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classes:2009:fall:phys4101.001:q_a_1123 [2009/11/22 19:49] – gebrehiwet | classes:2009:fall:phys4101.001:q_a_1123 [2009/11/28 22:18] (current) – ely | ||
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- | ===== Nov 23 (Mon) ===== | + | ===== Nov 23 (Mon) Spin operators, probabilities, |
**Return to Q&A main page: [[Q_A]]**\\ | **Return to Q&A main page: [[Q_A]]**\\ | ||
**Q&A for the previous lecture: [[Q_A_1120]]**\\ | **Q&A for the previous lecture: [[Q_A_1120]]**\\ | ||
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===Schrodinger' | ===Schrodinger' | ||
He uses the commutation relation [AB,C] = A[B,C] + [A,C]B. The first term [Lx^2,Lx], is zero since Lx commutes with itself. Then using the commutation relation I introduced you expands [Ly^2,Lx] and [Lz^2,Lx]. Lets just expand [Ly^2,Lx], just to illustrate how the commutation relation works. In this case, A=Ly, B=Ly, and C=Lx. Using the relation we have [Ly*Ly,Lx] = Ly[Ly,Lx] + [Ly,Lx]Ly. He similar does this with [Lz^2, | He uses the commutation relation [AB,C] = A[B,C] + [A,C]B. The first term [Lx^2,Lx], is zero since Lx commutes with itself. Then using the commutation relation I introduced you expands [Ly^2,Lx] and [Lz^2,Lx]. Lets just expand [Ly^2,Lx], just to illustrate how the commutation relation works. In this case, A=Ly, B=Ly, and C=Lx. Using the relation we have [Ly*Ly,Lx] = Ly[Ly,Lx] + [Ly,Lx]Ly. He similar does this with [Lz^2, | ||
+ | ====Daniel Faraday 11/22 8:30pm==== | ||
+ | Where does the minus sign come from when you operate Sz on < | ||
+ | === Zeno 11/22 9pm === | ||
+ | When you multiply the definition matrices for each value you have: | ||
+ | < | ||
+ | === Daniel Faraday 11/23 8am === | ||
+ | But aren't the ' | ||
+ | === Blackbox 11/ | ||
+ | The minus sign comes from " | ||
+ | Therefore < | ||
+ | ==== Zeno 11/22 9:30pm ==== | ||
+ | I'm having a little trouble understanding Larmor precession (Example 4.3, pg 179). Basically a particle with spin 1/2 is at rest in a uniform magnetic field pointing in the k-hat direction. Griffiths shows that the energy of the particle is lowest when the dipole moment is parallel to the field lines, which makes intuitive sense. Where I don't follow is when he just chooses--seemingly arbitrarily--the values of a and b, in terms of an angle alpha, and assumes that the angle is constant in time... finally arriving at the conclusion that the dipole " | ||
+ | ==Schrodinger' | ||
+ | I find myself answering my own question a lot, while I write on here to. | ||
+ | ==== Zeno 11/23 10:15am ==== | ||
+ | This is kind of a tangential question regarding the Stern-Gerlach experiment, but how would one produce an electron beam? And how would the medium through which the beam passes affect the precision? It seems like electrons would be diffracted and the beam would be diffused relatively quickly in air, or even in a decent vacuum chamber that you could reasonably hope to create in a lab. Any thoughts? | ||
+ | |||
+ | ===chavez 11/23 10:56am=== | ||
+ | Cathode ray tubes (http:// | ||
+ | |||
+ | == Zeno 11/25 9am == | ||
+ | I knew there was something obvious that I was overlooking. Thanks! | ||
+ | |||
+ | ===David Hilbert' | ||
+ | As far as I know they actually cooked silver atoms from a furnace. Wikipedia mentions that you need to have particles with a total electric charge of zero because otherwise they would deflect under the influence of a magnetic field before coming out of the apparatus - http:// | ||
+ | |||
+ | ===David Hilbert' | ||
+ | Also http:// | ||
+ | |||
+ | ===Dark Helmet 11/28 10:15=== | ||
+ | I don't know if it is exactly the same thing, but a free-electron laser would be a beam of electrons. | ||
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