Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments
Given the recent constraints from the dark matter (DM) direct detections, we examine a light GeV-scale (2–30 GeV) neutralino DM in the alignment limit of the Minimal Supersymmetric Standard Model (MSSM). In this limit without decoupling, the heavy CP-even scalar H plays the role of the Standard Mode...
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doaj-f9f3a51983334a138763820761d1346a2020-11-24T21:35:49ZengElsevierPhysics Letters B0370-26931873-24452018-03-01778C29630210.1016/j.physletb.2018.01.030Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experimentsGuang Hua Duan0Wenyu Wang1Lei Wu2Jin Min Yang3Jun Zhao4Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, Jiangsu 210023, ChinaInstitute of Theoretical Physics, College of Applied Science, Beijing University of Technology, Beijing 100124, ChinaDepartment of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, Jiangsu 210023, ChinaCAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, ChinaInstitute of Theoretical Physics, College of Applied Science, Beijing University of Technology, Beijing 100124, ChinaGiven the recent constraints from the dark matter (DM) direct detections, we examine a light GeV-scale (2–30 GeV) neutralino DM in the alignment limit of the Minimal Supersymmetric Standard Model (MSSM). In this limit without decoupling, the heavy CP-even scalar H plays the role of the Standard Model (SM) Higgs boson while the other scalar h can be rather light so that the DM can annihilate through the h resonance or into a pair of h to achieve the observed relic density. With the current collider and cosmological constraints, we find that such a light neutralino DM above 6 GeV can be excluded by the XENON-1T (2017) limits while the survivied parameter space below 6 GeV can be fully tested by the future germanium-based light dark matter detections (such as CDEX), by the Higgs coupling precison measurements or by the production process e+e−→hA at an electron–positron collider (Higgs factory).http://www.sciencedirect.com/science/article/pii/S0370269318300388 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Guang Hua Duan Wenyu Wang Lei Wu Jin Min Yang Jun Zhao |
spellingShingle |
Guang Hua Duan Wenyu Wang Lei Wu Jin Min Yang Jun Zhao Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments Physics Letters B |
author_facet |
Guang Hua Duan Wenyu Wang Lei Wu Jin Min Yang Jun Zhao |
author_sort |
Guang Hua Duan |
title |
Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments |
title_short |
Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments |
title_full |
Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments |
title_fullStr |
Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments |
title_full_unstemmed |
Probing GeV-scale MSSM neutralino dark matter in collider and direct detection experiments |
title_sort |
probing gev-scale mssm neutralino dark matter in collider and direct detection experiments |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 1873-2445 |
publishDate |
2018-03-01 |
description |
Given the recent constraints from the dark matter (DM) direct detections, we examine a light GeV-scale (2–30 GeV) neutralino DM in the alignment limit of the Minimal Supersymmetric Standard Model (MSSM). In this limit without decoupling, the heavy CP-even scalar H plays the role of the Standard Model (SM) Higgs boson while the other scalar h can be rather light so that the DM can annihilate through the h resonance or into a pair of h to achieve the observed relic density. With the current collider and cosmological constraints, we find that such a light neutralino DM above 6 GeV can be excluded by the XENON-1T (2017) limits while the survivied parameter space below 6 GeV can be fully tested by the future germanium-based light dark matter detections (such as CDEX), by the Higgs coupling precison measurements or by the production process e+e−→hA at an electron–positron collider (Higgs factory). |
url |
http://www.sciencedirect.com/science/article/pii/S0370269318300388 |
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