States with minimum energy for electrons in mag field with nonzero Lz

vdweller
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Homework Statement



For an electron in a uniform magnetic field, say B\hat{z} with no angular momentum, the Hamiltonian can be expressed as \hat{H}=\frac{1}{2m}\Big(\hat{p}_x^2+\frac{mω^2}{2}\hat{x}^2\Big)+\frac{1}{2m}\Big(\hat{p}_y^2+\frac{mω^2}{2}\hat{y}^2\Big)

Which is equivalent to two separate harmonic oscillators.

Now the ground state is Ψ=Ne^{\frac{mω}{\hbar}r^2}

where r=\sqrt{x^2+y^2} and ω=ω_B/2=eB/2mc

which yields energy equal to \hbarω

Now there are other states with nonzero angular momentum L_z which yield the same energy. Those states are Ψ_n=Nr^ne^{inφ}e^{\frac{mω}{\hbar}r^2}

(n is not the quantum number)

The question is to prove that \hat{H}Ψ_n=\frac{\hbarω_B}{2}Ψ_n

since Ψ_n is also an eigenstate of the Hamiltonian.

My question is, how do we prove that? I tried using the Hamiltonian with polar coordinates but I can't seem to get to the result.

Is there any other way (using the creation/annihilation operators)?
 
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vdweller said:

Homework Statement



For an electron in a uniform magnetic field, say B\hat{z} with no angular momentum, the Hamiltonian can be expressed as \hat{H}=\frac{1}{2m}\Big(\hat{p}_x^2+\frac{mω^2}{2}\hat{x}^2\Big)+\frac{1}{2m}\Big(\hat{p}_y^2+\frac{mω^2}{2}\hat{y}^2\Big)

Which is equivalent to two separate harmonic oscillators.

Now the ground state is Ψ=Ne^{\frac{mω}{\hbar}r^2}

where r=\sqrt{x^2+y^2} and ω=ω_B/2=eB/2mc

which yields energy equal to \hbarω

Now there are other states with nonzero angular momentum L_z which yield the same energy. Those states are Ψ_n=Nr^ne^{inφ}e^{\frac{mω}{\hbar}r^2}

(n is not the quantum number)

The question is to prove that \hat{H}Ψ_n=\frac{\hbarω_B}{2}Ψ_n

since Ψ_n is also an eigenstate of the Hamiltonian.

My question is, how do we prove that? I tried using the Hamiltonian with polar coordinates but I can't seem to get to the result.

Is there any other way (using the creation/annihilation operators)?

Did you try simply staying in cartesian coordinates and applying the hamiltonian?
 
Yes, it's still a mess.

By the way, the correct ground state is Ψ=Ne^{-\frac{mω}{ℏ}r^2} (forgot a minus). I can't see the edit button any more...
 
vdweller said:
Yes, it's still a mess.

By the way, the correct ground state is Ψ=Ne^{-\frac{mω}{ℏ}r^2} (forgot a minus). I can't see the edit button any more...

Sorry, I did not notice your ## \phi## dependence on the one you must check.
Then you must use polar coordinates (you are working in two dimensions, right?).
You need ## \nabla^2 ## in polar coordinates. Once you reexpress the hamltonian in polar coordinates, it should be easy to check.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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