Type-I two-Higgs-doublet model and gravitational waves from domain walls bounded by strings

被引：4

作者：

Fu, Bowen ^{[1
]}

Ghoshal, Anish ^{[2
]}

King, Stephen F. ^{[3
]}

Rahat, Moinul Hossain ^{[4
,5
]}

机构：

[1] Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 200240, Peoples R China

[2] Univ Warsaw, Inst Theoret Phys, Fac Phys, Ul Pasteura 5, PL-02093 Warsaw, Poland

[3] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, England

[4] Univ Valencia, Inst Fis Corpuscular, Edificio Inst Invest,C Catedrat Jose Beltran 2, Paterna 46980, Spain

[5] CSIC, Edificio Inst Invest,C Catedrat Jose Beltran 2, Paterna 46980, Spain

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2024年 / 08期

基金：

英国科学技术设施理事会; 欧盟地平线“2020”;

关键词：

Cosmology of Theories BSM; Early Universe Particle Physics; Multi-Higgs Models; Phase Transitions in the Early Universe; RADIATION;

D O I：

10.1007/JHEP08(2024)237

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The spontaneous breaking of a U(1) symmetry via an intermediate discrete symmetry may yield a hybrid topological defect of domain walls bounded by cosmic strings. The decay of this defect network leads to a unique gravitational wave signal spanning many orders in observable frequencies, that can be distinguished from signals generated by other sources. We investigate the production of gravitational waves from this mechanism in the context of the type-I two-Higgs-doublet model extended by a U(1)R symmetry, that simultaneously accommodates the seesaw mechanism, anomaly cancellation, and eliminates flavour-changing neutral currents. The gravitational wave spectrum produced by the string-bounded-wall network can be detected for U(1)R breaking scale from 1012 to 1015 GeV in forthcoming interferometers including LISA and Einstein Telescope, with a distinctive f3 slope and inflexion in the frequency range between microhertz and hertz.

引用

页数：25

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