• You can start from one nucleus and go to the next nucleus, and there are no zero planes, no nodes, nothing.

    你可以从一个核出发,看向另一个核,中间没有平面,没有节点,什么没有。

    麻省理工公开课 - 固态化学导论课程节选

  • We looked at pressure change before, actually, in discussing the third law, the fact that the entropy goes to zero as the absolute temperature goes to zero for a pure,perfect crystal.

    在讨论热力学第三定律的时候,我们讨论过压强变化,即对于纯净的完美晶体,随着温度下降到绝对度熵变成

    麻省理工公开课 - 热力学与动力学课程节选

  • So, the wave function at all of these points in this plane is equal to zero, so therefore, also the wave function squared is going to be equal to zero.

    因此这里的,波函数平方等于,如果我们说在这整个平面上,任何地方找到一个p电子的概率都是

    麻省理工公开课 - 化学原理课程节选

  • When does it hit the ground" is "When is y=0"?

    何时落地"就是"何时位移为"

    耶鲁公开课 - 基础物理课程节选

  • It's not even a zero-- or rather if I have less, you'll have less- that's a negative sum game-- or a zero sum game-- if I have more, you'll have less- it's a fixed pie.

    甚至不是一个…,或者我更少,你会更少,那是负和游戏-,或和游戏,我更多,你就会更少-,饼就那么大。

    哈佛公开课 - 幸福课课程节选

  • Actually, you can't say what the share price is because there are zero shares and they have a zero price, so the value of the price per share is zero over zero and you can't define it.

    实际上你并不能确定它的股价多少,因为股数为,其市值,所以每股价值就是,除以,无法计算

    耶鲁公开课 - 金融市场课程节选

  • And we saw that, you saw that the Joule coefficient for an ideal gas was zero.

    我们会发现,你们会发现,理想气体的焦耳系数是

    麻省理工公开课 - 热力学与动力学课程节选

  • It could be zero. It could be something else.

    它可以是可以不是

    麻省理工公开课 - 热力学与动力学课程节选

  • That's the point where velocity is 0.

    就是速度为的点

    耶鲁公开课 - 基础物理课程节选

  • Anything else, which is to say any spontaneous process, it'll be less than zero.

    其它任何情况下,就是任何自发过程,都将小于

    麻省理工公开课 - 热力学与动力学课程节选

  • but right now you're going to have to take it for granted. So, if the Joule-Thomson coefficient is equal to zero, just like we wrote, du = Cv dT du = Cv dT for an ideal gas, we're going to dH = Cp dT have dH = Cp dT for an ideal gas as well.

    但是现在请你们应该把它看成理所当然的,所以,如果焦耳-汤姆逊系数等于,就像我们写的,对于理想气体,我们可以得到对于理想气体。

    麻省理工公开课 - 热力学与动力学课程节选

  • As T2 goes to zero, the cold reservoir, then this goes to zero and our efficiency approaches one.

    是当T2达到就是低温热源,达到度的时候,效率可以达到一。

    麻省理工公开课 - 热力学与动力学课程节选

  • And so, we can immediately write this du and then we can write du for the universe, which is system plus surroundings is equal to zero.

    因此,我们可以立刻写出这个等式,然后可以写出总的的,就是系统加环境的du,等于

    麻省理工公开课 - 热力学与动力学课程节选

  • I expect that if I add -A to A, I should get the guy who plays the role of 0 in this world, which is the vector of no length.

    我希望如果用 -A 加上 A,应该得到一个矢量,就是一个没有模长的矢量

    耶鲁公开课 - 基础物理课程节选

  • du/dV under constant temperature was equal to zero for an ideal gas. And by analogy, we expect the same thing to be true here, because enthalpy and energy have all this analogy going on here. So let's look at an ideal gas.

    偏U偏V在恒温下等于,可以类比,我们希望在这里一样,因为焓和能量有很强的类比性,让我们看看理想气体,【理想气体】

    麻省理工公开课 - 热力学与动力学课程节选

  • So in this experiment here, delta p is less than zero. You need to have this whole thing greater than zero. So delta T is less than zero as well. So if you're below the inversion temperature and you do the Joule-Thomson experiment, you're going to end up with something that's colder on this side than that side.

    所以在这个实验中,Δp小于,这全部都大于,因此ΔT小于,所以如果在低于转变,温度的情况下做焦耳-汤姆孙实验,最后的结果是,这边的温度比这边低。

    麻省理工公开课 - 热力学与动力学课程节选

  • Last time we reach the third law which is telling us that we can't quite get to zero degrees Kelvin .but that as the temperature approaches zero degrees Kelvin, the absolute entropy of a pure substance in perfect crystalline form is zero.

    上次课我们得到了热力学第三定律,这个定律告诉我们我们无法,达到0K的温度,但是在我们接近绝对度的过程中,以完美晶体形式存在的纯物质的绝对熵,趋向于

    麻省理工公开课 - 热力学与动力学课程节选

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