三轻子末态和缺少横向动量的大型强子对撞机中Higgsinos和Gauginos等电荷-中微子对产生的研究

Nada Ezzelarab, Ahmed Ali Abdelalim, M. Sirag
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引用次数: 0

摘要

研究了√s = 14 TeV的大型强子对撞机中电荷-中性子对产生的计算。在质量参数的四种条件下,对MSSM生产电荷-中性子对的不同基准点进行了评估。结果与LHC在√(s) = 8,13,14 TeV下记录的最新pp碰撞数据进行了比较。在SM的最小超对称扩展(MSSM)中,用M1、M2和μ表示的二能级、二能级和高能级的质量参数。我们的结果取决于电荷-中性子对产生的性质及其质量。对于轻的高介子,如slepton,总横截面在小x处产生,而对于高介子,如s-夸克,由于受CMS和ATLAS约束的高介子比1 TeV重,在大x处产生。假设最轻的超对称粒子(LSP) x ^ 1^0是稳定的,具有r宇称守恒,它是一个可行的暗物质候选者。在这个搜索中考虑了电荷-中性子对产生的两种情况。第一种情况下,高基诺具有两种条件,分别是wino-bino和higgsino质量参数[(M1 < M2 < μ)和(M1 < M2 <−μ)]。第二种情况是Higgsino,在wino-bino和Higgsino质量参数[(M1 <−μ < M2)和(−μ < M1 < M2)]两个条件下。此外,还讨论了μ的符号和值对高、高能粒子总截面的影响。Nada Ezzelarab等人。j .科学。研究科学。浙江农业学报,2022,39 (1):31-46
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Study of Chargino-Nutralino Pair Production like Higgsinos and Gauginos at The LHC with Three Leptons Final State and Missing Transverse Momentum
The calculation of chargino-nutralino pair production at the LHC with √s = 14 TeV had been studied. Different benchmark points are evaluated for the chargino-nutralino pair production using MSSM for four conditions on mass parameters. The results were compared with the latest data recorded by the LHC at √(s) = 8, 13, 14 TeV for pp collisions. In the minimal supersymmetric extension of the SM (MSSM) the mass parameters for the bino, wino, and higgsino states represented by M1, M2, and μ. Our results depend on the nature of the chargino-nutralino pair production and its masses. In case of light higgsino like sleptons the total cross section produced at small x, while for gauginos like s-quarks produced at large x due to the fact that gaugino constrained by CMS and ATLAS as heavier than 1 TeV. Assuming that the lightest supersymmetric particle (LSP) x ̃_1^0 is stable with R-parity conservation, it is a well-motivated to viable dark-matter candidate. Two scenarios of chargino-nutralino pair production are considered in this search. The first scenario Gaugino like with two conditions on the wino-bino and higgsino mass parameters [(M1 < M2 < μ) and (M1 < M2 < −μ)]. The second scenario Higgsino like with two conditions on the wino-bino and higgsino mass parameters [(M1 < −μ < M2) and (−μ < M1 < M2)]. Also, the effect of the sign and value of μ on the total cross sections for higgsinos and gauginos was represented. Nada Ezzelarab et al. J. Sci. Res. Sci., 2022, 39, (1): 31-46
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