How to Calculate Energy Corrections using Perturbation Theory

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Discussion Overview

The discussion revolves around calculating energy corrections using perturbation theory in the context of a harmonic oscillator with a specific perturbation. Participants explore the implications of the perturbation, its physical meaning, and the resulting energy corrections, including first and second order corrections.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants question the physical interpretation of the perturbation \(\hat{H}' = \alpha\hat{p}\) and its implications for the harmonic oscillator.
  • One participant calculates the first order energy correction as 0 and the second order correction as \(E_n^2 = m\alpha^2/2\), expressing skepticism about the independence of this result from the quantum number \(n\).
  • Another participant mentions the possibility of solving the problem analytically and shares numerical results from Matlab that align with the perturbation theory outcomes.
  • Hints are provided regarding the classical Hamiltonian of a particle in an electromagnetic field and the implications of completing the square in the context of the Hamiltonian.
  • Some participants discuss the relationship between perturbation theory and classical results, suggesting that perturbation theory yields exact results in specific cases.
  • There is a discussion about the expectation values of angular momentum operators \(L_x\) and \(L_y\) in a mixed state, raising questions about symmetry and directionality in quantum mechanics.
  • Participants engage in a dialogue about the effects of applying rotations to quantum states and the implications for expectation values.

Areas of Agreement / Disagreement

Participants express differing views on the physical interpretation of the perturbation and the implications of the energy corrections. While some agree on the results obtained from perturbation theory, others remain uncertain about the independence of energy corrections from quantum states and the implications of symmetry in quantum mechanics.

Contextual Notes

There are unresolved questions regarding the physical meaning of the perturbation and the assumptions underlying the calculations. Participants also note the dependence on the definitions and mathematical steps involved in the perturbation theory.

broegger
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Hi,

I'm new to this subject, so bear with me. We consider the harmonic oscillator with a pertubation:

[tex]\hat{H}' = \alpha\hat{p}.[/tex]​

(What kind of a perturbation is that anyway, it's not a disturbance in the potential, what does it correspond to physically.)

Now I have to calculate the first and second order energy corrections. I express p by the ladder operators:

[tex]p=i\sqrt{\tfrac{\hslash m\omega}2}(a_+-a_-).[/tex]​

I find that the first order correction is 0, and that the second order correction is [tex]E_n^2=m\alpha^2/2[/tex], that is, the energy shift is INDEPENDENT of n (i.e. it is the same for all excited states of the oscillator), but this can't be true, can it?
 
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broegger said:
Hi,

I'm new to this subject, so bear with me. We consider the harmonic oscillator with a pertubation:

[tex]\hat{H}' = \alpha\hat{p}.[/tex]​

(What kind of a perturbation is that anyway, it's not a disturbance in the potential, what does it correspond to physically.)

Now I have to calculate the first and second order energy corrections. I express p by the ladder operators:

[tex]p=i\sqrt{\tfrac{\hslash m\omega}2}(a_+-a_-).[/tex]​

I find that the first order correction is 0, and that the second order correction is [tex]E_n^2=m\alpha^2/2[/tex], that is, the energy shift is INDEPENDENT of n (i.e. it is the same for all excited states of the oscillator), but this can't be true, can it?

Hint 1: H_harm= k1^2.p^2+k2^2.q^2
If you add this potential (alpha.p) what do you obtain?

Hint 2: what is the interaction of a spinless charged particle with a magnetic field?

Seratend.
 
Well, it could be solved analytically, but I don't know how. I'm not particularly familiar with solving such differential equations. I've tried solving it numerically in Matlab, and this confirms my result, but it's not quite satisfying.

I don't know much about magnetic interactions in QM, haven't touched the subject in our intro course, unfortunately.
 
broegger said:
Well, it could be solved analytically, but I don't know how. I'm not particularly familiar with solving such differential equations. I've tried solving it numerically in Matlab, and this confirms my result, but it's not quite satisfying.

I don't know much about magnetic interactions in QM, haven't touched the subject in our intro course, unfortunately.

Hint 3: a^2+ka= (a+k/2)^2 - k^2

Hint 4: do you known the classical hamiltonian of a particle with an electromagnetic field?

Seratend.
 
I've tried completing the square, but I don't know how to go on.

The energy of a classical particle in an electromagnetic field is just the sum of the energy associated with the electric and magnetic field, respectively, right?

[tex]E = \frac{q_1q_2}{4\pi\epsilon_0r^2}-\mu\cdot B[/tex]​
 
broegger said:
I've tried completing the square, but I don't know how to go on.

