• pV=RT p plus a over v bar squared times v bar minus b equals r t. All right if you take a equal to zero, these are the two parameters, a and b. If you take those two equal to zero you have p v is equal to r t.

    我们就回到,也就是理想气体,状态方程,下面我们来看看,这个方程。

    麻省理工公开课 - 热力学与动力学课程节选

  • It can't just be a matter of not P-functioning.

    肯定不止和人格功能性有关。

    耶鲁公开课 - 死亡课程节选

  • Texts that insist on a central sanctuary are probably Josiah's time or later. And there are many sections of P that don't seem to assume a central sanctuary.

    一些章节坚持中心圣所,则可能在约西亚或之后时期,P资源中有很多部分,并没有呈现出一个中心圣所。

    耶鲁公开课 - 旧约导论课程节选

  • v We don't know what it is yet. In order to change this from a p to a V, you have to use the chain rule. So let's use the chain rule.

    为了把这里的p变成,我们需要利用链式法则,好,让我们使用链式法则。

    麻省理工公开课 - 热力学与动力学课程节选

  • So that's true for a hydrogen atom, it doesn't matter if you're in a p or an s orbital, their energies are the same.

    这对于氢原子来说是这样的,不论是p或,者s轨道,能量是一样的。

    麻省理工公开课 - 化学原理课程节选

  • But we don't have a P-functioning body.

    但这不是具有人类能力的肉体

    耶鲁公开课 - 死亡课程节选

  • We want a relationship in p-V space, not in T-V space. So we're going to have to do something about that. But first, it turns out that now we have this R over Cv.

    我们想要p-V空间中的结果,而不是T-V空间中的,因此需要做一些变换,先来看现在的关系,它跟R/Cv有关。

    麻省理工公开课 - 热力学与动力学课程节选

  • And this shows that G is written naturally as a function of T and p.

    这表明G可以很自然的,写成Tp的函数。

    麻省理工公开课 - 热力学与动力学课程节选

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