Beam polarization effects in the radiative production of lightest neutralinos in e+e- collisions in supersymmetric grand unified models

被引:5
|
作者
Pandita, P. N. [1 ]
Patra, Monalisa [2 ]
机构
[1] NE Hill Univ, Dept Phys, Shillong 793002, Meghalaya, India
[2] Indian Inst Sci, Ctr High Energy Phys, Bangalore 560012, Karnataka, India
来源
PHYSICAL REVIEW D | 2013年 / 88卷 / 05期
关键词
SINGLE-PHOTON; MISSING ENERGY; GAUGINO MASSES; PARTICLES; SEARCH; EVENTS; SUPERGRAVITY; ANNIHILATION; PHOTINOS; NEUTRINO;
D O I
10.1103/PhysRevD.88.055018
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the production of the lightest neutralinos in the process e(+)e(-) -> chi(0)(1)chi(0)(1)gamma 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 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 e(+)e(-)-> nu(nu) over bar gamma 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 e(+)e(-) -> (nu) over tilde(nu) over tilde*gamma with longitudinally polarized beams. The process can be a major background to the radiative production of neutralinos when the scalar neutrinos decay invisibly.
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页数:22
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