论文标题
宇宙学SU的热力学稳定性（2）-Weak仪表场
Thermodynamic stability of a cosmological SU(2)-weak gauge field
论文作者
论文摘要
CGF宇宙学是从电气过渡到宇宙学的完整理论。它是半古典的。在领先顺序上，唯一的问题是暗物质 - 宇宙学SU（2） - 持量规（CGF）。普通物质是从古典状态周围的波动中进行的转向纠正。 CGF在想象时间是周期性的。它充当标准模型场波动的热浴。在这里，构建了SU（2）量规场波动的初始热状态，并显示为热力学稳定。这是（1）构建所有波动的初始热状态以计算其时间演变的热身，（2）表明初始状态在热力学上稳定，以表明CGF宇宙学在物理上是自然的。
The CGF cosmology is a complete theory of cosmology from the electroweak transition onward. It is semi-classical. At leading order the only matter is dark matter -- a cosmological SU(2)-weak gauge field (the CGF). Ordinary matter is a subleading correction from fluctuations around the classical state. The CGF is periodic in imaginary time. It acts as thermal bath for the fluctuations of the Standard Model fields. Here, the initial thermal state of the SU(2) gauge field fluctuations is constructed and shown to be thermodynamically stable. This is a warm-up for (1) constructing the initial thermal state of all the fluctuations in order to calculate its time evolution and (2) showing that initial state to be thermodynamically stable in order to show that the CGF cosmology is physically natural.