The energy of a classical particle in an electromagnetic field is just the sum of the energy associated with the electric and magnetic field, respectively, right?

[tex]E = \frac{q_1q_2}{4\pi\epsilon_0r^2}-\mu\cdot B[/tex]​

Ok,

First, Let't take the harmonic oscillator hamiltonian:
H= p^2+k.q^2
You know the solutions of such an hamiltonian. Therefore I suppose you know the solution of H'=(p+a)^2+k.q^2, don't you?

(k>0, I have choosen the units to got simple equations, you are free to choose your own units)

If I had the interaction hamiltonian, I get:

choosing alpha= 2a

H=p^2+k.q^2+2a.p= (p+a)^2 + k.q^2 -a^2

We just recover another harmonic oscillator with p'=p+a:
[p,q]=[p+a,q]=-ihbar.

The constant -a^2 does not change the spectrum (when you write the hamiltonian it is defined up to a constant).
Or if you prefer a more mathematical way:
the commutator [p'^2 + k.q^2 -a^2, p'^2 + k.q^2]=0 => we have the same eigenvalues. Or just solve the equation with an additional constant (not very difficult)

Second: Classical hamiltonian: H= (P - qA)^2/2m + eV. Where A and V are the electromagnetic field potentials.
Now, develop the square and assume A^2 is very very small, what do you obtain?

Seratend.

Edit: correction of minor typo errors + others : )
 
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I don't know if I'm doing it right, but I get the same result as perturbation theory - E = (n+1/2)hw - ma^2/2 - (that's a good sign, isn't it :)), so perturbation theory yields the exact result in this case?
 
broegger said:
I don't know if I'm doing it right, but I get the same result as perturbation theory - E = (n+1/2)hw - ma^2/2 - (that's a good sign, isn't it :)), so perturbation theory yields the exact result in this case?

For the sign, I think it's ok.
bravo!

Seratend
 
Weeh, thanks for helping!
 
  • #10
Additionnal question for you: why does the pertubation theory give the same result in this case?

Seratend.
 
  • #11
Hmm, I think it's because we were able to factor the Hamiltonian perfectly, but I don't know, I was wondering the same thing...

I also have a quick question for you (I asked this in a another thread, but I'm still thinking about it). Suppose you have a hydrogen electron in the mixed state:
[tex]|\psi\rangle=\frac1{\sqrt2}(|210\rangle + |211\rangle)[/tex]​
(|nlm> denotes an eigenstate of H, L^2 and L_z - n is the main quantum number and l and m is the quantum numbers associated with L^2 and L_z, respectively).

Now, I find that L_x and L_y has different expectation values (h/sqrt(2) and 0, respectively), but how can this be, when there is nothing to distinguish the x- and y-directions in this case??
 
  • #12
broegger said:
Now, I find that L_x and L_y has different expectation values (h/sqrt(2) and 0, respectively), but how can this be, when there is nothing to distinguish the x- and y-directions in this case??

Apply a rotation (z axis) to the state, does it change?

Seratend.
 
  • #13
broegger said:
Hmm, I think it's because we were able to factor the Hamiltonian perfectly, but I don't know, I was wondering the same thing...

Think on the functions: f(x) and f(x+h)~f(x)+hf'(x). When do you have the equality?
Think now on the expansion of the hamiltonian, with the pertubation theory. It just allows more possibilities.


Seratend.

EDIT change = into ~to avoid confusion : )
 
  • #14
No, I don't think so. It's symmetric with respect to x and y, that's the problem. I might be wrong, though :)
 
  • #15
broegger said:
No, I don't think so. It's symmetric with respect to x and y, that's the problem. I might be wrong, though :)

I am not sure, but you should try to work a little : )

here is the rotation matrix for an angle phi:
Code:
(exp(-i.phi/2) 		0) 	
(0		exp(iphi/2))
Do you keep saying the state does not change?

Seratend.

EDIT: corrected a missing i in the roation matrix. : )
 
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  • #16
seratend said:
I am not sure, but you should try to work a little : )
Hehe, you're right, I should...

seratend said:
here is the rotation matrix for an angle phi:
(exp(-i.phi/2) 0)
(0 exp(iphi/2))
Do you keep saying the state does not change?
Well no, I just thought "geometrically", you know :) I'll try working it out from the start again...
 
  • #17
broegger said:
Hehe, you're right, I should...
Well no, I just thought "geometrically", you know :) I'll try working it out from the start again...

Good. Progression in the knowledge requires somtimes some efforts : )

Seratend.
 

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