So, this makes this chart shown in pink make a lot more sense, because if we're way out at very far distances, essentially what we have here is we're talking about two separate atoms.
因此综合考虑这些因素可以发现这条粉红色曲线很合理,因为如果我们离得非常远,本质上来说,我们讨论的就是两个分开的原子。
and this... In the warm weather you see many, many people there. So... not far from here.
而且……在天气暖和的时候,你可以在那儿看到许许多多的人。所以……离这儿不远。
Now as you can imagine,this is very close to home for me.
可以想到,这离我们的意愿不远了。
For example, when we're talking about radial probability distributions, the most probable radius is closer into the nucleus than it is for the s orbital.
举例来说当我们讨论径向概率分布时,距离原子核最可能的半径是,比s轨道半径,更近的可以离原子核有多近。
As I say, you are very close to Portobello Road. And you could have a...
正如我说的,你离波托贝洛大街很近。然后你可以……
It is not something that can simply be pursued in isolation.
那并非,可以在孤离的情况下寻获的。
So that's just a little bit of a check for yourself, and it should make sense because what you're doing is you're calculating the difference between energy levels, so you just need to flip around which you put first to end up with a positive number here, and that's a little bit of a check that you can do what yourself.
所以你们总要确保括号,离得这项是正的,这是你们自己,可以做的检查,这事很有道理的,因为你们做的是计算能量差,所以你需要调整顺序来保证一个正数,这是你们自己可以做的检查。
And for the s electron, since it can get closer, what we're going to see is that s electrons are actually less shielded than the corresponding p electrons.
对于s电子,因为它可以离得更近,我们可以看到s电子事实上,相对于p电子受到,更少的屏蔽。
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