TD perturbation - state initially in continuous part

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Discussion Overview

The discussion revolves around time-dependent perturbation theory, specifically addressing the scenario where an electron is initially prepared in a state of the continuous part of the energy spectrum. Participants explore the implications of this setup, particularly focusing on the normalization and definition of coefficients associated with the wave functions in this context.

Discussion Character

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

Main Points Raised

  • One participant presents the perturbed wave function as a superposition of unperturbed wave functions, questioning the definition of coefficients when the electron is in a continuous state.
  • Another participant corrects the interpretation of probability density, suggesting that the product |a_{E_0}(t)|^2dE represents the probability of the electron having energy in an infinitesimal shell around E_0.
  • Concerns are raised about the validity of using |a_{E_0}(t)|^2 as a delta function, with some arguing that the squared modulus should be a number, not a delta function.
  • Participants discuss the implications of using delta functions in the context of energy eigenstates versus position or momentum eigenstates.
  • There is a suggestion that the electron cannot be in an unnormalizable state, prompting further inquiry into the implications of this for the initial conditions of the electron.
  • Some participants express confusion over the dimensionality of coefficients and the normalization of wave functions, leading to a deeper exploration of the mathematical framework involved.

Areas of Agreement / Disagreement

Participants express differing views on the interpretation of coefficients in the context of continuous energy states, particularly regarding the use of delta functions and normalization. There is no consensus on the correct approach or interpretation, and the discussion remains unresolved.

Contextual Notes

Participants highlight potential misunderstandings regarding the mathematical treatment of wave functions and the implications of using delta functions in quantum mechanics. The discussion reveals uncertainties about the definitions and properties of the involved mathematical entities.

Who May Find This Useful

This discussion may be of interest to those studying quantum mechanics, particularly in the context of perturbation theory and the treatment of continuous energy spectra.

Nemanja989
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Hi everyone,

I am doing a time dependent perturbation theory, in a case when the electron is prepared in a state of the continuous part of the energy spectrum. Existence of the discrete part and the degeneracy of the continuous part is irrelevant at the moment and will not be considered.

First, the perturbed wave function is given as a superposition of the unperturbed wave functions:

\Psi(t) = \int a_E(t) \Psi_E dE
where \Psi_E=\psi_E e^{-i\omega_Et} and the integral is done over the whole spectrum of energies. The unperturbed wave functions are normalized to the Dirac delta with energy as an argument: \int \Psi_{E_i}^*\Psi_{E_j}dx=\delta(E_i-E_j) and have units of \frac{1}{\sqrt{m⋅J}}, while the perturbated wave function has the units of \frac{1}{\sqrt{m}}. The unit of a_E(t) is \frac{1}{\sqrt{J}}, while the product |a_{E_0}(t)|^2dE is the probability that the electron has the energy E_0 at the time t, which implies \int|a_{E_0}(t)|^2dE=1. For more details one can look in the Landau Lifshitz course - https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n29/mode/2up, introductory chapter about operators.

Now comes the issue:

If the electron is initially in the state with the energy E_0 , then it has to be that |a_{E_0}(t)|^2=\delta(E-E_0), while it also holds that a_{E_0}=\int \Psi_{E_0}^*\Psi dx. My question is, if one can write any expression for the value of a_{E_0} only? The problem for me is that the \sqrt{\delta(E-E_0)} does not seem to be well defined.

This would be very important as it would be used in the first order of the perturbation theory.

In other case, when the electron is initially in a discrete state, this problem is rather trivial and that's why I think I am missing something obvious here.

Thanks for your help!
 
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I think there are a few things off in your notation (either because of conceptual reasons or a typographic mistake). I will correct a few things to what I believe should be there to avoid confusion--correct me if you don't agree.
Nemanja989 said:
Hi everyone,
while the product |a_{E_0}(t)|^2dE is the probability that the electron has the energy E_0 at the time t, which implies \int|a_{E_0}(t)|^2dE=1.
The product |a_{E_0}(t)|^2dE is the probability that the electron has an energy in an infinitesimal shell around E_0 with size ##dE## at the time t, which implies \int|a_{E}(t)|^2dE=1.

If the electron is initially in the state with the energy E_0 , then it has to be that |a_{E_0}(t)|^2=\delta(E-E_0),
I would rather say |a_{E}(0)|^2=\delta(E-E_0)
----------------------------------------------------------------------------

I am not sure what you are really after. But if it is only the initial state you are interested in, global phase can be chosen arbitrarily.
 
Thanks for the corrections! You are absolutely right about both of them :) I was not rigorous enough, although meant the same as you.

