Model Independent Approach to Focus Point Supersymmetry: from Dark Matter to Collider Searches

Details Model Independent Approach to Focus Point Supersymmetry: from Dark Matter to Collider Searches Model Independent Approach to Focus Point Supersymmetry: from Dark Matter to Collider Searches

2005-07-25

arxiv.org/abs/hep-ph/0507282v2

JHEP 0510 (2005) 020

Physics

High Energy Physics

High Energy Physics - Phenomenology

34 pages plus 36 eps figures

Scientific paper

10.1088/1126-6708/2005/10/020

The focus point region of supersymmetric models is compelling in that it simultaneously features low fine-tuning, provides a decoupling solution to the SUSY flavor and CP problems, suppresses proton decay rates and can accommodate the WMAP measured cold dark matter (DM) relic density through a mixed bino-higgsino dark matter particle. We present the focus point region in terms of a weak scale parameterization, which allows for a relatively model independent compilation of phenomenological constraints and prospects. We present direct and indirect neutralino dark matter detection rates for two different halo density profiles, and show that prospects for direct DM detection and indirect detection via neutrino telescopes such as IceCube and anti-deuteron searches by GAPS are especially promising. We also present LHC reach prospects via gluino and squark cascade decay searches, and also via clean trilepton signatures arising from chargino-neutralino production. Both methods provide a reach out to m_{\tg}\sim 1.7 TeV. At a TeV-scale linear e^+e^- collider (LC), the maximal reach is attained in the \tz_1\tz_2 or \tz_1\tz_3 channels. In the DM allowed region of parameter space, a \sqrt{s}=0.5 TeV LC has a reach which is comparable to that of the LHC. However, the reach of a 1 TeV LC extends out to m_{\tg}\sim 3.5 TeV.

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