What Are the Eigenvalues and Eigenvectors of This Spin Hamiltonian?

dreamspy
Messages
41
Reaction score
3

Homework Statement



I'm struggling with this question here from my QM class. I have read all my material on Spin (both Griffiths, and a chapter in an Icelandic book). I'we done some problems, but I really have no Idea where to start with this one. It goes something like this:

Two particles have spin 1/2 and are stationary, but their spins interact with this Hamilton operator:

\hat H = \gamma \hat S_3^{(1)} + \gamma \hat S_3^{(2)}

where \bf{S}^{(j)} is the spin operator for particle j, and j=1,2.

As a basis in the state space (hope that's the right word) you can f.x. take u_s^{(1)}u_r^{(2)} wherer,s,=\pm\frac{1}{2}, and \hat S_3^{1}u_s^{1}=shu_s^{j} and \hat S_3^{2}u_r^{2}=rhu_r^{j}

Questions:
(i) Find the eigenvalues and eigenvektors of the Hamilton operator.

(ii) How would the result be if we used this Hamilton operator instead:

\hat H = \gamma \hat S_3^{(1)} + \gamma \hat S_3^{(2)} + \lambda \hat{\underline S}^{(1)}\cdot \lambda \hat{\underline S}^{(2)}

The Attempt at a Solution



Now here is a quick solution I got from my teacher:

(i)
Triplet:


u_{\frac{1}{2}}u_{\frac{1}{2}}
(u_{\frac{1}{2}}u_{-\frac{1}{2}}+u_{-\frac{1}{2}}u_{\frac{1}{2}})\frac{1}{\sqrt 2}
u_{-\frac{1}{2}}u_{-\frac{1}{2}}

\underlince{\hat S}^2 = s(s+1)

The Eigenvalues:

(\gamma S_3^{(1)}-\gamma S_3^{(2)})u_{\frac{1}{2}}u_{\frac{1}{2}} = \gamma \hbar(s+r)u_{\frac{1}{2}}u_{\frac{1}{2}}
(the others should follow the same procedure)

(ii)
Two spin operators:

\underline{\hat S}^{(1)}, \underline{\hat S}^{(2)}

\underline{\hat S}^{(1)}\cdot \underline{\hat S}^{(2)} = \frac{1}{2}(\underline{\hat S}^{2}-(\underline{\hat S}^{(1)})^2-(\underline{\hat S}^{(1)})^2)

\underline{\hat S} = \underline{\hat S}^{(1)} + \underline{\hat S}^{(2)}<br />

\underline{\hat S}} has eigenvalue s(s+1) \hbar ^2, s=0,1


Now I almost have no clue on what's going on here.

Now I suppose the part in the Triplet section, is all possible linear combinations of the u vektors. And the eigenvalue can be read from the right side of the formula below. But could anyone care to comment on this? I'm standing on very shaky ground here :) This is the solution my teacher gave us, nobody has a clue what's going on, and were taking the exam tomorrow :)


Thanks in advance for any comments!
Frímann
 
Physics news on Phys.org
My basic quesion is probably, how do I choose the part in the Triplet section, are those the eigenfunctions? If not then how would I find them?
 
Well if I am not mistaken for two fermions the eigenstate should be anti symmetrical, i.e singlet and not triplet which is symmetric.

But I myself in a shaky ground... :-)
 
\underline{\hat S}^{(1)}\cdot \underline{\hat S}^{(2)} = \frac{1}{2}(\underline{\hat S}^{2}-(\underline{\hat S}^{(1)})^2-(\underline{\hat S}^{(1)})^2) = (1/2)[s(s+1) - (3/2)]<br />

remember

S_{1}^{2} = S_{2}^{2} = (1/2)[(1/2) + 1]
 
But what if we have u_{\frac{1}{2}}^1u_{-\frac{1}{2}}^2

How do we calculate \underline{\hat S}^2u_{\frac{1}{2}}^1u_{-\frac{1}{2}}^2 ?
 
[QUOTE said:
dreamspy;2493358]But what if we have u_{\frac{1}{2}}^1u_{-\frac{1}{2}}^2

How do we calculate \underline{\hat S}^2u_{\frac{1}{2}}^1u_{-\frac{1}{2}}^2 ?
[/QUOTE]

That is a singlet state which has s = 0.
 
Hello everyone, I’m considering a point charge q that oscillates harmonically about the origin along the z-axis, e.g. $$z_{q}(t)= A\sin(wt)$$ In a strongly simplified / quasi-instantaneous approximation I ignore retardation and take the electric field at the position ##r=(x,y,z)## simply to be the “Coulomb field at the charge’s instantaneous position”: $$E(r,t)=\frac{q}{4\pi\varepsilon_{0}}\frac{r-r_{q}(t)}{||r-r_{q}(t)||^{3}}$$ with $$r_{q}(t)=(0,0,z_{q}(t))$$ (I’m aware this isn’t...
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
Back
Top