LHC data excludes certain Higgsino-dominant neutralino masses up to 460 GeV.
Electroweak fine-tuning around 20 remains compatible with experimental bounds.
Abstract
We study natural supersymmetry in the Generalized Minimal Supergravity (GmSUGRA). For the parameter space with low energy electroweak fine-tuning measures less than 50, we are left with only the -pole, Higgs-pole and Higgsino LSP scenarios for dark matter (DM). We perform the focused scans for such parameter space and find that it satisfies various phenomenological constraints and is compatible with the current direct detection bound on neutralino DM reported by the LUX experiment. Such parameter space also has solutions with correct DM relic density besides the solutions with DM relic density smaller or larger than 5 WMAP9 bounds. We present five benchmark points as examples. In these benchmark points, gluino and the first two generations of squarks are heavier than 2 TeV, stop are in the mass range TeV, while sleptons are lighter than 1 TeV. Some…
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