Electroweak bubble wall speed limit

被引:216
作者
Boedeker, Dietrich [1 ]
Moore, Guy D. [2 ]
机构
[1] Univ Bielefeld, Fac Phys, D-33501 Bielefeld, Germany
[2] Tech Univ Darmstadt, Inst Kernphys, Schlossgartenstr 2, D-64289 Darmstadt, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2017年 / 05期
基金
加拿大自然科学与工程研究理事会;
关键词
cosmological phase transitions; primordial gravitational waves (theory); baryon asymmetry; primordial magnetic fields; FLUCTUATION-DISSIPATION FORMULA; PHASE-TRANSITION; BARYOGENESIS; NUCLEATION; VELOCITY; GROWTH;
D O I
10.1088/1475-7516/2017/05/025
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In extensions of the Standard Model with extra scalars, the electroweak phase transition can be very strong, and the bubble walls can be highly relativistic. We revisit our previous argument that electroweak bubble walls can "run away," that is, achieve extreme ultrarelativistic velocities gamma similar to 10(14). We show that, when particles cross the bubble wall, they can emit transition radiation. Wall-frame soft processes, though suppressed by a power of the coupling alpha, have a significance enhanced by the gamma-factor of the wall, limiting wall velocities to gamma similar to 10(14). Though the bubble walls can move at almost the speed of light, they carry an infinitesimal share of the plasma's energy.
引用
收藏
页数:14
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