As you pointed, there is no problem with the phase. The problem that I have is that in the later calculations I will have to use a_E(0) instead of |a_E(0)|^2, and a_E(0)=\sqrt{\delta(E-E_0)} is not well defined.

E.g. How would one calculate the following:

\int a_E(0)\Psi_E dE=\int\sqrt{\delta(E-E_0)}\Psi_E dE \quad ?

I have a feeling that having a square root should not have extremely big influence, but I do not have a knowledge of a mathematician of distributions, and therefore it is a puzzle for me..
 
Nemanja989 said:
If the electron is initially in the state with the energy ##E_0## , then it has to be that ##|a_{E_0}(t)|^2 = \delta(E - E_0)##

This doesn't make sense. The squared modulus of the wave function is a number, not a delta function.

Also, an energy eigenstate is not described by a delta function like ##\delta(E - E_0)## with energy as an argument; that only works for a position eigenstate like ##\delta(x - x_0)## (in the position representation) or a momentum eigenstate like ##\delta(p - p_0)## (in the momentum representation). I suspect you are misunderstanding something in whatever source you are using; what source (textbook or paper) are you trying to learn time-dependent perturbation theory from?

Nemanja989 said:
while it also holds that ##a_{E_0}=\int \Psi_{E_0}^*\Psi dx##.

I don't know what you mean by this.
 
thephystudent said:
I would rather say |aE(0)|2=δ(E−E0)

This doesn't make sense; the squared modulus is a number, not a delta function. See my response to the OP just now.
 
The electron cannot be initially in an unnormalizable state.
 
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PeterDonis said:
This doesn't make sense; the squared modulus is a number, not a delta function. See my response to the OP just now.
Both on the left and the right hand side is a function of ##E##.

Also, ##\delta(E-E_0)## is sometimes used to define a microcanonical ensemble in quantum statistical mechanics. I think one usually doesn't take the continuum limit all the way though, but assumes a very dense discrete spectrum and thinks of the delta function as having a small width compared to all relevant energy scales, but still finite such that a sufficient amount of eigenstates is captured. If you explicitly won't allow for degeneracies, I don't see any problem with using the delta function for an individual energy eigenstate.
 
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For the simplicity and trying to avoid a chaos or confusion let's go one by one:

PeterDonis said:
This doesn't make sense. The squared modulus of the wave function is a number, not a delta function.

Any physical quantity f, characterized with the operator \hat{f} has eigenvalues f and eigenfunction \Psi_f . Let's assume it can take continuous values. Then we can represent any wave function \Psi as \Psi=\int a_f \Psi_f df. Now, \Psi_f is normalized in such a way that the product |a_f|^2 df is a probability for f to have a value in between f and f+df.

Here I tried to clarify the idea of what I have written beforehand. Can you now explain how can |a_f|^2 be a number, when it is not a dimensionless quantity?

Second, concerning the normalization of a wave function, it can be shown that, again for any quantity f it holds:

a_f=\int a_{f_0}× \int \Psi_{f_0}*\Psi_f^*dx df_0

This is true if and only if
\int \Psi_{f_0}*\Psi_f^* dx=\delta(f_0-f)

Could you please explain me your point again? This works for any quantity, we can simply use the case \hat{f}=\hat{H}, and everything holds just for energy instead of a generic quantity f.
 
A. Neumaier said:
The electron cannot be initially in an unnormalizable state.

Thank for the answer. But could you please explain this in greater detail? I could think of an electron starting in a discrete state and later being excited into one of the states of the continuous spectrum. The time after the excitation would be something I consider.
 
  • #10
thephystudent said:
Both on the left and the right hand side is a function of ##E##.

Meaning that ##a_E## is actually a function of ##E##?

Nemanja989 said:
Can you now explain how can ##|a_f|^2## be a number, when it is not a dimensionless quantity?

Lots of numbers in physics are not dimensionless. My weight is a number, but it's not a dimensionless quantity.
 
  • #11
PeterDonis said:
This doesn't make sense. The squared modulus of the wave function is a number, not a delta function.

Also, an energy eigenstate is not described by a delta function like ##\delta(E - E_0)## with energy as an argument; that only works for a position eigenstate like ##\delta(x - x_0)## (in the position representation) or a momentum eigenstate like ##\delta(p - p_0)## (in the momentum representation). I suspect you are misunderstanding something in whatever source you are using; what source (textbook or paper) are you trying to learn time-dependent perturbation theory from?
I don't know what you mean by this.
PS are you aware of how the delta function is changed if its argument is a function of another quantity?
 
  • #12
PeterDonis said:
Meaning that ##a_E## is actually a function of ##E##?

Yes. up to some trivial isomorphism at least if you insist to be a purist.
 
  • #13
Nemanja989 said:
are you aware of how the delta function is changed if its argument is a function of another quantity?

