arXiv · 2204.00799
Gravitational-Wave Signatures of Chiral-Symmetric Technicolor
Abstract
A chiral-symmetric technicolor model successfully reconciles the tension between electroweak precision tests and traditional technicolor models. Focusing on its simplest realization preserving the conventional Higgs mechanism, we study its primordial gravitational wave signatures originating from first order phase transitions in the early Universe. We found that abundant phase transition patterns arise from a physically viable parameter space. Besides, we have also found gravitational wave signals possibly visible by future experiments, such as LISA, BBO and u-DECIGO. Our results stress the importance of gravitational wave detectors in exploring new physics complementary to ground colliders in the multi-messenger astronomy era.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Hao Yang, Felipe F. Freitas, Antonino Marciano, António P. Morais, Roman Pasechnik, João Viana. 2022-05-11. Gravitational-Wave Signatures of Chiral-Symmetric Technicolor. https://doi.org/10.1016/j.physletb.2022.137162
Cite the original work for its findings. Save a collection to share your selection of sources.