McDonald J
Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, Scotland.
Phys Rev Lett. 2000 May 22;84(21):4798-801. doi: 10.1103/PhysRevLett.84.4798.
A large neutrino asymmetry could have significant observable consequences for nucleosynthesis and the cosmic microwave background. If the baryon asymmetry originates via the Affleck-Dine mechanism along a d = 4 flat direction of the scalar potential in the minimal supersymmetric standard model and if the lepton asymmetry originates via Affleck-Dine leptogenesis along a d = 6 direction, corresponding to the lowest dimension directions conserving R parity, then the ratio n(L)/n(B) is naturally in the range 10(8)-10(9). As a result, a potentially observable neutrino asymmetry is correlated with a baryon asymmetry of the order of 10(-10).
较大的中微子不对称性可能对核合成和宇宙微波背景产生显著的可观测后果。如果重子不对称性通过阿弗莱克-丁机制在最小超对称标准模型中标量势的d = 4平坦方向上产生,并且轻子不对称性通过阿弗莱克-丁轻子生成在d = 6方向上产生,对应于守恒R宇称的最低维方向,那么n(L)/n(B)的比值自然处于10(8)-10(9)的范围内。因此,一个潜在可观测的中微子不对称性与约为10(-10)量级的重子不对称性相关。