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Huang, FP; Yu, JH
Exploring inert dark matter blind spots with gravitational wave signatures
发表期刊PHYSICAL REVIEW D
语种英语
关键词FALSE VACUUM RADIATION
摘要Motivated by the absence of dark matter signals in direct detection experiments and the discovery of gravitational waves (GWs) at aLIGO, we discuss the possibility to explore a generic classes of scalar dark matter models using the complementary searches via phase transition GWs and the future lepton collider signatures. We focus on the inert scalar multiplet dark matter models and the mixed inert scalar dark matter models, which could undergo a strong first-order phase transition during the evolution of the early universe, and might produce detectable phase transition GW signals at future GW experiments, such as LISA, DECIGO and BBO. We find that the future GW signature, together with the collider signature at future lepton collider, could further explore the model's blind spot parameter region, at which the dark matter-Higgs coupling is identically zero, thus avoiding the dark matter spin-independent direct detection constraints.
2018
ISSN2470-0010
卷号98期号:9页码:95022
学科领域Astronomy & Astrophysics ; Physics
学科门类Astronomy & Astrophysics ; Physics, Particles & Fields
DOI10.1103/PhysRevD.98.095022
收录类别SCIE
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/22778
专题理论物理所科研产出_SCI论文
作者单位1.Chinese Acad Sci, Inst High Energy Phys, Theoret Phys Div, POB 918-4, Beijing 100049, Peoples R China
2.Univ Massachusetts, Dept Phys, Amherst Ctr Fundamental Interact, Amherst, MA 01002 USA
3.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
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Huang, FP,Yu, JH. Exploring inert dark matter blind spots with gravitational wave signatures[J]. PHYSICAL REVIEW D,2018,98(9):95022.
APA Huang, FP,&Yu, JH.(2018).Exploring inert dark matter blind spots with gravitational wave signatures.PHYSICAL REVIEW D,98(9),95022.
MLA Huang, FP,et al."Exploring inert dark matter blind spots with gravitational wave signatures".PHYSICAL REVIEW D 98.9(2018):95022.
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