1. Introduction
The Supersymmetry Standard Model (SUSY) [1–7], suggests adding a new symmetry to particle physics'
Standard Model (SM), as well as a symmetry between bosons and fermions, and anticipates the presence of
potential partners for each Standard Model (SM) particle. This provides resolve for the hierarchy dilemma
[7-12] and a nominee for dark matter in the form of the lightest supersymmetric particle (LSP), which will
be static in the situation of conserved R-parity [13].
The SM's minimal supersymmetric extension (MSSM) [14, 15], The bino, the winos, and the Higgsino are
the superpartners of the U(1)Y and SU(2)L gauge fields, as well as the Higgs field. The mass terms for the
bino, wino, and Higgsino states are M1,M2, and, μ respectively. Since they not carry color charge, they can
only be produced through electroweak interactions or the decay of colored superpartners. Because
electroweak processes have smaller cross sections, the masses of these objects are observationally less limited
than the masses of colored SUSY particles. According to the mass spectrum. Through mixing of the
superpartners, chargino (
) and neutralino (
) mass eigenstates are created. These are known as
electroweakinos, and the subscripts imply increasing electroweakino mass. If the
is stable, for
example as the lightest supersymmetric particle (LSP) and R-parity conservation is postulated, it is a viable
dark-matter candidate [16, 17].
This paper calculates the cross sections (σ) as a function of center of mass energy a search for direct
production of neutral Higgs boson and two charged charginos from electron-positron annihilation via
different propagators for the process
1.1 The Cross-section Scattering
In physics, the significance of cross section is an indicator of the probability that a particular process will
occur when a particular type of radiant excitation encounters a highly concentrated phenomenon. The
Rutherford cross-section, for example, is an indicator of the chance of an alpha particle being diverted by a
specific direction throughout an interaction with an atomic nucleus. σ (sigma) cross section and is measured
in term of area, specifically barns. In some ways, it can be compared to the size of the object that the excitation
must strike throughout order for the process to take place.
We have learned a lot about nuclear and atomic physics through scattering experiments, such as the discovery
of subatomic particles (such as quarks). Scattering phenomena, such as neutron, electron, and x-ray scattering,
are used to investigate solid state systems in low energy physics. As a main overview, it is therefore essential
in any advanced quantum mechanics course.
If the radiation is thought to be made up of quanta, The quantity of incident particles hitting the target's
surface per unit time per unit area is the flux, and the cross-section measures the scattering rate per unit
incident radiation flux. Calculating scattering cross-sections for long-wavelength electromagnetic radiation
means dividing the power of the scattered wave by the intensity of the incident wave. A cross-section
represents an area in dimensions, with its unit is barn, which has an area of 10−28 m2. Instead of a true