379 research outputs found
Implications of vacuum stability constraints on the nonminimal supersymmetric standard model with lepton number violation
We carry out a detailed analysis of the scalar sector of the nonminimal
supersymmetric standard model with lepton number violation, and study the
constraints imposed on it by the stability of the electroweak symmetry breaking
vacuum. The model contains a trilinear lepton mumber violating term in the
superpotential together with the associated \susy breaking interactions which
can give rise to neutrino masses. We evaluate the mass matrices for the various
boson and fermion modes and then discuss the effect that the lepton number
violating interactions have on the mass spectra using a phenomenological
precription to implement the experimental constraints on the light neutrinos
mass matrix. We also discuss qualitatively the conditions on the lepton number
violating parameters set by the unbounded from below directions, and from the
absence of the charge and color breaking minima in this model.Comment: 39 pages, 5 figures, Latex file, ps figure
Beam polarization effects in the radiative production of lightest neutralinos in collisions in supersymmetric grand unified models
We study the production of the lightest neutralinos in the process in supersymmetric grand unified models
for the International Linear Collider Energies with longitudinally polarized
beams. We consider cases where the standard model gauge group is unified into
the grand unified gauge groups SU(5), or SO(10). We have carried out a
comprehensive study of this process in the SU(5) and SO(10) grand unified
theories which includes the QED radiative corrections. We compare and contrast
the dependence of the signal cross section on the grand unified gauge group,
and on the different representations of the grand unified gauge group, when the
the electron and positron beams are longitudinally polarized. To assess the
feasibility of experimentally observing the radiative production process, we
have also considered in detail the background to this process coming from the
radiative neutrino production process
with longitudinally polarized electron and positron beams. In addition we have
also considered the supersymmetric background coming from the radiative
production of scalar neutrinos in the process with longitudinally polarized beams. The process can be a
major background to the radiative production of neutralinos when the scalar
neutrinos decay invisibly.Comment: 26 pages, 18 figures; typos and misprints corrected; results and
conclusions unchanged; this paper is a sequel to and draws material from the
paper arXiv:1210.647
Radiative neutralino production in low energy supersymmetric Models. II. The case of beam polarization
We study the production of the lightest neutralinos in the radiative process
in low energy supersymmetric
models for the International Linear Collider energies with longitudinally
polarized electron and positron beams. For this purpose we consider the case of
nonminimal supersymmetric standard model as well as the case of minimal
supersymmetric standard model. At the first stage of a linear collider, with
GeV, the radiative production of the lightest neutralinos may
be a viable channel to study supersymmetric partners of the Standard Model
particles, especially if the other supersymmetric particles are too heavy to to
be pair-produced. We consider in detail the effect of beam polarization on the
production cross section. We compare and contrast the dependence of the signal
cross section on the parameters of the neutralino sector of the nonminimal and
minimal supersymmetric standard model when the electron and positron beams are
longitudinally polarized. In order to assess the feasibility of experimentally
observing the radiative neutralino production process, we consider the
background to this process coming from the Standard Model process with longitudinally polarized electron and positron beams.
We also consider the supersymmetric background to the radiative neutralino
production process coming from the radiative production of the scalar partners
of the neutrinos (sneutrinos) ,
with longitudinally polarized beams. This process can be a a background to the
radiative neutralino production when the sneutrinos decay invisibly.Comment: 20 pages, 16 figures, 13 tables; latex problem fixe
Phenomenology of light Higgs bosons in supersymmetric left-right models
We carry out a detailed analysis of the light Higgs bosons in supersymmetric
left-right models (SLRM). This includes models with minimal particle content
and those with additional Higgs superfields. We also consider models with
non-renormalizable higher-dimensional terms. We obtain an upper bound on the
mass of the lightest CP-even neutral Higgs boson in these models. The upper
bound depends only on the gauge couplings, and the vacuum expectation values of
those neutral Higgs fields which control the spontaneous breakdown of the
gauge symmetry. We calculate the one-loop radiative
corrections to this upper bound, and evaluate it numerically in the minimal
version of the supersymmetric left-right model. We consider the couplings of
this lightest CP-even Higgs boson to the fermions, and show that in a
phenomenologically viable model the branching ratios are similar to the
corresponding branching ratios in the minimal supersymmetric standard model
(MSSM). We then study the most promising particle for distinguishing the SLRM
from other models, namely the doubly charged Higgs boson. We obtain the mass of
this doubly charged Higgs boson in different types of supersymmetric left-right
models, and discuss its phenomenology.Comment: 29 pages, 4 figure
Mass of the lightest Higgs Boson in Supersymmetric Left-Right Models
We consider the lightest Higgs boson in naturally R-parity conserving
supersymmetric left-right models. We obtain an upper bound on the tree level
mass of this lightest Higgs boson. This upper bound depends on the
and gauge couplings, and the vacuum expectation values of bidoublet
Higgs fields, which are needed to break . The upper bound
does not depend on either the breaking scale or the supersymmetry
breaking scale. We evaluate the bound numerically by assuming that the theory
remains perturbative upto some scale . We find that the bound can be
considerably larger than in MSSM. The dominant radiative corrections to the
upper bound due to top-stop and bottom-sbottom systems are of the same form as
in the minimal supersymmetric standard model.Comment: 14 pages including 2 figures, LaTe
- …