Transition between two states probability

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Homework Help Overview

The discussion revolves around the probability of transitioning between two quantum states, specifically using time-dependent perturbation theory. Participants are exploring the mathematical formulation of probabilities related to state transitions and time evolution operators.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants discuss the calculation of transition probabilities using different methods, including perturbation theory and time evolution operators. There are attempts to derive expressions for probabilities and eigenstates, along with questions about the correctness of these approaches.

Discussion Status

Some participants express uncertainty about the results obtained for different parts of the problem, particularly regarding the eigenvalues and eigenstates. There is an ongoing exploration of the implications of non-commuting operators and the correct formulation of the Hamiltonian. Guidance is provided on the relationship between the eigenstates and the time evolution of the system.

Contextual Notes

Participants are navigating constraints related to the Hamiltonian's formulation and the assumptions about the system's initial conditions. There is mention of the need to find eigenstates and the significance of expressing states in relation to the net magnetic field direction.

unscientific
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Homework Statement



i6witl.png


Part (a): Show probability to transit from state i to j is given by:
Part (b)i: Use answer in part (a) to find probability
Part (b)ii: Use time evolution to find probability

Homework Equations


The Attempt at a Solution



Part (a) was alright, bookwork question on time dependent perturbation theory.

What's interesting was, I got different answers for part (b)i and (b)ii.

Part (b)i

Amplitude of finding particle in state j:

a_j = \frac{1}{i\hbar}\int V_{ji} exp(\frac{i\Delta E}{\hbar}t) dt

In this case, ##\Delta E = 2\mu B##, and since the additional hamiltonian is ##-\mu b \sigma_x##, hence ##V_{ji} = \mu b##.

a_j = \frac{1}{i\hbar} V_{ij}^{*} \int_0^T exp(\frac{i2\mu B}{\hbar}t) dt

|a_j|^2 = (\frac{b}{B})^2 sin^2(\frac{\mu B l}{\hbar v})

Part (b)ii

The time evolution operator is given by ##U_{(t)} = e^{-\frac{iH}{\hbar}t}## such that ##|\psi_t> = U_t |\psi_0>##.

To find the time evolution operator:
e^{-\frac{iH}{\hbar}t} = exp(\frac{i\mu B \sigma_z}{\hbar}t) exp(\frac{i\mu b \sigma_x}{\hbar}t)

For each of the exponentials, I found them in matrix form:

2884jnb.png


Now to overlap the desired |-,B> = (0 1) state with evolved state ##|\psi_t>##:

<-,B|\psi_t> = i sin (\frac{\mu b}{\hbar}t) exp(\frac{-i\mu B}{\hbar}t)

Thus, probability is ##sin^2 (\frac{\mu b l}{\hbar v})##
 
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unscientific said:
To find the time evolution operator:
e^{-\frac{iH}{\hbar}t} = exp(\frac{i\mu B \sigma_z}{\hbar}t) exp(\frac{i\mu b \sigma_x}{\hbar}t)

Keeping in mind that ##\sigma_z## and ##\sigma_x## do not commute, is this correct?
 
TSny said:
Keeping in mind that ##\sigma_z## and ##\sigma_x## do not commute, is this correct?

I was thinking about that, as the original operator was: ##U = e^{-\frac{iH}{\hbar}t} = exp(\frac{i\mu B \sigma_z}{\hbar}t + \frac{i\mu b \sigma_x}{\hbar}t)##

Do I use ##\sigma_x \sigma_z## or ## \sigma_z \sigma_x##?

And is the answer to (b)i correct?
 
unscientific said:
And is the answer to (b)i correct?

Edit: I think your answer to (b)i is correct.

For (b)ii, can you find the exact eigenvalues and eigenvectors for ##H=-\mu( B \sigma_z+ b \sigma_x)##?
 
Last edited:
TSny said:
Edit: I think your answer to (b)i is correct.

For (b)ii, can you find the exact eigenvalues and eigenvectors for ##H=-\mu( B \sigma_z+ b \sigma_x)##?

