|
|
|
|||
| Journals Home | Journals List | EJs Extra | This Journal | Search | Authors | Referees | Librarians | User Options | Help | | ||||
JHEP10(2008)079 doi: 10.1088/1126-6708/2008/10/079
![]()
This is an Open Access article.
|
||||
Abstract.
The requirement of t−b−τ Yukawa coupling unification
is common in simple grand unified models based on the gauge group
SO(10), and it also places a severe constraint on the expected
spectrum of superpartners.
For Yukawa-unified models with μ>0, the spectrum is characterized by
three mass scales:
i) first and second generation scalars in the multi-TeV range,
ii) third generation scalars, μ and mA in the few-TeV range and
iii) gluinos in the ~ 350−500 GeV range with
chargino masses around 100-160 GeV.
In such a scenario, gluino pair production should occur at large rates at the CERN LHC,
followed by gluino three-body decays into neutralinos or charginos.
Discovery of Yukawa-unified SUSY at the LHC
should hence be possible with only 1 fb−1 of integrated
luminosity, by tagging multi-jet events with 2-3 isolated leptons,
without relying on missing ET.
A characteristic dilepton mass edge should easily be apparent above
Standard Model background. Combining dileptons with b-jets, along with
the gluino pair production cross section information, should allow
for gluino and neutralino mass reconstruction. A secondary corroborative
signal should be visible at higher integrated luminosity in the
±1
02 → 3
channel, and should exhibit the same
dilepton mass edge as in the gluino cascade decay signal.
Key words: Supersymmetry Phenomenology
E-print number: 0809.0710
Cited: by
Refers: to
| Post to CiteUlike | | Post to Connotea | | Post to Bibsonomy |
|
Journals Home | Journals List | EJs Extra | This Journal | Search | Authors | Referees | Librarians | User Options | Help | Recommend this journal EndNote, ProCite ® and Reference Manager ® are registered trademarks of ISI Researchsoft. Copyright © Institute of Physics and IOP Publishing Limited 2009 - electronic design and EJs software. © SISSA - the name "Journal of High Energy Physics" (JHEP), all content and the submissions and administrative software / processes. Use of this service is subject to compliance with the terms and conditions of use. In particular, reselling and systematic downloading of files is prohibited. |
|
| |