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Model independent approach to focus point supersymmetry: from dark matter to collider searches

Baer H
•
Krupovnickas T
•
Profumo S
•
Ullio, Piero
2005
  • journal article

Periodico
JOURNAL OF HIGH ENERGY PHYSICS
Abstract
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(g) similar to 1.7TeV. At a TeV-scale linear e(+)e(-) collider (LC), the maximal reach is attained in the Z(1)Z(2) or Z(1)Z(3) channels. In the DM allowed region of parameter space, a root s = 0.5TeV LC has a reach which is comparable to that of the LHC. However, the reach of a 1TeV LC extends out to m(g) similar to 3.5TeV.
DOI
10.1088/1126-6708/2005/10/020
WOS
WOS:000232976700020
Archivio
http://hdl.handle.net/20.500.11767/12639
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-27544455844
https://doi.org/10.1088/1126-6708/2005/10/020
Diritti
open access
Soggetti
  • dark matter and doubl...

  • Hadron-Hadron scatter...

  • supersymmetry phenome...

  • Settore FIS/02 - Fisi...

Scopus© citazioni
62
Data di acquisizione
Jun 14, 2022
Vedi dettagli
Web of Science© citazioni
91
Data di acquisizione
Mar 17, 2024
Visualizzazioni
2
Data di acquisizione
Apr 19, 2024
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