Yes, my issue is not with the use of delta functions.
 
  • #14
PeterDonis said:
Yes, my issue is not with the use of delta functions.
Ok, may I ask you for your opinion on how would you describe a_E(0), if you know that
\int |a_E(0)|^2dE=1

and for all E except E=E_0, a_E(0)=0?

PS Can you answer the second question in my post #8?
 
  • #15
Nemanja989 said:
may I ask you for your opinion on how would you describe ##a_E(0)##,

I wouldn't. The only thing that I would say has a well-defined physical meaning is any integral in which ##|a_E|^2## and ##dE## appear in the integrand. The normalization integral you give is an example of such an integral (but of course not the only possible one). But the integral having a well-defined meaning does not require that ##a_E## itself have a well-defined meaning.
 
  • #16
PeterDonis said:
I wouldn't.

But still, having on one side a delta function with properties that

\int\delta(x-x')dx=1 and \delta(x)=0 for x\neq x'

and on the other

\int|a_E|^2dE=1 and |a_E|^2=0 for E\neq E'

doesn't tell you that |a_E|^2=\delta(E-E')?

And again, can you answer the second question in my post #8, concerning the normalization of a wave function in the continuous spectrum? What I am doing there is to take any operator \hat{f}, find its eigenfunctions \Psi_f and normalize these eigenfunction as \int\Psi_{f'}^*\Psi_{f}dx=\delta(f-f'). I think that this is perfectly valid and good for any operator and so as for \hat{H}.
 
  • #17
Nemanja989 said:
And again, can you answer the second question in my post #8, concerning the normalization of a wave function in the continuous spectrum? What I am doing there is to take any operator \hat{f}, find its eigenfunctions \Psi_f and normalize these eigenfunction as \int\Psi_{f'}^*\Psi_{f}dx=\delta(f-f'). I think that this is perfectly valid and good for any operator and so as for \hat{H}.
No, it is not. Operators are defined on the Hilbert space and if and operators do not have eigenstates corresponding to values in their continuous spectrum in this space. You can extend the analysis to rigged Hilbert spaces, where these eigenvectors can be defined, but still, this normalisation condition will not arise.
 
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  • #18
DrDu said:
No, it is not. Operators are defined on the Hilbert space and if and operators do not have eigenstates corresponding to values in their continuous spectrum in this space. You can extend the analysis to rigged Hilbert spaces, where these eigenvectors can be defined, but still, this normalisation condition will not arise.

Thanks. For my own clarifications may I ask you the following:

On the https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n29/mode/2up, equation (5.4) states what I have written in my previous post. It is either that I misunderstood something there or that the statement in that link is wrong?

(PS I have no problem when pointed of being wrong, to me it is a way of progressing and understanding the subject better and better.)
 
  • #19
Nemanja989 said:
Thank for the answer. But could you please explain this in greater detail? I could think of an electron starting in a discrete state and later being excited into one of the states of the continuous spectrum. The time after the excitation would be something I consider.
An electron starting in a discrete eigenstate would evolve into a weighted integral over continuum eigenstates. Then the problems with the delta function disappear.
 
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  • #20
Nemanja989 said:
Thanks. For my own clarifications may I ask you the following:

On the https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n29/mode/2up, equation (5.4) states what I have written in my previous post. It is either that I misunderstood something there or that the statement in that link is wrong?

(PS I have no problem when pointed of being wrong, to me it is a way of progressing and understanding the subject better and better.)

Also, on https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n75/mode/2up Landau and Lifshitz discuss in detail on how to change the normalization condition from momentum to energy. I really think there is not much to be misunderstood there, but still it's either that or that the problem is in communication between us or in the end that the book is not right.
 
  • #21
A. Neumaier said:
An electron starting in a discrete eigenstate would evolve into a weighted integral over continuum eigenstates. Then the problems with the delta function disappear.

I can be very well wrong, but from a purely theoretical point of view, why cannot the transition happen to a single state in the continuous spectrum? In that case the weight within the integral is still a density of states in respect to energy, just given as a delta function. This is used again in the Landau Lifshitz book https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n159/mode/2up, when going from eq. (42.5) to (42.6).
 
  • #22
Nemanja989 said:
I can be very well wrong, but from a purely theoretical point of view, why cannot the transition happen to a single state in the continuous spectrum? In that case the weight within the integral is still a density of states in respect to energy, just given as a delta function. This is used again in the Landau Lifshitz book https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n159/mode/2up, when going from eq. (42.5) to (42.6).
Because single continuum states are not normalizable. Ignoring this is the cause of all your problems
 
  • #23
A. Neumaier said:
Because single continuum states are not normalizable. Ignoring this is the cause of all your problems
Sorry for looking as if I am stubborn, but I simply want to clarify things for myself.

