Fakultät für Physik, Universität Bielefeld, D-33615 Bielefeld, Germany.
Phys Rev Lett. 2010 Mar 26;104(12):121102. doi: 10.1103/PhysRevLett.104.121102. Epub 2010 Mar 25.
Thermal leptogenesis explains the observed matter-antimatter asymmetry of the universe in terms of neutrino masses, consistent with neutrino oscillation experiments. We present a full quantum mechanical calculation of the generated lepton asymmetry based on Kadanoff-Baym equations. Origin of the asymmetry is the departure of the statistical propagator of the heavy Majorana neutrino from the equilibrium propagator, together with CP violating couplings. The lepton asymmetry is calculated directly in terms of Green's functions without referring to "number densities." A detailed comparison with Boltzmann equations shows that conventional leptogenesis calculations have an uncertainty of at least 1 order of magnitude. Particularly important is the inclusion of thermal damping rates in the full quantum mechanical calculation.
热致轻子生成根据中微子质量解释了宇宙中观测到的物质-反物质不对称性,这与中微子振荡实验一致。我们基于 Kadanoff-Baym 方程对生成的轻子不对称性进行了全量子力学计算。不对称性的起源是重 Majorana 中微子的统计传播子偏离平衡传播子,以及 CP 破坏耦合。不对称性直接根据格林函数计算,而不涉及“数密度”。与 Boltzmann 方程的详细比较表明,传统的轻子生成计算至少存在 1 个数量级的不确定性。特别重要的是在全量子力学计算中包含热阻尼率。