On the wall velocity dependence of electroweak baryogenesis

被引:37
作者
Dorsch, Glauber C. [1 ]
Huber, Stephan J. [2 ]
Konstandin, Thomas [3 ]
机构
[1] Univ Fed Minas Gerais, Dept Fis, BR-31270901 Belo Horizonte, MG, Brazil
[2] Univ Sussex, Brighton BN1 9QH, E Sussex, England
[3] DESY, Notkestr 85, D-22607 Hamburg, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2021年 / 08期
基金
英国科学技术设施理事会;
关键词
baryon asymmetry; cosmological phase transitions; particle physics - cosmology connection; physics of the early universe;
D O I
10.1088/1475-7516/2021/08/020
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We re-evaluate the status of supersonic electroweak baryogenesis using a generalized fluid Ansatz for the non-equilibrium distribution functions. Instead of truncating the expansion to first order in momentum, we allow for higher order terms as well, including up to 21 fluctuations. The collision terms are computed analytically at leading-log accuracy. We also point out inconsistencies in the standard treatments of transport in electroweak baryogenesis, arguing that one cannot do without specifying an Ansatz for the distribution function. We present the first analysis of baryogenesis using the fluid approximation to higher orders. Our results support the recent findings that baryogenesis may indeed be possible even in the presence of supersonic wall velocities.
引用
收藏
页数:24
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