4.5 Article

LHC Dark Matter Working Group: Next-generation spin-0 dark matter models

期刊

PHYSICS OF THE DARK UNIVERSE
卷 27, 期 -, 页码 -

出版社

ELSEVIER
DOI: 10.1016/j.dark.2019.100351

关键词

-

资金

  1. JSPS KAKENHI [16K17715]
  2. United States-Israel Binational Science Foundation, Jerusalem, Israel
  3. Israel Science Foundation
  4. German Federal Ministry of Education and Research [05H15PACC1]
  5. Helmholtz Foundation
  6. U.S. DOE [DE-SC0011726]
  7. European Research Council under the European Union's Horizon 2020 research and innovation program [679305]
  8. Swedish Research Council
  9. NSF CAREER grant [PHY-1654502]
  10. NSF [PHY11-25915, PHY-1316792]
  11. Aspen Center for Physics
  12. National Science Foundation [PHY-1066293]
  13. CERN Theoretical Physics Department
  14. Ministry of Education, Science, Sports, and Culture (MEXT), Japan [16H06492]
  15. World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
  16. European Research Council under the European Union's Horizon 2020 program [648680]
  17. Programa Atraccion de Talento de la Comunidad de Madrid [2017-T1/TIC-5202]
  18. STFC [ST/M005437/1]
  19. National Science Centre, Poland
  20. HARMONIA project [UMO-2015/18/M/ST2/00518]
  21. National Research, Development and Innovation Fund in Hungary [K 25105]
  22. STFC [ST/M005437/1, ST/P001246/1] Funding Source: UKRI
  23. European Research Council (ERC) [679305] Funding Source: European Research Council (ERC)

向作者/读者索取更多资源

Dark matter (DM) simplified models are by now commonly used by the ATLAS and CMS Collaborations to interpret searches for missing transverse energy (E-T(miss)). The coherent use of these models sharpened the LHC DM search program, especially in the presentation of its results and their comparison to DM direct-detection (DD) and indirect-detection (ID) experiments. However, the community has been aware of the limitations of the DM simplified models, in particular the lack of theoretical consistency of some of them and their restricted phenomenology leading to the relevance of only a small subset of E-T(miss) signatures. This document from the LHC Dark Matter Working Group identifies an example of a next-generation DM model, called 2HDM+a, that provides the simplest theoretically consistent extension of the DM pseudoscalar simplified model. A comprehensive study of the phenomenology of the 2HDM+a model is presented, including a discussion of the rich and intricate pattern of mono-X signatures and the relevance of other DM as well as non-DM experiments. Based on our discussions, a set of recommended scans are proposed to explore the parameter space of the 2HDM+a model through LHC searches. The exclusion limits obtained from the proposed scans can be consistently compared to the constraints on the 2HDM+a model that derive from DD, ID and the DM relic density. (C) 2019 The Authors. Published by Elsevier B.V.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.5
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据