The eigenvalues are ##\lambda = \pm \mu \sqrt{b^2 + B^2}##. I'm having trouble finding the eigenstates. What's the point of finding them anyway?
 
unscientific said:
The eigenvalues are ##\lambda = \pm \mu \sqrt{b^2 + B^2}##.

OK.

I'm having trouble finding the eigenstates. What's the point of finding them anyway?

How have you gone about it?

The eigenstates of H have a simple time evolution and they can be used as basis states for expressing the spin state of the particle.
 
TSny said:
OK.
How have you gone about it?

The eigenstates of H have a simple time evolution and they can be used as basis states for expressing the spin state of the particle.

For example, consider ##\lambda = \mu \sqrt{b^2 + B^2}##, then I get these two simultaneous equations:

Be_1 + be_2 = \sqrt{b^2 + B^2}(e_1)
be_1 - Be_2 = \sqrt{b^2 + B^2}(e_2)

By the way, what's wrong with my method with the time evolution operator ##U_t## above?
 
unscientific said:
For example, consider ##\lambda = \mu \sqrt{b^2 + B^2}##, then I get these two simultaneous equations:

Be_1 + be_2 = \sqrt{b^2 + B^2}(e_1)
be_1 - Be_2 = \sqrt{b^2 + B^2}(e_2)

Looks like you might have forgotten the minus sign in the expression for the Hamiltonian, so some signs are incorrect here. The two equations are not independent, but you can use normalization to get a second condition.

There is another way to get the eigenstates if you note that the particle will be in a net magnetic field that lies in the xz plane at an angle of θ = tan-1(b/B) to the z-axis. So, the eigenstates will be spin "up" and "down" along the direction of the net magnetic field. So, if you know how to rotate spin 1/2 states, you could rotate a spin up along the z-axis to produce a spin up or spin down along the net magnetic field direction.

By the way, what's wrong with my method with the time evolution operator ##U_t## above?

I don't think the method is wrong, but you can't factor the time evolution operator as you did.
 
TSny said:
Looks like you might have forgotten the minus sign in the expression for the Hamiltonian, so some signs are incorrect here. The two equations are not independent, but you can use normalization to get a second condition.

ok I ended up with this pair of simultaneous equations for the positive eigenvalue:

-Be_1 - be_2 = \sqrt{b^2+B^2}e_1
-be_1+Be_2 = \sqrt{b^2+B^2}e_2

Still can't solve it simply, I'm trying to get something simple like ##e_1=\pm e_2##.

TSny said:
There is another way to get the eigenstates if you note that the particle will be in a net magnetic field that lies in the xz plane at an angle of θ = tan-1(b/B) to the z-axis. So, the eigenstates will be spin "up" and "down" along the direction of the net magnetic field. So, if you know how to rotate spin 1/2 states, you could rotate a spin up along the z-axis to produce a spin up or spin down along the net magnetic field direction.



I don't think the method is wrong, but you can't factor the time evolution operator as you did.

For a spin orientation (θ,ø) where θ = tan-1(b/B) to z-axis, the spin of the particle can be characterized as:

|+,t\rangle = e^{\frac{-i\phi}{2}} cos \left(\frac{\theta}{2}\right) |+,z\rangle + e^{\frac{i\theta}{2}} sin \left(\frac{\theta}{2}\right)|-,\rangle

Since ##\phi = 0##:

|+,t=0\rangle = cos \left(\frac{\theta}{2}\right) |+,z\rangle + sin \left(\frac{\theta}{2}\right)|-,z\rangle

This is the particle's spin state at t=0.

So at time t, the particle evolves as:

|+,t\rangle = cos (\frac{\theta}{2})*exp\left(\frac{-i\mu\sqrt{b^2+B^2}}{\hbar}t\right) |+,z\rangle + sin (\frac{\theta}{2})*exp\left(\frac{i\mu\sqrt{b^2+B^2}}{\hbar}t\right) |-,z\rangle

Thus the probability of it being in the ##|-,z\rangle## state at time t is

sin^2\left(\frac{\theta}{2}\right) = \frac{1}{2}\left[1 - sin\theta\right]

Using ##tan\theta = \frac{b}{B}##, ##sin\theta = \frac{b}{\sqrt{b^2+B^2}}##:


Probability is ##\frac{1}{2}\left[1 - \frac{b}{\sqrt{b^2+B^2}}\right]##

This is clearly a different answer as it is a constant and there should be a factor of ##sin^2(\theta)## according to perturbation theory..
 
