Bubble trouble: A review on electroweak baryogenesis
5 affiliations
- 1Theoretical Physics Department , CERN , 1 Esplanade des Particules , CH-1211 Geneva 23 , Switzerland
- 2Institute for Theoretical Physics , University of Amsterdam , Science Park 904 , 1098 XH Amsterdam , The Netherlands
- 3Nikhef , Science Park 105 , 1098 XG Amsterdam , The Netherlands
- 4Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, 6500 GL Nijmegen, The Netherlands
- 5Nikhef, Science Park 105, 1098 XG Amsterdam, The Netherlands
Abstract
The origin of the universal asymmetry between matter and antimatter remains a mystery. Electroweak baryogenesis is a well-motivated mechanism for generating the asymmetry dynamically, using interesting features of the Standard Model. In addition, it relies on beyond-the-Standard Model physics active around the electroweak scale: new physics coupling to the Higgs to make the electroweak phase transition first order, and a new mechanism of CP violation. The relatively low energy scale at which electroweak baryogenesis occurs makes certain aspects of the mechanism testable through collider experiments, electric dipole moment measurements, and gravitational wave observations. However, scenarios of electroweak baryogenesis are increasingly challenged by results from contemporary experiments. The developing experimental programs will play a crucial role in either falsifying or detecting the new physics responsible for electroweak baryogenesis. To achieve this, it is essential to make precise predictions for the baryon asymmetry and the corresponding experimental signatures within specific scenarios. This review aims to provide a comprehensive overview of the rich physics involved in these predictions. Our goal is to offer a practical computational guide, with a focus on recent developments in the field.
Related
- Electroweak baryogenesis from charged current anomalies in B meson decays
- Electroweak-Scale Cosmic Magnetism: Magnetogenesis, Baryogenesis, Phase Transitions and Gravitational Waves
- Electroweak Baryogenesis in Top-Philic Type-III Two-Higgs-Doublet Model motivated by the tt̅ Excess at the LHC
- Gravitational baryogenesis in asymptotically safe gravity
- Signatures of Leptophilic Baryogenesis at Muon Colliders
BibTeX
@article{vis2026bubble,
title = {{Bubble trouble: A review on electroweak baryogenesis}},
author = {Jorinde van de Vis and Jordy de Vries and Marieke Postma},
journal = {Progress in Particle and Nuclear Physics},
year = {2026},
month = may,
doi = {10.1016/j.ppnp.2026.104244},
url = {https://doi.org/10.1016/j.ppnp.2026.104244},
note = {CC BY},
}
RIS
TY - JOUR
TI - Bubble trouble: A review on electroweak baryogenesis
AU - Jorinde van de Vis
AU - Jordy de Vries
AU - Marieke Postma
PY - 2026
DA - 2026/05/12
JO - Progress in Particle and Nuclear Physics
DO - 10.1016/j.ppnp.2026.104244
UR - https://doi.org/10.1016/j.ppnp.2026.104244
AB - The origin of the universal asymmetry between matter and antimatter remains a mystery. Electroweak baryogenesis is a well-motivated mechanism for generating the asymmetry dynamically, using interesting features of the Standard Model. In addition, it relies on beyond-the-Standard Model physics active around the electroweak scale: new physics coupling to the Higgs to make the electroweak phase transition first order, and a new mechanism of CP violation. The relatively low energy scale at which electroweak baryogenesis occurs makes certain aspects of the mechanism testable through collider experiments, electric dipole moment measurements, and gravitational wave observations. However, scenarios of electroweak baryogenesis are increasingly challenged by results from contemporary experiments. The developing experimental programs will play a crucial role in either falsifying or detecting the new physics responsible for electroweak baryogenesis. To achieve this, it is essential to make precise predictions for the baryon asymmetry and the corresponding experimental signatures within specific scenarios. This review aims to provide a comprehensive overview of the rich physics involved in these predictions. Our goal is to offer a practical computational guide, with a focus on recent developments in the field.
SN - 0146-6410
SN - 1873-2224
ER -