Primordial black holes from first-order phase transition in the singlet-extended SM

被引：4

作者：

Goncalves, Dorival ^{[1
]}

Kaladharan, Ajay ^{[1
]}

Wu, Yongcheng ^{[2
,3
]}

机构：

[1] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA

[2] Nanjing Normal Univ, Dept Phys, Nanjing 210023, Peoples R China

[3] Nanjing Normal Univ, Inst Theoret Phys, Nanjing 210023, Peoples R China

来源：

PHYSICAL REVIEW D | 2025年 / 111卷 / 03期

基金：

中国国家自然科学基金; 美国国家科学基金会;

关键词：

GRAVITATIONAL-RADIATION; FALSE VACUUM; HIGGS-BOSON; BUBBLE NUCLEATION; SEARCH; LIMITS; MASS; RESONANCES; COLLISIONS; FATE;

D O I：

10.1103/PhysRevD.111.035009

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Supercooled first-order phase transition (FOPT) can lead to the formation of primordial black holes (PBHs). This scenario imposes stringent requirements on the profile of the effective potential. In this work, we use the singlet extended Standard Model (xSM) as a benchmark model to investigate this possibility at the electroweak scale. The PBHs formed during a supercooled FOPT have a narrow mass distribution around the mass of Earth. This distribution is closely tied to the temperature at which the PBHs form, corresponding to the FOPT at the electroweak scale. This scenario can be probed with microlensing experiments, space-based gravitational wave detectors, and collider experiments. Remarkably, the future space-based gravitational wave detector LISA will hold the potential to either confirm this scenario that leads to PBH formation across the observable Universe in the xSM or completely rule it out. Interestingly, our findings suggest that PBHs within the xSM framework may align with observations of the six ultrashort timescale events reported by the OGLE microlensing experiment.

引用

页数：22

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