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  • #10
unscientific said:
ok I ended up with this pair of simultaneous equations for the positive eigenvalue:

-Be_1 - be_2 = \sqrt{b^2+B^2}e_1
-be_1+Be_2 = \sqrt{b^2+B^2}e_2

Still can't solve it simply, I'm trying to get something simple like ##e_1=\pm e_2##.

Looks good.
I found it helpful to divide both sides of the first equation by ##\small \sqrt{b^2+B^2}## and then express the coefficients in terms of cos θ and sin θ where θ = tan-1(b/B).

|+,t=0\rangle = cos \left(\frac{\theta}{2}\right) |+,z\rangle + sin \left(\frac{\theta}{2}\right)|-,z\rangle
This is the particle's spin state at t=0.

The right side of your equation represents a state with spin that is parallel to the net B-field.

But this is not the spin state at t = 0. At t = 0 the particle has spin in the z-direction.

So at time t, the particle evolves as:

|+,t\rangle = cos (\frac{\theta}{2})*exp\left(\frac{-i\mu\sqrt{b^2+B^2}}{\hbar}t\right) |+,z\rangle + sin (\frac{\theta}{2})*exp\left(\frac{i\mu\sqrt{b^2+B^2}}{\hbar}t\right) |-,z\rangle

No. The states ##|+,z\rangle## and ##|-,z\rangle## do not evolve with time this way. It's the spin states that are parallel or antiparallel to Bnet that have simple time evolution.
 
  • #11
TSny said:
Looks good.
I found it helpful to divide both sides of the first equation by ##\small \sqrt{b^2+B^2}## and then express the coefficients in terms of cos θ and sin θ where θ = tan-1(b/B).
Yeah I got these two eigenstates:
551r2x.png


At t = 0, the state of the particle is along z-axis, but we wish to express it in basis along net B field, B'.

|\psi_0\rangle = |+,z\rangle = a|+,B'\rangle + c|-,B'\rangle

This implies that ##a = \langle+,B'|+,z\rangle = \frac{1}{\sqrt{2sec\theta(sec \theta + 1)}}(1+sec\theta) = \sqrt{\frac{1+cos\theta}{2}}## and ##c = \langle-,B'|+,z\rangle = \frac{1}{\sqrt{2sec\theta(sec\theta-1)}}(1-sec\theta) = -\sqrt{\frac{1-cos\theta}{2}}##

TSny said:
The right side of your equation represents a state with spin that is parallel to the net B-field.

But this is not the spin state at t = 0. At t = 0 the particle has spin in the z-direction.
No. The states ##|+,z\rangle## and ##|-,z\rangle## do not evolve with time this way. It's the spin states that are parallel or antiparallel to Bnet that have simple time evolution.

That's true, because these are basis kets in the z-direction, and not in direction of tan θ. I suppose the above method can only be used.

Following from above, the ket at time t is:
|\psi_t\rangle = a*exp(\frac{-i\lambda_{+}}{\hbar}t)|+,B'\rangle + c*exp(\frac{-i\lambda_{-}}{\hbar}t)|-,B'\rangle

Thus probability amplitude is:

\langle -,z|\psi_t\rangle = a*exp(\frac{-i\lambda_{+}}{\hbar}t)\langle-,z|+,B'\rangle + c*exp(\frac{-i\lambda_{-}}{\hbar}t)\langle -,z|-,B'\rangle

where ##\langle-,z|+,B'\rangle = \langle -,z|-,B'\rangle = \frac{1}{\sqrt{2sec\theta(sec \theta + 1)}} tan \theta##

Separating real and imaginary parts:

