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20112026
most citedRadiative natural SUSY with a 125 GeV Higgs boson

304 citations · 1.9k across the 38 of their papers we have counts for

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hep-ph2012★ 220 cited

Radiative natural supersymmetry: Reconciling electroweak fine-tuning and the Higgs boson mass

Howard Baer, Vernon Barger, Peisi Huang +3

Models of natural supersymmetry seek to solve the little hierarchy problem by positing a spectrum of light higgsinos <~ 200-300 GeV and light top squarks <~ 600 GeV along with very…

hep-ph2012★ 115 cited

Post-LHC7 fine-tuning in the mSUGRA/CMSSM model with a 125 GeV Higgs boson

Howard Baer, Vernon Barger, Peisi Huang +3

The recent discovery of a 125 GeV Higgs-like resonance at LHC, coupled with the lack of evidence for weak scale supersymmetry (SUSY), have severely constrained SUSY models such as…

hep-ph2012★ 304 cited

Radiative natural SUSY with a 125 GeV Higgs boson

Howard Baer, Vernon Barger, Peisi Huang +2

It has been argued that requiring low electroweak fine-tuning (EWFT) along with a (partial) decoupling solution to the SUSY flavor and CP problems leads to a sparticle mass spectra…

hep-ph2012★ 17 cited

Flavor-Tuned 125 GeV SUSY Higgs Boson at the LHC: MSSM and NATURAL SUSY TESTS

Vernon Barger, Peisi Huang, Muneyuki Ishida +1

We show that an enhanced two-photon signal of the Higgs boson, h, observed with 125 GeV mass by the ATLAS and CMS collaborations, can be obtained if it is identified principally wi…

hep-ph2012★ 30 cited

Scalar-Top Masses from SUSY Loops with 125 GeV mh and precise Mw, mt

Vernon Barger, Peisi Huang, Muneyuki Ishida +1

We constrain the masses of scalar-tops (stop) by analyzing the new precision Tevatron measurement of the W-boson mass and the LHC/Tevatron indications of a Higgs boson of mass 125.…

hep-ph2012★ 133 cited

Natural Supersymmetry: LHC, dark matter and ILC searches

Howard Baer, Vernon Barger, Peisi Huang +1

Particle physics models with Natural Supersymmetry are characterized by a superpotential parameter μ\sim m_h \sim125$ GeV, while third generation squarks have mass <0.5-1.5 TeV. Gl…