Spontaneous baryogenesis from axions with generic couplings

被引:35
|
作者
Domcke, Valerie [1 ,2 ,3 ]
Ema, Yohei [1 ]
Mukaida, Kyohei [1 ]
Yamada, Masaki [3 ,4 ]
机构
[1] DESY, Notkestr 85, D-22607 Hamburg, Germany
[2] CERN, Theoret Phys Dept, 1 Esplanade Particules, CH-1211 Geneva 23, Switzerland
[3] Ecole Polytech Fed Lausanne, Lab Particle Phys & Cosmol, Inst Phys, CH-1015 Lausanne, Switzerland
[4] Tohoku Univ, Frontier Res Inst Interdisciplinary Sci, Sendai, Miyagi 9808578, Japan
基金
欧洲研究理事会;
关键词
Cosmology of Theories beyond the SM; Thermal Field Theory; CP CONSERVATION;
D O I
10.1007/JHEP08(2020)096
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Axion-like particles can source the baryon asymmetry of our Universe through spontaneous baryogenesis. Here we clarify that this is a generic outcome for essentially any coupling of an axion-like particle to the Standard Model, requiring only a non-zero velocity of the classical axion field while baryon or lepton number violating interactions are present in thermal bath. In particular, coupling the axions only to gluons is sufficient to generate a baryon asymmetry in the presence of electroweak sphalerons or the Weinberg operator. Deriving the transport equation for an arbitrary set of couplings of the axion-like particle, we provide a general framework in which these results can be obtained immediately. If all the operators involved are efficient, it suffices to solve an algebraic equation to obtain the final asymmetries. Otherwise one needs to solve a simple set of differential equations. This formalism clarifies some theoretical subtleties such as redundancies in the axion coupling to the Standard Model particles associated with a field rotation. We demonstrate how our formalism automatically evades potential pitfalls in the calculation of the final baryon asymmetry.
引用
收藏
页数:49
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