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classes:2009:fall:phys4101.001:lec_notes_1125 [2009/11/29 10:59] – x500_razi0001 | classes:2009:fall:phys4101.001:lec_notes_1125 [2009/11/29 22:20] (current) – yk | ||
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Wrong! When you separate the particles based on their x-direction spin, you lose all your knowledge of the z-direction spin. In fact, you cause the z-direction spin to become indeterminate. This is because x-direction spin and z-direction spin are incompatible observables. | Wrong! When you separate the particles based on their x-direction spin, you lose all your knowledge of the z-direction spin. In fact, you cause the z-direction spin to become indeterminate. This is because x-direction spin and z-direction spin are incompatible observables. | ||
- | |||
====Section 2: Addition of angular momenta==== | ====Section 2: Addition of angular momenta==== | ||
===Part 1: Why do it? Why do we care about adding angular momenta?=== | ===Part 1: Why do it? Why do we care about adding angular momenta?=== | ||
+ | Example: when looking at fine structure, < | ||
+ | In a magnetic field, the hamiltonian will have an extra term, so that | ||
+ | < | ||
+ | , and < | ||
+ | |||
+ | Notice that we are going to ignore the < | ||
+ | |||
+ | Anyway, if the magnetic field we apply is in the < | ||
+ | < | ||
+ | In that case, which is associated with the Zeeman Effect, < | ||
+ | |||
+ | If the magnetic field is not on, then the < | ||
+ | < | ||
+ | |||
+ | So, we want to find eigenfunctions of < | ||
+ | |||
+ | Well, if we let < | ||
+ | < | ||
+ | < | ||
+ | and then we can use < | ||
+ | |||
+ | In short, let's just trust that this addition of angular momentum technique we develop in this chapter will be very useful later, and move on to the technique itself. | ||
+ | |||
+ | ===Part 2: How to add angular momenta=== | ||
+ | The basic idea of the following section is to define < | ||
+ | |||
+ | First of all, we know that | ||
+ | < | ||
+ | < | ||
+ | |||
+ | For each of the two Hilbert spaces (one for S1 and one for S2) we have a pair of spin-up and spin-downs represented as follows: | ||
+ | < | ||
+ | < | ||
+ | < | ||
+ | < | ||
+ | Remember these can also be represented with up and down arrows, which will be done below.\\ | ||
+ | |||
+ | We have to be careful with these since each pair is associated with a different Hilbert space. If we want to be able to represent combined states of S1 and S2, one way to do it is to use a column 4-vector and define it like this...\\ | ||
+ | < | ||
+ | \uparrow\downarrow = \begin{pmatrix} 0\\ 1 \\0\\0\end{pmatrix} \:\: | ||
+ | \downarrow\uparrow = \begin{pmatrix} 0\\ 0 \\1\\0\end{pmatrix} \:\: | ||
+ | \downarrow\downarrow = \begin{pmatrix} 0\\ 0 \\0\\1\end{pmatrix}</ | ||
+ | |||
+ | Now, let's try adding < | ||
+ | < | ||
+ | < | ||
+ | |||
+ | Now, how do we find this sum? \\ | ||
+ | Well, we already know that \\ | ||
+ | < | ||
+ | < | ||
+ | |||
+ | but what about < | ||
+ | |||
+ | Well,\\ | ||
+ | < | ||
+ | |||
+ | Now, we know all of the spin matrices in the above expression, so we can just plug them all in and solve, and we will get \\ | ||
+ | < | ||
+ | //Yuichi// I mis-stated here. It should have been:< | ||
+ | |||
+ | Using a similar technique, we can also find (with corrections)... | ||
+ | |||
+ | < | ||
+ | 2\vec{S_1}\cdot\vec{S_2}\downarrow\uparrow = -\frac{1}{2}\hbar^2\downarrow\uparrow + \hbar^2\downarrow\uparrow \\ | ||
+ | 2\vec{S_1}\cdot\vec{S_2} \downarrow\downarrow = \frac{1}{2}\hbar^2\downarrow\downarrow \\</ | ||
+ | |||
+ | |||
+ | |||
+ | We can use our 4 element column vector notation described above to represent < | ||
+ | < | ||
+ | |||
+ | //Yuichi// and this should have been < | ||
- | Me or the other guy will finish the notes later; happy Thanksgiving! | + | \\ |
+ | \\ | ||
+ | Happy Thanksgiving! | ||
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**To go back to the lecture note list, click [[lec_notes]]**\\ | **To go back to the lecture note list, click [[lec_notes]]**\\ |