Recent content by jcharles513

  1. J

    Time-Dependent Degenerate Pertubation Theory for 3x3 matrix

    Homework Statement H0 = [2,0,0;0,2,0;0,0,4] H1 = [0,1,0;1,0,1;0,1,0] Find energy eigenvalues to 2nd order. Homework Equations The Attempt at a Solution I know that I need to diagonalize the perturbation in the 2x2 subspace (for my 2 degenerate eignevalues of 2 but I'm not sure...
  2. J

    Time-Dependent Degenerate Pertubation Theory for Spin System

    I diagonalized the pertubation (B-part) and then added it the A-part. This made it diagonal. I'm not sure if that's the right way to do it or not? If not, can you get me started on the correct method?
  3. J

    Time-Dependent Degenerate Pertubation Theory for Spin System

    I used the 3x3 subspace and got eigenvalues 0,A+B, and A-B. Is this correct? And the correct procedure?
  4. J

    Time-Dependent Degenerate Pertubation Theory for Spin System

    Degen. Perturb. I'm confused about how to use degenerate perturbation on this system. My understanding of degenerate perturbation is shaky. I know that I need to take a subspace of this matrix that has the degeneracy and then transform the perturbation of that subspace to this new diagonal...
  5. J

    Time-Dependent Degenerate Pertubation Theory for Spin System

    Thank you. That makes sense. I guess I wasn't searching for the right thing in google. I may have more questions after that but this gets me started.
  6. J

    Time-Dependent Degenerate Pertubation Theory for Spin System

    Homework Statement Consider the so-called Spin Hamiltonian H=AS2Z+B(S2X-S2Y) for a system of spin 1. Show that the Hamiltonian in the SZ basis is the 3x3 matrix: \hbar2*[(A,0,B; 0,0,0; B,0,A)].Find the eigenvalues using degenerate pertubation theory. Homework Equations Spin Pauli MatricesThe...
  7. J

    Quantum Mechanical Harmonic Oscillator Problem Variation

    Ah yes of course. So that means I would have a √2 out front for the normalization. So I would multiply each of my probabilities by two. I get 1/∏ for the ground state and 1/2 for the first excited state for t > 0.
  8. J

    Quantum Mechanical Harmonic Oscillator Problem Variation

    I believe so. The normalized initial wavefunction is just A_0*(1/√2)*2*x'*exp(-x'^2/2) where x' = (xmω/hbar)^(1/4) and A_0 = (1/∏)^(1/4). Am I missing something?
  9. J

    Quantum Mechanical Harmonic Oscillator Problem Variation

    I got the probability for hbarω/2 = 1/(2*∏) and then 3hbarω/2 = 1/4. What did you get?
  10. J

    Quantum Mechanical Harmonic Oscillator Problem Variation

    If that's the probability amplitude than the probability would just be the magnitude of that squared correct? So now all I need is to figure out the form of the wave function before and after. t < 0 the wave function is in the groundstate of the half harmonic oscillator so for x >0 it looks...
  11. J

    Quantum Mechanical Harmonic Oscillator Problem Variation

    If I was given the wavefunction ψ(x). The probability is just calculated <\phi_0|ψ(x)>. For t > 0, Ʃ<\phi_n|ψ(x)>|ψ(x)> will be the expanded wavefunction. This means that to get the different values I would just integrate and multiply by the \phi_n^* to get the probabilities where n = 0,1.
  12. J

    Quantum Mechanical Harmonic Oscillator Problem Variation

    Homework Statement At time t < 0 there is an infinite potential for x<0 and for x>0 the potential is 1/2m*w^2*x^2 (harmonic oscillator potential. Then at time t = 0 the potential is 1/2*m*w^2*x^2 for all x. The particle is in the ground state. Assume t = 0+ = 0- a) what is the probability that...
  13. J

    Quantum Mechanics- statistical physics fermi-dirac distribution.

    That makes sense. I hate when the mistake I make is a simple integral mistake. Thanks again. You would think I should know this if I have a final soon. He taught it to us yesterday and testing monday on the final on it. So I've been working on learning it ever since. Thanks, James
  14. J

    Quantum Mechanics- statistical physics fermi-dirac distribution.

    Using the results from Britney Spears, 3d density of states = \frac{1}{2{\pi}^{2}}\frac{2m}{{{\hbar}^{2}}}^{3/2}E^{1/2} and integrating from 0 to ∞ of the density of states multiplied by Fermi-Dirac distribution The result is: \frac{1}{{\pi}^{2}} {\frac{2m}{{\hbar}^{2}}}^{3/2}*E_f * ln(2) I...
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