• So, what we're saying is that we have n equals to 4, and m sub I being equal to negative 2.

    我们说的是n等于4,ml等于-2

    麻省理工公开课 - 化学原理课程节选

  • Of course in the reversible case, you're always pushing against an external pressure, which is essentially equal to the internal pressure.

    当然在可逆的情况下,外压力,总是,等于内部压力。

    麻省理工公开课 - 热力学与动力学课程节选

  • z So what we end up seeing is 34 that the z effective is equal to positive 1 . 3 4.

    看到有效的,等于+1。

    麻省理工公开课 - 化学原理课程节选

  • F Then I'm going to print a capital F just % 1f C to be aesthetically interesting equals another %.1fc.

    然后我将打印大写字母,使其比较美观的,等于另一个。

    哈佛公开课 - 计算机科学课程节选

  • 8 You will see if you get --I think the delta here is 1.78, 8 which is roughly 1.8.

    我认为电负性差值应该是1。,约等于1。

    麻省理工公开课 - 固态化学导论课程节选

  • But if we accept the no branching rule, we're saying whether or not we've got identity depends on what's happening elsewhere.

    但如果我们接受了无分支规则,就等于赞同,我们是否有认同感依赖于在别处发生的事情。

    耶鲁公开课 - 死亡课程节选

  • It takes on the value 1 with the probability of 20% and the value of 0 with the probability of 80%.

    等于1的概率是20%,等于0的概率是80%

    耶鲁公开课 - 金融市场课程节选

  • It sets the mean to 0, for s in stocks and then for s in the stocks, it moves it, giving it the bias and the momentum, then it shows the history.

    它会让平均值等于,然后,它会改变它们的值,给它一个偏向值和股价势头值,然后它就会显示历史。

    麻省理工公开课 - 计算机科学及编程导论课程节选

  • Now, gravity, well force, is equal to mass times acceleration, g and the acceleration due to gravity is g.

    是重力,等于质量乘以加速度,由重力导致的加速度是。

    麻省理工公开课 - 热力学与动力学课程节选

  • 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

  • And then we have c, the speed of light, 2.998 times 10 to the 8 meters per second.

    然后我们知道光速等于,2,998乘以10的8次方米每秒。

    麻省理工公开课 - 化学原理课程节选

  • And what I want to point out here is this angular dependence for the p orbitals for the l equals 1 orbital.

    这里我要指出的是,l等于1的p轨道随角度的变化。

    麻省理工公开课 - 化学原理课程节选

  • So this delta energy here is very simply the energy of the initial state minus the energy of the final state.

    很简单的,这个能量差等于,初始能量减去末能量。

    麻省理工公开课 - 化学原理课程节选

  • dT/dp is mu JT. So for a real gas like air, this is a positive number. It's not zero.

    所以对于像空气这样的真实气体,这是一个正数,不等于零。

    麻省理工公开课 - 热力学与动力学课程节选

  • Two plus one equaled three before there were people; two plus one equals three now; two plus one will always equal three.

    在人类出现之前,二加一就等于三,二加一现在等于三,并将永远等于

    耶鲁公开课 - 死亡课程节选

  • So you buy it at a discount and the return you get is of course a hundred minus--the return you get is the discount.

    所以以折价买入,并且回报等于,100减去,回报等于折扣差价

    耶鲁公开课 - 金融市场课程节选

  • And so, in this case, l could equal zero, 2 l could equal one or l could equal two.

    所以这样的话,l可以等于,也可以等于1或。

    麻省理工公开课 - 固态化学导论课程节选

  • We all do believe something makes it true that two plus one equals three, but it's not the fact that empirical objects-- We don't do empirical experiments to see whether two plus one equals three.

    我们都相信有些东西,使2加1等于3是正确的,但这不是说现实的东西,我们不会在现实中做实验,去看看二加一是不是等于

    耶鲁公开课 - 死亡课程节选

  • So if n is greater than or equal to 1 and n is less than or equal to 3, let's just judge this thing a small number arbitrarily.

    所以n大于等于1,并且n小于等于,我们武断的判定它为,一个小的数字。

    哈佛公开课 - 计算机科学课程节选

  • If we look at n equals one, here is n equals one, hydrogen and helium.

    先看n等于1的情况,这里有个n等于1的例子,氢和氦。

    麻省理工公开课 - 固态化学导论课程节选

  • And in the case of the 3 s orbital, that's going to be equal to 11 . 5 times a nought.

    对于3s轨道,它等于11.5a0.

    麻省理工公开课 - 化学原理课程节选

  • So I could have written right here immediately CvdT equals Cv dT, and that was the end of my derivation.

    于是我在这里就可以直接写,来它等于,完成了整个推导。

    麻省理工公开课 - 热力学与动力学课程节选

  • /2 So the bond order is going to be equal to 1/2, and then it will be 2 minus 2.

    它的键序等于,然后乘以2减去2。

    麻省理工公开课 - 化学原理课程节选

  • /2 You can have it equal to plus 1/2, and that's what we call spin up, 1/2 or you can have it equal to minus 1/2, which is what we call spin down.

    它可能会等于,我们叫它自选朝上,或者它等于负,我们叫它自旋朝下。

    麻省理工公开课 - 化学原理课程节选

  • And we know what that's equal to, this is something we've been over and over, ionization energy is simply equal to the negative of the binding energy.

    而且你知道它等于什么,这是我们说过一遍又一遍的,电离能就等于,负的束缚能。

    麻省理工公开课 - 化学原理课程节选

  • PROFESSOR: OK. We can have n 4, l 3, and then, sure, we can have m sub l equal negative 2 if l equals 3 What's the second value of l that we can have?

    教授:嗯,我们有n4,l3,然后我们有ml等于-2,如果l等于3,l可以有的第二个值是多少?

    麻省理工公开课 - 化学原理课程节选

  • l l So what you can do for a 1 s is just take 1 minus 1 and then l is equal to 0, so you have zero radial nodes.

    等于1减去,是等于0的,所以没有节点,这和我们看到的是相符的。

    麻省理工公开课 - 化学原理课程节选

  • So, since the speed of light equals lambda nu, we can say that momentum is equal to h divided by lambda.

    所以,既然光速等于λ乘以υ,我们可以得到动量等于h除以λ

    麻省理工公开课 - 化学原理课程节选

  • For an angular node, we're just talking about what the l value is, so whatever l is equal to is equal to the number of angular nodes you have.

    对于角向节点,我们其实就是在讨论l,的值是多少,因此不管,l,的值等于几,它就等于你所有的角向节点的数目。

    麻省理工公开课 - 化学原理课程节选

  • We're getting further away from the nucleus because we're jumping, for example, from the n equals 2 to the n equals 3 shell, or from the n equals 3 to the n equals 4 shell.

    我们将会离原子核越来越远,因为我们在跃迁,比如从,n,等于,2,的壳层到n等于,3,的壳层,或者从,n,等于,3,的壳层到n等于,4,的壳层。

    麻省理工公开课 - 化学原理课程节选

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