2011/12/31 by Jonathan L. Feng, K. Matchev, Konstantin T. Matchev +1 · 135 citations
Physics and Astronomy · #Anomalous magnetic dipole moment #Chargino #Dark Matter and Cosmic Phenomena #Dark matter #Higgs boson #Minimal Supersymmetric Standard Model #Muon #Neutralino #Neutrino Physics Research #Parameter space #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Standard Model (mathematical formulation) #Statistics #Supergravity #Supersymmetry #hep-ex #hep-ph
paper · pdf · doi:10.1103/physrevd.85.075007
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 85(7) (American Physical Society) · v3: 20 pages, 20 figures, minor numerical error in relic density calculation corrected, fixed contours in figure 5
openalex publication_date 2012/04/05 · arxiv created 2012/08/21 · arxiv updated 2013/05/29 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Recent results from Higgs boson and supersymmetry searches at the Large Hadron Collider provide strong new motivations for supersymmetric theories with heavy superpartners. We reconsider focus point supersymmetry (FP SUSY), in which all squarks and sleptons may have multi-TeV masses without introducing fine-tuning in the weak scale with respect to variations in the fundamental SUSY-breaking parameters. We examine both FP SUSY and its familiar special case, the FP region of minimal supergravity, also known as the constrained minimal supersymmetric standard model (mSUGRA/CMSSM), and show that they are beautifully consistent with all particle, astroparticle, and cosmological data, including Higgs boson mass limits, null results from SUSY searches, electric dipole moments, b\ensuremath→s\ensuremathγ, Bs\ensuremath→\ensuremathμ+\ensuremathμ^\ensuremath-, the thermal relic density of neutralinos, and dark matter searches. The observed deviation of the muon's anomalous magnetic moment from its standard model value may also be explained in FP SUSY, although not in the FP region of mSUGRA/CMSSM. In light of recent data, we advocate refined searches for FP SUSY and related scenarios with heavy squarks and sleptons, and we present a simplified parameter space within mSUGRA/CMSSM to aid such analyses.