Spin inversion under dipole-dipole interaction of fermions

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SUMMARY

The discussion centers on the spin inversion of two spin-1/2 fermions interacting via a dipole-dipole potential, defined by the equation \(\hat{V} = A\frac{(\hat{\sigma_1} \cdot \hat{\sigma_2})r^2 - (\sigma_1 \cdot \vec{r})(\sigma_2 \cdot \vec{r})}{r^5}\). Participants clarify that \(A\) represents the interaction strength, not a normalization constant, and emphasize the importance of the time-dependent Schrödinger equation in determining the time evolution of the system. The initial state is identified as a singlet state, and the Hamiltonian is derived from the dipole interaction, leading to the expression \(\hat{H} = \frac{A}{d^3}(\sigma_{1x}\sigma_{2x} + \sigma_{1y}\sigma_{2y})\). The discussion concludes with a focus on diagonalizing the Hamiltonian to construct the evolution operator.

PREREQUISITES
  • Understanding of quantum mechanics, specifically spin-1/2 particles.
  • Familiarity with the time-dependent Schrödinger equation.
  • Knowledge of dipole-dipole interactions in quantum systems.
  • Experience with Hamiltonians and their diagonalization in quantum mechanics.
NEXT STEPS
  • Study the derivation and implications of the time-dependent Schrödinger equation in quantum mechanics.
  • Learn about the properties and applications of dipole-dipole interactions in quantum systems.
  • Explore the process of diagonalizing Hamiltonians and constructing evolution operators.
  • Investigate the significance of antisymmetric wave functions in fermionic systems.
USEFUL FOR

Quantum mechanics students, researchers in theoretical physics, and anyone studying the dynamics of spin-1/2 particles under dipole-dipole interactions will benefit from this discussion.

Siberion
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Homework Statement



Consider two spin 1/2 particles interacting through a dipole-dipole potential

\hat{V} = A\frac{(\hat{\sigma_1} \cdot \hat{\sigma_2})r^2 - (\sigma_1 \cdot \vec{r})(\sigma_2 \cdot \vec{r})}{r^5}

If both spins are fixed at a distance d between each other, and at t = 0 one of them is parallel to the radius vector r, whereas the other one is anti-parallel to r, find the first moment when the orientations of the spins have inverted.

(Please note that the wording of the problem doesn't mention what does A nor sigma mean, but I assume A must be a normalisation constant and sigma/2 the corresponding spin operators)

Homework Equations


[/B]
Time-dependent Schrödinger equation:

-\frac{\hbar^2}{2m}\nabla^2\Psi + V(\mathbf{r})\Psi<br /> = i\hbar \frac{\partial\Psi}{\partial t}

The Attempt at a Solution


[/B]
I don't really know where to start from. This exercise is included in the Identical Particles homework series of my Quantum Mechanics II course. I'm not sure what does "find the first moment" really mean. How can there be "a first moment" when in general all we tan talk about is probabilities of measuring certain observables?

As I have to deal with the time variable, I was guessing it might have something to do with the time-dependent Schödinger equation. I guess the wave function needs to evolve with time, and the orientation of the spins would have to change either continuously or spontaneously. Plus the wave function must be anti-symmetric because we are dealing with fermions... Uhm... I am kind of lost. Any kind of help or reference would be greatly appreciated.
 
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Siberion said:
(Please note that the wording of the problem doesn't mention what does A nor sigma mean, but I assume A must be a normalisation constant and sigma/2 the corresponding spin operators)
##A## is not a normalization constant, but rather parametrizes the strength of the interaction.

Siberion said:

Homework Equations


[/B]
Time-dependent Schrödinger equation:

-\frac{\hbar^2}{2m}\nabla^2\Psi + V(\mathbf{r})\Psi<br /> = i\hbar \frac{\partial\Psi}{\partial t}
The particles being fixed, I don't know why you have a momentum operator there. The first part of such a problem is determining what the Hamiltonian is, and then you can write the proper Schrödinger equation.