The fact that it is not possible to induce a transition to the single state of the continuous spectrum is in the direct contradiction with, I quote from the LL book:

"If the energy levels of the continuous spectrum are not degenerate, so that \nu can be taken as the value of the energy alone, then the whole "interval" of states dE reduces to a single state with energy E=E^{(0)}_N+\hbar\omega and the probability of a transition to this state is ... "

To me, they clearly say that the transition from a discrete state to a single state of a continuous spectrum is very possible. Could you please explain me the cause of the contradiction? Thanks.
 
  • #24
Nemanja989 said:
Sorry for looking as if I am stubborn, but I simply want to clarify things for myself.

The fact that it is not possible to induce a transition to the single state of the continuous spectrum is in the direct contradiction with, I quote from the LL book:

"If the energy levels of the continuous spectrum are not degenerate, so that \nu can be taken as the value of the energy alone, then the whole "interval" of states dE reduces to a single state with energy E=E^{(0)}_N+\hbar\omega and the probability of a transition to this state is ... "

To me, they clearly say that the transition from a discrete state to a single state of a continuous spectrum is very possible. Could you please explain me the cause of the contradiction? Thanks.
They call the probability density probability,. But there is zeeo probability of making such a transition. The continuum behaves quite different from the discrete part. To get a positive probability one needs to integrate over a whole interval of states.
 
  • #25
A. Neumaier said:
They call the probability density probability,. But there is zeeo probability of making such a transition. The continuum behaves quite different from the discrete part. To get a positive probability one needs to integrate over a whole interval of states.
No, they do not call the probability density as probability. What they did change is calling the rate of probability as probability.

Here it goes:

|a_{fi}|^2=(2\pi/\hbar)|F_{fi}|^2\delta(E_f-E^{0}_i-\hbar\omega)t

and then they say |a_{fi}|^2 d\nu_f is the probability of a transition from the original state to one in the interval d\nu_f, where in case of no degeneracy d\nu_f=dE. |a_{fi}|^2 d\nu_f is in absolute consistency with the interpretation they gave in the earlier chapters, being the probability for something to happen, not probability density or anything similar. Now one can get the rate of the probability ("the probability of the transition per unit time") as following:

dw_{fi}=(2\pi/\hbar)|F_{fi}|^2\delta(E_f-E^{0}_i-\hbar\omega)dE

and they integrate with respect to energy and obtain the rate of probability for a transition from a single discrete state to a single state of the continuous spectrum:

w_{Ei}=(2\pi/\hbar)|F_{Ei}|^2

So I think they did not make a mistake in labeling it as a probability density.
 
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  • #26
Since you seem to know it better why do you ask?
 
  • #27
Because of your statement earlier. You said something that I found contradicting some other fact. Further, you said that very thing will solve all of my problems.

I am not playing any game, but honestly trying to understand something. I get your last comment as a bit sarcastic, but I still want to ask you if you agree with my previous post or not, and why if possible?
 
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  • #28
Nemanja989 said:
Also, on https://archive.org/stream/QuantumMechanics_104/LandauLifshitz-QuantumMechanics#page/n75/mode/2up Landau and Lifshitz discuss in detail on how to change the normalization condition from momentum to energy. I really think there is not much to be misunderstood there, but still it's either that or that the problem is in communication between us or in the end that the book is not right.

And I would really like to hear a critical opinion of the others on the method that Landau and Lifshitz used for normalizing a continuous state, as this is something as far as I understood they were strongly opposing.

(In the end for me, this forum serves as a place for a constructive discussion, where if possible the problems get solved and confusion one may have goes away)
 
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  • #29
Nemanja989 said:
doesn't tell you that ##|a_E|^2=\delta(E-E')##?

You didn't ask about##|a_E|^2##, you asked about ##a_E##. The whole issue you have been struggling with is that you don't know how to take the square root of a delta function. The correct answer to that problem is "don't do that". You don't need to.
 
  • #30
Nemanja989 said:
if you agree with my previous post or not
Not at all. You simply dismiss my explanations, making me feel having wasted my time.

Any S-matrix is unitary hence preserves norms. Thus it cannot turn a discrete eigenstate (of norm 1) into a continuous one (of norm infinity). Thus there are no such transitions. The language in L/L is to be understood cum grano salis.

Nemanja989 said:
they did not make a mistake in labeling it as a probability density.
This is not a mistake but a widely used convention. Probabilities cannot have delta-functions as values, hence whenever you see such a ''probability'' you should conclude that a probability density is meant.

Take your time to see how both what L/L write and what I wrote makes sense.
 
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