Time Evolution Of A 1-D Gaussian Wave Packet Under The Gravitational Potential

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Discussion Overview

The discussion revolves around the time evolution of a Gaussian wave packet in the context of quantum mechanics, specifically under a gravitational potential. Participants explore the implications of time translation invariance and the appropriate propagator to use for evolving the wave function over time.

Discussion Character

  • Exploratory, Technical explanation, Conceptual clarification, Debate/contested

Main Points Raised

  • One participant questions how to time evolve a Gaussian wave packet under a gravitational potential, noting a lack of time translation invariance.
  • Another participant suggests that without time translation invariance, a conserved Hamiltonian cannot be established, and mentions that the gravitational potential can be modeled as a linear potential related to the Airy function.
  • A participant expresses uncertainty about whether they can simply substitute (t - t') for t in their calculations, indicating confusion about the implications of time translation invariance.
  • It is proposed that to solve for time evolution, one must compute the propagator and find the energy eigenfunctions from the time-independent Schrödinger equation.
  • Clarification is provided that the energy eigenfunctions are related to the Airy function, and boundary conditions will determine the allowed energy values.
  • One participant acknowledges the guidance received and expresses intent to pursue the suggested approach.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the method for time evolution, with some asserting the necessity of solving the time-independent Schrödinger equation while others express uncertainty about the substitution of variables.

Contextual Notes

Participants reference specific equations and concepts from a paper, indicating that the discussion is grounded in particular theoretical frameworks and mathematical formulations. The implications of boundary conditions and the nature of the gravitational potential are also noted as critical to the discussion.

TheFinalThy
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Hello Colleagues,

I am curious about a problem in Quantum Mechanics that incorporates the evolution of a Gaussian Wave Packet under the Gravitational Potential.

What I am interested in is equation (3) in the following paper:
"On the quantum analogue of Galileo's leaning tower experiment"
(Unfortunately, I can not post a direct link due to forum restrictions...)

I have worked with Gaussian Packets representing a Free Particle before. In that case, I was able to time evolve the function trivially since I had time translation invariance on my side s.t. t ---> (t - t-initial) or (t - t_final).

However, with equation (3), I do not believe that I have time translation invariance. How, then, can I time evolve this function to some later or some earlier time? What Propagator would I use?

Thank you for any effort or time put into my question. If I can elaborate about what I am asking, please let me know.
 
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If there were no time translation invariance, we could not write down a conserved Hamiltonian. In this case, the gravitational potential is just modeled as a linear potential and the solutions to the time-independent Schrödinger equation, ##\phi_n(z)## are related to the Airy function, see http://www.physics.csbsju.edu/QM/fall.03.html for some concrete results.

The propagator can presumably be computed from the usual formula

$$ K(x',t';x,t) = \sum_n \phi_n^*(x')\phi_n(x) e^{-iE_n(t'-t)/\hbar} .$$

You will need to look up identities for the Airy function to perform the sum and later integrals. Things like the integral representation or representation in terms of Bessel functions would be useful.
 
So, you are saying that it is not as simple as plugging in (t - t') for my original "t" as in equation (3), as I suspected, correct? I think that this is the case, but I am not positive.

Then, assuming that my assumption about not having time translation invariance is correct, if I want to solve for a time before or after time "t" in the formula, I must first solve for the propagator and use that in the normal fashion to find my new function?

And, if this is true, then what will be my \phi_n(x)? Will it be equation (1) in "On the quantum analogue of Galileo's leaning tower experiment"?

Or, am I just making a mess of things and is it true that I could insert (t - t') in for "t"?
I am sorry for the confusion, but I fear that it is the case that I am quite puzzled about how this works.
 
No, you can't just substitute t-t' for t. You have to solve the time-independent Schrödinger equation to find the ##\phi_n(x)##. That link I gave explains how to do this. You leave the energy eigenvalue ##E## arbitrary and find that the solutions look like ##\mathrm{Ai}(x-E)##. (I am leaving various details out.) Applying the boundary conditions fixes the allowed values of ##E## in terms of the zeros of this function. Once you have the energy eigenfunctions and eigenvalues, you can use the standard formula for the propagator.

Now this is the most straightforward method. There may be a simpler way to find the answer by using the symmetry of the Schrödinger equation: ##x\rightarrow x + a, E\rightarrow E - mga##.
 
Ah, indeed. Thank you for your help! I shall try this.
 

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