Gravitational waves from dark first order phase transitions and dark photons

被引：38

作者：

Addazi, Andrea ^{[1
]}

Marciano, Antonino

机构：

[1] Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China

来源：

CHINESE PHYSICS C | 2018年 / 42卷 / 02期

关键词：

dark matter; gravitational waves; colliders; VECTOR GAUGE BOSON; PHI-MESON DECAYS; SEARCH; RADIATION;

D O I：

10.1088/1674-1137/42/2/023107

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Cold Dark Matter particles may interact with ordinary particles through a dark photon, which acquires a mass thanks to a spontaneous symmetry breaking mechanism. We discuss a dark photon model in which the scalar singlet associated to the spontaneous symmetry breaking has an effective potential that induces a first order phase transition in the early Universe. Such a scenario provides a rich phenomenology for electron-positron colliders and gravitational waves interferometers, and may be tested in several different channels. The hidden first order phase transition implies the emission of gravitational waves signals, which may constrain the dark photon's space of parameters. Compared limits from electron-positron colliders, astrophysics, cosmology and future gravitational waves interferometers such as eLISA, U-DECIGO and BBO are discussed. This highly motivates a cross-checking strategy of data arising from experiments dedicated to gravitational waves, meson factories, the International Linear Collider (ILC), the Circular Electron Positron Collider (CEPC) and other underground direct detection experiments of cold dark matter candidates.

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