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classes:2009:fall:phys4101.001:q_a_1118 [2009/11/17 20:44] – gebrehiwet | classes:2009:fall:phys4101.001:q_a_1118 [2009/11/30 09:00] (current) – x500_bast0052 | ||
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====prest121 8:40pm 11/ | ====prest121 8:40pm 11/ | ||
Spin. Griffiths tells me that particle spin is intrinsic angular momentum. | Spin. Griffiths tells me that particle spin is intrinsic angular momentum. | ||
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+ | ===Spherical Chicken Stardate 63255.0=== | ||
+ | Is this magnetic moment perhaps similar but different in the same way that spin is ' | ||
===chavez 10:10am 11/17/09=== | ===chavez 10:10am 11/17/09=== | ||
Even though the particle isn't actually ' | Even though the particle isn't actually ' | ||
- | ===Spherical Chicken Stardate 63255.0=== | ||
- | Is this magnetic moment perhaps similar but different in the same way that spin is ' | ||
==chavez 10:15am 11/17/09== | ==chavez 10:15am 11/17/09== | ||
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==David Hilbert' | ==David Hilbert' | ||
Griffiths advises to not push the analogy too far: an electron is considered a point particle that doesn' | Griffiths advises to not push the analogy too far: an electron is considered a point particle that doesn' | ||
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+ | ==Spherical Chicken == | ||
+ | Multiple sources say that there are two kinds of spin. There may be motion of the electron, but this is not necessarily where the spin comes from. Spin for the electron is an intrinsic property and part of the description of an electron. | ||
+ | I agree with Hilbert. I think this is getting pushed too far. | ||
====Spherical Chicken Stardate 63211.17 ==== | ====Spherical Chicken Stardate 63211.17 ==== | ||
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===Esquire (Age of No Ideas)=== | ===Esquire (Age of No Ideas)=== | ||
I have no idea what an eigenspinor physically represents. | I have no idea what an eigenspinor physically represents. | ||
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+ | ==Devlin== | ||
+ | Neither do I. | ||
+ | |||
===Green Suit 11/17=== | ===Green Suit 11/17=== | ||
This is what I found on Wikipedia: | This is what I found on Wikipedia: | ||
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//For a single spin 1/2 particle, they can be defined as the eigenvectors of the Pauli matrices.// | //For a single spin 1/2 particle, they can be defined as the eigenvectors of the Pauli matrices.// | ||
- | ==Schrodinger' | + | ==Schrodinger' |
- | // Eigenspinors have a similar place as do rotational quantities in classical mechanics do(for instance omega, which is indicated by the axis it is spinning on). Although rotational quantities in classical mechanics are given a direction, by the axis on which it spins around, this does not satisfy the definition of a vector, so we let it be a pseudo-vector. Sometimes we call rotational quantities vectors, because it fits for that situation and we forget to add that is actually on vector like, which is given by " | + | Eigenspinors have a similar place as do rotational quantities in classical mechanics do(for instance omega, which is indicated by the axis it is spinning on). Although rotational quantities in classical mechanics are given a direction, by the axis on which it spins around, this does not satisfy the definition of a vector, so we let it be a pseudo-vector. Sometimes we call rotational quantities vectors, because it fits for that situation and we forget to add that is actually on vector like, which is given by " |
- | //Similarly, in QM, eigenvectors found from our spin operators are pseudo-like in nature, to that of its close relative of the eigenstates, | + | |
+ | |||
+ | Similarly, in QM, eigenvectors found from our spin operators are pseudo-like in nature, to that of its close relative of the eigenstates, | ||
+ | |||
+ | Hope that helps, there is a lot of math behind this, but I don't think it is really important. | ||
+ | |||
+ | |||
+ | ====Schrodinger' | ||
+ | I looked at how Griffths calculated the probability when given a state, but how do you figure out the coefficients of psi+ and psi-? Without this, I am at a lost of calculated probability for certain spin states. | ||
+ | |||
+ | ===David Hilbert' | ||
+ | Do you mean ψ or χ? | ||
+ | |||
+ | ===David Hilbert' | ||
+ | As far as I can tell, a and b are always given or just some constants, so you can use [4.139] as well as the corresponding eigenvalue for whatever operator you're looking at. It is done in example 4.2 in the book for < | ||
+ | |||
+ | ====Schrodinger' | ||
+ | χ | ||
+ | |||
+ | ====Captain America 11/18 10:26 ==== | ||
+ | I'm looking for a better way to conceptualize what we are doing in class, can anyone help me understand how a particle can have 1/2 of a spin? I know " | ||
+ | |||
+ | ===David Hilbert' | ||
+ | If you look at equation 4.135, it seems to say that for those operators the observable values must be given in terms of s and < | ||
+ | |||
+ | Your question seems to be similar to one thing I was thinking of, which is how are these operators and observables grounded to reality? If you're given some operator, which you apply in a lab setting by taking a measurement, | ||
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+ | ====Zeno 11/18 10:45==== | ||
+ | |||
+ | This is a question relative to the discussion and problem 2.38, back when we were working with the infinite square well. If you recall, that was the problem where an infinite square well doubled in size, and the probability of measuring the same energy as before the expansion was 1/2 (I think). That problem was a mathematical curiosity, but our discussion problem last week with the cubical well approximated the FCC system we were describing fairly accurately. My questions regarding this concept are: | ||
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+ | 1. If you expanded the dimensions, or deformed them like in the extra-credit problem, would you get a similar result in terms of having a non-unity probability of measuring the same energy? | ||
+ | |||
+ | 2. Would the energy change between the expectation value of the first and second measurement be the energy required to deform the infinite cubic well (i.e., the FCC structure)? | ||
+ | |||
+ | 3. Does the validity of our approximation of the structure as an infinite cubic well break down if it's not cubic or if it's deformed much? I guess the extra credit problem proved that is does deviate to some extent. | ||
+ | |||
+ | I may have to work this out if I have some extra time. I was just wondering about it because we can deform these structures (at least slightly) and the 1-D infinite square well expansion led to an anti-intuitive result. | ||
+ | |||
+ | === Yuichi === | ||
+ | I like this question. | ||
- | //Hope that helps, there is a lot of math behind this, but I don't think it is really important. // | + | ====Pluto 4ever 11/18 5: |
+ | Does the value of the quantum number s depend on m, or is it completely independent | ||
+ | ===The Doctor 11/19 12:02AM=== | ||
+ | Equation 4.137 should solve the question. | ||
+ | I looks like s is a fixed value for a particular particle while m can change depending on the state of that particle. | ||
+ | ==David Hilbert' | ||
+ | Usually I think of s as being like a constant for each particle; all electrons have spins of 1/2, photons have spin of 1, and so on for every particle. Then when you measure it, spin can be up or down, so the < | ||