Chronos said:
Me neither. A detail-less answer, though: there is a jump in energy each time you go past a filled shell.
When you add an electron to an atom, it has to go into a quantum mechanically allowed “state” (everything is in a “state”). If you were to list the allowed states for electrons in order of increasing energy, you’d find that they lie in groups. There is a cluster of two states near the bottom, then a cluster of eight a little ways up, etc. (the cluster of eight is really more like another cluster of two and then a cluster of six, but they’re close enough to call one cluster of eight for our purposes.) Furthermore, if you add an electron to an atom, it can’t go into a state that already has an electron in it. If there are any electrons roaming around looking for a home, they will pick the home that will result in the lowest energy for them. If an electron tries to add itself to a noble gas (like neon, with 10 electrons), it will be forced to live in the 11th state – that high energy 11th state, past the first two clusters. But, if it finds fluorine (which has 9 electron), it gets to be the 10th one, so it gets to live at a lower level, down in that cluster of eight. (And thusly, fluorine is reactive; Neon is not.) These clusters are often called shells, and chemists (and others) speak of the shells as being “filled” as you move across the periodic table.
The question, then, becomes why are there 2 and 2 and 6 and … states in each shell. This is the harder part. What the heck. I’ll see what comes out. It’s long, so you’ll have to bear with me…
Since we don’t have those six months to learn some quantum mechanics (QM herafter), I will just claim some things.
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Angular momentum comes in two types, spin and orbital. Call the total orbital angular momentum L. The square of L can only take on values of the form l*(l+1)*(a constant) with l being any positive integer (1, 2, 3,…). (That’s an italics lowercase “L”, BTW, in case it’s not clear in your font.) The important point in this dense paragraph is that we can index the possible values of total orbital angular momentum by this l thing. We can say, “Our state has l=2.” l can be any non-negative integer.
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You need more than just l to specify a state, though. There are a whole slew of states with a given l. You can further identify a state by its angular momentum along one given axis. Notice the above quantity (L) was the total angular momentum. We can ask how much of that is along one axis (but only one – QM doesn’t allow you to specify the angular momenta along two different axes at the same time!) We can similarly index the allowed values of this quantity by an integer. Let’s call it m. Turns out that m can take on values from -l to l (integers only).
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There’s still more! An l and an m together is still not enough to fully say which state is which. An electron has a certain probability of being here or there. If you give me an l and an m, it turns out you’ve given me information about the angles at which I can expect to see the electron if I was sitting at the nucleus looking out. I still need information about how far away the electron is likely to be (angles aren’t enough) if I want to have a guess at where it is (i.e., if I want to specify the state.) This “distance” quantity can be indexed by an integer, too. Let’s call it n. Turns out that n can equal any positive integer above l.
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One more! The electrons can have two values of spin angular momentum (or simply, spin). We can obviously index this by an integer. Call it s. It can equal 1 or -1 (by convention).
Whew! So, if you give me an l, an m, an n, and an s, you have specified a state, and no two electrons can have the same values for all four of these “quantum numbers”.
Back to energy… You can work out an expression for the energy of a given state. Once you’ve done that, I can say, “How much energy does state (n, l, m, s)=(1,2,-1,1) have?” and you can go to your formula and say, “This much!” If you do this, you’ll find these facts:
- Changing n changes the energy a lot.
- Changing l changes the energy a lot.
- Changing m doesn’t.
- Changing s doesn’t.
So we can now see our clusters (shells) taking shape. Since n and l have a big effect, all the states in a given cluster have the same values for these. If we want to know how many states are in each cluster, we need only ask how many states have the same n’s and l’s. In order of increasing energy:
- n=1, l=0.
m can take on values -l to l, or simply 0. s can take on its two values. Thus, there are two states with n=1, l=0.
- n=2, l=0.
m can take on values -l to l, or simply 0. s can take on its two values. Thus, there are two states with n=2, l=0.
- n=2, l=1.
m can take on the values -1, 0, and 1. s can take on its two values. 2 times 3 equals 6 possible states. Thus, there are six states with n=1, l=0.
And so on. It turns out that the jump in energy from an l=0 state to an l=1 state isn’t that big, so the two and six states are often viewed as a single eight-state shell. Doing this means that l doesn’t matter anymore, and all you need to do is know n to know which shell you’re in. A different way or wording this: n affects the energy most of all.
I really should proofread this, but it is late. I am tired. Apologies.