\langle -,z|\psi_t\rangle = cos \left(\frac{\lambda_+}{\hbar}t\right)\langle-,z|+,B'\rangle\left(a+c\right) + i sin \left( \frac{\lambda_-}{\hbar}t \right)\langle-,z|+,B'\rangle (a-c)
= cos \left(\frac{\lambda_+}{\hbar}t\right)\langle-,z|+,B'\rangle\left(a+c\right) - i sin \left( \frac{\lambda_+}{\hbar}t \right)\langle-,z|+,B'\rangle (a-c)

Finally, the probability is:
|\langle -,z|\psi_t\rangle|^2 = \left(\langle-,z|+,B'\rangle\right)^2 \left[cos^2\left(\frac{\lambda_+}{\hbar}t\right)(a+c) + sin^2 \left(\frac{\lambda_+}{\hbar}t\right) (a-c)\right]

= \left(\langle-,z|+,B'\rangle\right)^2 \left[a + c*cos\left(\frac{2\lambda_+}{\hbar}t\right)\right]

= \left[\frac{sin^2\theta}{2(cos\theta+1)}\right]\left[\sqrt{\frac{1+cos\theta}{2}} - cos\left(\frac{2\lambda_+}{\hbar}t\right)\sqrt{\frac{1-cos\theta}{2}}\right]

This looks crazy, compared to the answer in part (b)i using perturbation theory.
 
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  • #12
unscientific said:
Yeah I got these two eigenstates:
551r2x.png

If you forget normalization for a moment, notice that ##|+,B'\rangle \sim \left(
\begin{array}{c}
1+\sec\theta\\
\tan\theta\\
\end{array}
\right)
\sim \left(
\begin{array}{c}
\cos\theta +1\\
\sin\theta\\
\end{array}
\right)
##

Use half-angle identities to express ##1+\cos\theta## and ##\sin\theta## in terms of ##\theta/2## and simplify.

At t = 0, the state of the particle is along z-axis, but we wish to express it in basis along net B field, B'.

|\psi_0\rangle = |+,z\rangle = a|+,B'\rangle + c|-,B'\rangle

This implies that ##a = \langle+,B'|+,z\rangle = \frac{1}{\sqrt{2sec\theta(sec \theta + 1)}}(1+sec\theta)## and ##c = \langle-,B'|+,z\rangle = \frac{1}{\sqrt{2sec\theta(sec\theta-1)}}(1-sec\theta)##



That's true, because these are basis kets in the z-direction, and not in direction of tan θ. I suppose the above method can only be used.

Following from above, the ket at time t is:
|\psi_t\rangle = a*exp(\frac{-i\lambda_{+}}{\hbar}t)|+,B'\rangle + c*exp(\frac{-i\lambda_{-}}{\hbar}t)|-,B'\rangle

Note that the eigenvalue ##\lambda_+## corresponds to the higher energy and therefore belongs to the spin state that is anti-parallel to B'. This is due to the overall negative sign in H.
 
  • #13
TSny said:
If you forget normalization for a moment, notice that ##|+,B'\rangle \sim \left(
\begin{array}{c}
1+\sec\theta\\
\tan\theta\\
\end{array}
\right)
\sim \left(
\begin{array}{c}
\cos\theta +1\\
\sin\theta\\
\end{array}
\right)
##

Use half-angle identities to express ##1+\cos\theta## and ##\sin\theta## in terms of ##\theta/2## and simplify.



Note that the eigenvalue ##\lambda_+## corresponds to the higher energy and therefore belongs to the spin state that is anti-parallel to B'. This is due to the overall negative sign in H.

Yeah it gets pretty messy, at this stage its hard to believe that it will all turn out to be a simple sin2θ function. I will definitely work it out later today or tomorrow. But for now, is this concept/method right?

1. Express initial state |+,z> in terms of basis along B'.
2. Each ket evolves with time given by exp(-iEt/h)
3. Overlap with <-,z| to find probability amplitude
 
  • #14
unscientific said:
But for now, is this concept/method right?

1. Express initial state |+,z> in terms of basis along B'.
2. Each ket evolves with time given by exp(-iEt/h)
3. Overlap with <-,z| to find probability amplitude

Yes. That will solve it.
 

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