Upper limit on first-order electroweak phase transition strength

被引:6
|
作者
AbdusSalam, Shehu [1 ]
Kazemi, Mohammad Javad [1 ]
Kalhor, Layla [1 ]
机构
[1] Shahid Beheshti Univ, Dept Phys, Tehran, Iran
来源
关键词
Electroweak baryogenesis; cosmological gravitational waves; bubble-wall velocity; GRAVITATIONAL-RADIATION; STANDARD MODEL; BARYOGENESIS; WAVES; GROWTH;
D O I
10.1142/S0217751X2150024X
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
For a cosmological first-order electroweak phase transition, requiring no sphaleron washout of baryon number violating processes leads to a lower bound on the strength of the transition. The velocity of the boundary between the phases, the so-called bubble wall, can become ultrarelativistic if the friction due to the plasma of particles is not sufficient to retard the wall's acceleration. This bubble "runaway" should not occur if a successful baryon asymmetry generation due to the transition is required. Using Boedeker-Moore criterion for bubble wall runaway, within the context of an extension of the Standard Model of particle physics with a real gauge-single scalar field, we show that a nonrunaway transition requirement puts an upper bound on the strength of the first-order phase transition.
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页数:14
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