And that will end up winning out at basically any realistic temperature where the stuff really is a gas.

在体系仍然处于气体状态的温度下,熵战胜了能量。

麻省理工公开课 - 热力学与动力学课程节选

Whereas under these conditions, these quantities, if you look at free energy change, for example at constant temperature and pressure, H you can still calculate H.

但是，在这些条件下，这些物理量，如果我们考察自由能的变化,例如在恒定的温度和压强下，我们仍然可以计算。

麻省理工公开课 - 热力学与动力学课程节选

Stays a gas, but now the pressure is less, the temperature is less.

它仍然是气态但现在压强变小了，温度降低了。

麻省理工公开课 - 热力学与动力学课程节选