Electroweak phase transition confronted with dark matter detection constraints

被引：7
作者：
Chiang, Cheng-Wei [1 ]
Huang, Da [2 ]
Lu, Bo-Qiang [1 ]
机构：
[1] Natl Taiwan Univ, Dept Phys, Taipei 10617, Taiwan
[2] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
来源：
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2021年 / 01期
基金：
美国国家科学基金会;
关键词：
dark matter theory; cosmological phase transitions; dark matter experiments; GRAVITATIONAL-WAVES; PHYSICS; NUMBER; LIMITS; MODEL;
D O I：
10.1088/1475-7516/2021/01/035
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study the type-II first-order electroweak phase transition and dark matter (DM) phenomenology in both real and complex singlet extensions of SM. In the real singlet extension with a Z(2) symmetry, we show that the parameter regions favored by the phase transition suffer from strong constraints from DM direct detection so that only a negligible fraction (fx similar to 10(-4) - 10(-5)) of DM composed of the real singlet scalar can survive the LUX and XENON1T constraints. In the complex singlet S case, we impose a CP symmetry S -> S* to the scalar potential. The real component of S can mix with SM Higgs boson while the imaginary component becomes a DM candidate due to the protection of the CP symmetry. By taking into account the current experimental constraints of invisible Higgs decays, Higgs signal strength measurements, and dark matter detections, we find that there exists a large parameter space for the type-II electroweak phase transition to occur while explaining all of the dark matter relic density. We identify a subset of parameter space that is promising for future experiments, including the di-Higgs and Higgs signal strength measurements at the HL-LHC and the dark matter direct detection in the XENONnT project.
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页数：28
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