中文版 | English
ITP OpenIR  > 理论物理所SCI论文
Third generation in cascade decays
Dutta, B; Li, TJ; Maxin, JA; Nanopoulos, DV; Sinha, K; Walker, JW; Dutta, B (reprint author), Texas A&M Univ, George P & Cynthia W Mitchell Inst Fundamental Ph, College Stn, TX 77843 USA.
2015
发表期刊PHYSICAL REVIEW D
卷号91期号:11页码:115021
文章类型Article
摘要In supersymmetric models with gluinos m((g) over tilde) similar to 1000-2000 GeV, new physics searches based on cascade decay products of the gluino are viable at the next run of the LHC. We investigate a scenario where the light stop is lighter than the gluino and both are lighter than all other squarks, and show that its signal can be established using multi b-jet, multi W and/or multi-lepton final state topologies. We then utilize both boosted and conventional jet topologies in the final state in conjunction with di-tau production as a probe of the stau-neutralino coannihilation region responsible for the model's dark matter content. This study is performed in the specific context of one such phenomenologically viable model named no-scale F-SU(5).
学科领域Astronomy & Astrophysics ; Physics
资助者DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program
DOIhttp://dx.doi.org/10.1103/PhysRevD.91.115021
关键词[WOS]8 TEV ; SEARCHES ; SUSY ; LHC
收录类别SCI
语种英语
资助者DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; DOE [DE-FG02-13ER42020] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; NSF Award [PHY-1206044] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; Natural Science Foundation of China [10821504, 11075194, 11135003, 11275246, 11475238] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; National Basic Research Program of China (973 Program) [2010CB833000] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; NASA Astrophysics Theory Grant [NNH12ZDA001N] ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program ; Sam Houston State University Enhancement Research Grant program
WOS类目Astronomy & Astrophysics ; Physics, Particles & Fields
引用统计
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/20952
专题理论物理所SCI论文
通讯作者Dutta, B (reprint author), Texas A&M Univ, George P & Cynthia W Mitchell Inst Fundamental Ph, College Stn, TX 77843 USA.
推荐引用方式
GB/T 7714		 Dutta, B,Li, TJ,Maxin, JA,et al. Third generation in cascade decays[J]. PHYSICAL REVIEW D,2015,91(11):115021.
APA Dutta, B.,Li, TJ.,Maxin, JA.,Nanopoulos, DV.,Sinha, K.,...&Dutta, B .(2015).Third generation in cascade decays.PHYSICAL REVIEW D,91(11),115021.
MLA Dutta, B,et al."Third generation in cascade decays".PHYSICAL REVIEW D 91.11(2015):115021.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Third generation in （4557KB）期刊论文出版稿开放获取CC BY-NC-SA请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Dutta, B]的文章
[Li, TJ]的文章
[Maxin, JA]的文章
百度学术
百度学术中相似的文章
[Dutta, B]的文章
[Li, TJ]的文章
[Maxin, JA]的文章
必应学术
必应学术中相似的文章
[Dutta, B]的文章
[Li, TJ]的文章
[Maxin, JA]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。