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Exploration of heavy Higgs bosons at a 100 TeV hadron collider within the semi-constrained next-to-minimal supersymmetric standard model
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作者 Kun Wang Pengfu Tian Jingya Zhu 《Chinese Physics C》 SCIE CAS CSCD 2024年第9期107-117,共11页
In this study,we explore the detectability of heavy Higgs bosons in the pp→bbH/A→bbtt channel at a100 TeV hadron collider within the semi-constrained next-to-minimal supersymmetric standard model.We calculate their ... In this study,we explore the detectability of heavy Higgs bosons in the pp→bbH/A→bbtt channel at a100 TeV hadron collider within the semi-constrained next-to-minimal supersymmetric standard model.We calculate their production cross sections and decay branching ratios and compare them with simulation results from literature.We focus on the heavy doublet-dominated CP-even Higgs H and CP-odd Higgs A,with mass limits set below 10TeV to ensure detectability.At a collider with an integrated luminosity of 3 ab^(-1),the potential for detecting heavy Higgs bosons varies significantly with their mass and tanβ.Heavy Higgs bosons with masses below 2 TeV are within the testable range,while those heavier than 7 TeV are below the exclusion and discovery thresholds,rendering them undetectable.For masses between 2 and 7 TeV,heavy Higgs bosons with tanβ smaller than 20 can be detected,whereas those with tanβ larger than 20 are beyond the current discovery or exclusion capabilities. 展开更多
关键词 next-to-minimal supersymmetric standard model heavy Higgs boson 100 tev hadron collider
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中日合作西藏ASγ实验首次发现100TeV以上能量宇宙γ射线辐射 被引量:2
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作者 高启 拉巴次仁 +1 位作者 单增罗布 刘茂元 《高原科学研究》 CSCD 2020年第2期109-117,共9页
2019年7月中日合作西藏ASγ实验宣布发现来自蟹状星云方向能量高于100TeV(100万亿电子伏特)的宇宙γ射线辐射,这是人类首次观测到能量大于100 TeV的宇宙γ射线辐射。文章首先回顾了西藏ASγ实验在甚高能及以上能区宇宙γ射线探测所做的... 2019年7月中日合作西藏ASγ实验宣布发现来自蟹状星云方向能量高于100TeV(100万亿电子伏特)的宇宙γ射线辐射,这是人类首次观测到能量大于100 TeV的宇宙γ射线辐射。文章首先回顾了西藏ASγ实验在甚高能及以上能区宇宙γ射线探测所做的长期努力,介绍了这一发现背后西藏ASγ实验地面阵列进行的重大升级改造和主要观测结果,并对100TeV以上能量宇宙γ射线辐射观测结果重要意义作了分析讨论。 展开更多
关键词 西藏ASγ实验 μ子探测器(MD) 超高能γ射线 100 tev 蟹状星云
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Study on the separation of 100 TeV γ-rays from cosmic rays for the Tibet ASγ experiment
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作者 冯朝阳 张毅 +7 位作者 刘成 樊超 李红超 王博 吴含荣 胡红波 卢红 谭有恒 《Chinese Physics C》 SCIE CAS CSCD 2011年第2期153-157,共5页
A γhadron separation analysis is described for the observed air shower events with primary energy above 100 TeV based on the Tibet ASγ detector configuration. The shower age and size parameters are fitted from the m... A γhadron separation analysis is described for the observed air shower events with primary energy above 100 TeV based on the Tibet ASγ detector configuration. The shower age and size parameters are fitted from the measured lateral density distribution and used as discrimination variables. According to the MC simulation while taking into account the systematic uncertainty estimated from data and MC comparison, it is found that 70% of the cosmic ray (CR) background can be rejected while more than 78% of the T-rays can be retained. Sensitivity for 100 TeV γ-rays observation can thus be improved by at least 40%. 展开更多
关键词 origin of cosmic rays 100 tev γ-rays emission Tibet AST experiment NKG-function
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