• If this were to be an absolute zero Kelvin, then we could we can have something, T2 Sorry, it's T2.

    如果它等于绝对零度,我们可以,对不起,这是。

    麻省理工公开课 - 热力学与动力学课程节选

  • In principle, this value, this efficiency, can approach 1 as the low temperature approaches absolute zero.

    这个值,效率,当低温热源的温度1,是据对零度时可以达到一。

    麻省理工公开课 - 热力学与动力学课程节选

  • And the temperature scale that turns out to be well-defined and ends up giving us the concept of an absolute zero is the ideal gas thermometer.

    比如理想气体温标,它有精确的定义,并能引出绝对零度的概念,今天我们就先来谈谈它。

    麻省理工公开课 - 热力学与动力学课程节选

  • If I had taken as my interpolation scheme, my white curve here, I could go to infinity and have the equivalent of absolute zero being at infinity, minus infinity.

    要注意,如果我们采用,像图中白线这样的插值方案的话,我就可以一直降温下去,相应的绝对零度点。

    麻省理工公开课 - 热力学与动力学课程节选

  • And so now, instead of using these reference points for the Kelvin scale, we use the absolute zero, which isn't going to care what the pressure is.

    就像理想气体温标,与气体的种类无关一样,具有普适性,在开尔文温标中。

    麻省理工公开课 - 热力学与动力学课程节选

  • So, this temperature, this absolute zero here, which is absolute zero on the Kelvin scale.

    在负无穷处,现在把绝对零度定义为,开尔文温标中的0度。

    麻省理工公开课 - 热力学与动力学课程节选

  • And our other reference point is the triple point of water - reference points become zero Kelvin, absolute zero, and the triple point.

    而使用绝对零度,它与压强无关,是最低的温度,另一个参考点是水的三相点。

    麻省理工公开课 - 热力学与动力学课程节选

  • The only way you could possibly contemplate it is to be working at absolute zero Kelvin.

    在绝对零度下工作,猜一下热力学第三定律告诉我们什么?

    麻省理工公开课 - 热力学与动力学课程节选

  • There is an absolute zero of entropy, and that's really what we learn.

    而熵是有绝对零点的,这就是我们学到的。

    麻省理工公开课 - 热力学与动力学课程节选

  • So the concept of an absolute zero, a temperature below which you just can't go, that's directly out of the scheme here, this linear interpolation scheme with these two reference points.

    这就是绝对零度,这样,从线性插值的图像出发,我们得到了绝对零度的概念,你永远无法达到,低于绝对零度的状态。

    麻省理工公开课 - 热力学与动力学课程节选

  • That's the absolute zero.

    有意义的最低的温度。

    麻省理工公开课 - 热力学与动力学课程节选

  • 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零度熵也变成零。

    麻省理工公开课 - 热力学与动力学课程节选

  • The absolute number that you assign to it is something that's arbitrary. You have to set what the zero is. And so there's a well-understood convention for what the zero is.

    你指定给它的绝对值是有任意性的,你需要设定零点的位置,因此有一个经过充分研究的,关于设定零点的约定。

    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零度的过程中,以完美晶体形式存在的纯物质的绝对熵,也趋向于零。

    麻省理工公开课 - 热力学与动力学课程节选

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