Siberion said:
I'm not sure what does "find the first moment" really mean. How can there be "a first moment" when in general all we tan talk about is probabilities of measuring certain observables?
But what if the probabilities are time dependent?

Siberion said:
As I have to deal with the time variable, I was guessing it might have something to do with the time-dependent Schödinger equation. I guess the wave function needs to evolve with time, and the orientation of the spins would have to change either continuously or spontaneously. Plus the wave function must be anti-symmetric because we are dealing with fermions...
Exactly. You have to start by writing the initial state of the system, then find its time evolution (which will be continuous, I don't know why it would be "spontaneous"). As for the parity of the wave function, just make sure that the initial wave function is anti-symmetric, and the time evolution will preserve the parity.
 
Thank you very much for your reply. I am getting some problems with the algebra:

As the particles are fixed, the hamiltonian is going to be equal to the potential energy:

\hat{H} = \hat{V}

Generally speaking,

\hat{\sigma_1} = \sigma_{1x} \hat{i} + \sigma_{1y} \hat{j} + \sigma_{1z} \hat{k}
\hat{\sigma_2} = \sigma_{2x} \hat{i} + \sigma_{2y} \hat{j} + \sigma_{2z} \hat{k}

Let \vec{r} point in the \hat{k} direction, i.e. \vec{r}=z\hat{k}

At t = 0, we have:

\hat{\sigma_1} = \sigma_{1z} \hat{k}
\hat{\sigma_2} =-\sigma_{2z} \hat{k}

(\hat{\sigma_1} \cdot z\hat{k})(\hat{\sigma_2} \cdot z\hat{k}) = -z^2 \sigma_{1z} \sigma_{2z}

whereas

\hat{\sigma_1} \cdot \hat{\sigma_2} = - \sigma_{1z} \sigma_{2z}

thus the potential vanishes at t = 0. I might be messing up at some very basic mistake, right?

Thanks in advance!
 
Sorry, I think my reasoning was erroneous (it still might be)

I think it is better to say that the initial state of the system can be described by the singlet state (because they point in opposite directions at t = 0, and the wave function needs to be antisymmetric):

\Psi(0) = 1/ \sqrt{2} ( |+ \rangle |- \rangle - |-\rangle |+ \rangle)

Now, to construct the time evolution operator, the hamiltonian of the system is given by the dipole interaction. As I said previously, in general we have

\hat{\sigma_1} \cdot \hat{\sigma_2} = \sigma_{1x}\sigma_{2x} + \sigma_{1y}\sigma_{2y} + \sigma_{1z}\sigma_{2z}

and (assuming that \vec{r} points in the k direction

\hat{\sigma_i} \cdot \vec{r} = d \sigma_{iz}

so the second term in the potential would be d^2 \sigma_{1z}\sigma_{2z}, while the first term corresponds to d^2(\sigma_{1x}\sigma_{2x} + \sigma_{1y}\sigma_{2y} + \sigma_{1z}\sigma_{2z})

This way, the hamiltonian would read
\hat{H} = \frac{A}{d^3}(\sigma_{1x}\sigma_{2x} + \sigma_{1y}\sigma_{2y} + \sigma_{1z}\sigma_{2z} - \sigma_{1z}\sigma_{2z})
\hat{H} = \frac{A}{d^3}(\sigma_{1x}\sigma_{2x} + \sigma_{1y}\sigma_{2y})

I am not sure how to proceed from here. I was hoping to get a single-matrix expression for the hamiltonian so I could diagonalise it and construct the evolution operator. Does this procedure make some sense at all?
 
The standard trick is to use ##\vec{S}^2 = (\vec{S}_1+\vec{S}_2)^2 = \vec{S}_1^2+\vec{S}_2^2+2\vec{S}_1\cdot\vec{S}_2##.
 
vela said:
The standard trick is to use ##\vec{S}^2 = (\vec{S}_1+\vec{S}_2)^2 = \vec{S}_1^2+\vec{S}_2^2+2\vec{S}_1\cdot\vec{S}_2##.

do you suggest using that relation on the last part, or did I make a wrong choice from the beginning?
 

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