A brief review is given of the implications of a 126 GeV Higgs boson for the
discovery of supersymmetry. Thus a 126 GeV Higgs boson is problematic within
the Standard Model because of vacuum instability pointing to new physics beyond
the Standard Model. The problem of vacuum stability is overcome in the SUGRA
GUT model but the 126 GeV Higgs mass implies that the average SUSY scale lies
in the several TeV region. The largeness of the SUSY scale relieves the tension
on SUGRA models since it helps suppress flavor changing neutral currents and CP
violating effects and also helps in extending the proton life time arising from
baryon and lepton number violating dimension five operators. The geometry of
radiative breaking of the electroweak symmetry and fine tuning in view of the
large SUSY scale are analyzed.Consistency with the Brookhaven \$g\_\mu-2\$
result is discussed. It is also shown that a large SUSY scale implied by the
126 GeV Higgs boson mass allows for light gauginos (gluino, charginos,
neutralinos) and sleptons. These along with the lighter third generation
squarks are the prime candidates for discovery at RUN II of the LHC.
Implication of the 126 GeV Higgs boson for the direct search for dark matter is
discussed. Also discussed are the sparticles mass hierarchies and their
relationship with the simplified models under the Higgs boson mass constraint.
%0 Generic
%1 Nath2015Supersymmetry
%A Nath, Pran
%D 2015
%K shortreview, susy
%T Supersymmetry after the Higgs
%U http://arxiv.org/abs/1501.01679
%X A brief review is given of the implications of a 126 GeV Higgs boson for the
discovery of supersymmetry. Thus a 126 GeV Higgs boson is problematic within
the Standard Model because of vacuum instability pointing to new physics beyond
the Standard Model. The problem of vacuum stability is overcome in the SUGRA
GUT model but the 126 GeV Higgs mass implies that the average SUSY scale lies
in the several TeV region. The largeness of the SUSY scale relieves the tension
on SUGRA models since it helps suppress flavor changing neutral currents and CP
violating effects and also helps in extending the proton life time arising from
baryon and lepton number violating dimension five operators. The geometry of
radiative breaking of the electroweak symmetry and fine tuning in view of the
large SUSY scale are analyzed.Consistency with the Brookhaven \$g\_\mu-2\$
result is discussed. It is also shown that a large SUSY scale implied by the
126 GeV Higgs boson mass allows for light gauginos (gluino, charginos,
neutralinos) and sleptons. These along with the lighter third generation
squarks are the prime candidates for discovery at RUN II of the LHC.
Implication of the 126 GeV Higgs boson for the direct search for dark matter is
discussed. Also discussed are the sparticles mass hierarchies and their
relationship with the simplified models under the Higgs boson mass constraint.
@misc{Nath2015Supersymmetry,
abstract = {A brief review is given of the implications of a 126 GeV Higgs boson for the
discovery of supersymmetry. Thus a 126 GeV Higgs boson is problematic within
the Standard Model because of vacuum instability pointing to new physics beyond
the Standard Model. The problem of vacuum stability is overcome in the SUGRA
GUT model but the 126 GeV Higgs mass implies that the average SUSY scale lies
in the several TeV region. The largeness of the SUSY scale relieves the tension
on SUGRA models since it helps suppress flavor changing neutral currents and CP
violating effects and also helps in extending the proton life time arising from
baryon and lepton number violating dimension five operators. The geometry of
radiative breaking of the electroweak symmetry and fine tuning in view of the
large SUSY scale are analyzed.Consistency with the Brookhaven \$g\_{\mu}-2\$
result is discussed. It is also shown that a large SUSY scale implied by the
126 GeV Higgs boson mass allows for light gauginos (gluino, charginos,
neutralinos) and sleptons. These along with the lighter third generation
squarks are the prime candidates for discovery at RUN II of the LHC.
Implication of the 126 GeV Higgs boson for the direct search for dark matter is
discussed. Also discussed are the sparticles mass hierarchies and their
relationship with the simplified models under the Higgs boson mass constraint.},
added-at = {2019-02-23T22:09:48.000+0100},
archiveprefix = {arXiv},
author = {Nath, Pran},
biburl = {https://www.bibsonomy.org/bibtex/264bf391cb6397985a5c813ec9d98aca3/cmcneile},
citeulike-article-id = {13478723},
citeulike-linkout-0 = {http://arxiv.org/abs/1501.01679},
citeulike-linkout-1 = {http://arxiv.org/pdf/1501.01679},
day = 7,
eprint = {1501.01679},
interhash = {df377827261940081f3b13d9cc701a8c},
intrahash = {64bf391cb6397985a5c813ec9d98aca3},
keywords = {shortreview, susy},
month = jan,
posted-at = {2015-01-09 12:15:55},
priority = {2},
timestamp = {2019-02-23T22:15:27.000+0100},
title = {{Supersymmetry after the Higgs}},
url = {http://arxiv.org/abs/1501.01679},
year = 2015
}