Path integral in momentum representation

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Discussion Overview

The discussion revolves around the derivation of the Schrödinger equation in momentum representation from a path integral perspective. Participants explore the differences in behavior of the action when fixing points in spatial versus momentum space, and the implications for the formulation of quantum mechanics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants question whether the expression Ψ(x_f, t_f) = e^{iS/\hbar}Ψ(x_i, t_i) is equivalent to the time-dependent Schrödinger equation (TDSE), suggesting that a different formulation involving an integral might be more appropriate.
  • There is a discussion about the calculation of the action in momentum space, with some participants noting that the classical Hamilton function is defined over position space, raising questions about how to compute the action given momentum endpoints.
  • One participant proposes that in momentum space, linear paths between momentum points should be considered, similar to the approach in position space, and provides a specific formulation for the action.
  • Another participant points out that applying the Euler-Lagrange equations in the context of momentum does not yield the expected results, indicating a potential misunderstanding of the interchangeability of position and momentum in Lagrangian mechanics.
  • Some participants express intrigue about the canonical approach and the role of generating functions in transforming between position and momentum representations.
  • There is a reference to Feynman's work on path integrals, with one participant suggesting that it provides insights into the derivation of the Schrödinger equation in momentum space.

Areas of Agreement / Disagreement

Participants express differing views on the equivalence of certain formulations and the appropriate methods for deriving the Schrödinger equation in momentum representation. The discussion remains unresolved, with multiple competing perspectives presented.

Contextual Notes

Some participants note limitations in their understanding of the action principle and its application in different representations, as well as the need for clarity regarding the definitions of position and momentum in the context of the Lagrangian and Hamiltonian frameworks.

jostpuur
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Is it possible to derive the Shrodinger's equation

[tex] i\hbar\partial_t \Psi(t,p) = \frac{|p|^2}{2m}\Psi(t,p)[/tex]

in momentum representation directly from a path integral?

If I first fix two points [itex]x_1[/itex] and [itex]x_2[/itex] in spatial space, solve the action for a particle to propagate between these point in time [itex]\Delta t[/itex], and then take the limit [itex]\Delta t\to 0[/itex], the action approaches infinity.

If I instead fix two points [itex]p_1[/itex] and [itex]p_2[/itex] in the momentum space, solve the action for a particle to propagate between these points in time [itex]\Delta t[/itex], and then take the limit [itex]\Delta t\to 0[/itex], the action does not approach infinity, but instead zero. So it looks like stuff goes somehow differently here.
 
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first of all, do you agree that

[tex]\Psi(x_f, t_f) = e^{\frac{iSt}{\hbar}}\Psi(x_i, t_i)[/tex]

is equivalent to the TDSE? all you need to do is take the time derivative and know from classical mechanics that [tex]E_f = \frac{\partial S}{\partial t_f}[/tex]
 
quetzalcoatl9 said:
first of all, do you agree that

[tex]\Psi(x_f, t_f) = e^{\frac{iSt}{\hbar}}\Psi(x_i, t_i)[/tex]

is equivalent to the TDSE? all you need to do is take the time derivative and know from classical mechanics that [tex]E_f = \frac{\partial S}{\partial t_f}[/tex]

Not really, unless there is a misunderstanding with the notation. Wouldn't

[tex] \Psi(x_f,t_f) = N\int dx_i\; e^{iS/\hbar} \Psi(x_i,t_i) + O((t_f-t_i)^2)[/tex]

be better?
 
jostpuur said:
Not really, unless there is a misunderstanding with the notation. Wouldn't

[tex] \Psi(x_f,t_f) = N\int dx_i\; e^{iS/\hbar} \Psi(x_i,t_i) + O((t_f-t_i)^2)[/tex]

be better?

sorry, its not [tex]e^{iSt/\hbar}[/tex] it should be [tex]e^{iS/\hbar}[/tex]
 
jostpuur said:
Not really, unless there is a misunderstanding with the notation. Wouldn't

[tex] \Psi(x_f,t_f) = N\int dx_i\; e^{iS/\hbar} \Psi(x_i,t_i) + O((t_f-t_i)^2)[/tex]

be better?

why would you do that? what i originally had (minus the typo) was correct

also, btw, you could do the other way around via

[tex] Q = e^{-\beta \hat{H}}[/tex]

impose the trotter thm:

[tex] e^{A + B} = \lim_{P \rightarrow \infty} (e^{A/P} e^{B/P})^P[/tex]

to separate the kinetic and potential parts. then use the resolution of the identity to insert the complete position and momenta states. when you're done you will arrive at the path integral.

the P has the significance of being the Trotter ("bead") number, which we tune when doing numerical simulation via path integrals.
 
quetzalcoatl9 said:
first of all, do you agree that

[tex]\Psi(x_f, t_f) = e^{\frac{iSt}{\hbar}}\Psi(x_i, t_i)[/tex]

is equivalent to the TDSE? all you need to do is take the time derivative and know from classical mechanics that [tex]E_f = \frac{\partial S}{\partial t_f}[/tex]

What is [itex]x_i[/itex] on the right side?
 
quetzalcoatl9, the way you insist that the integral is not needed remainds me of an equation that was something like this (it could be I remember some details wrong, I'm not checking now)

[tex] \int dx_2\; N^2 e^{iS(x_3,x_2)/\hbar} e^{iS(x_2,x_1)/\hbar} = N e^{iS(x_3,x_1)/\hbar}[/tex]

where [itex]S(y,x)[/itex] means action to move from x to y. Could it be that you are confusing this equation with my OP? Otherwise, I cannot understand what's the idea behind your response.
 
The classical Hamilton function S is defined over two points in position space -- because the Lagrangian is defined over position and the first derivative of position, and not over momentum. How did you calculate the action given momentum of the end points?
 
genneth said:
The classical Hamilton function S is defined over two points in position space -- because the Lagrangian is defined over position and the first derivative of position, and not over momentum. How did you calculate the action given momentum of the end points?

I'm interested in the non-relativistic case now, so momentum and velocity are more or less the same thing now.

In position representation we can assume, that the particle travels from point [itex]x_1[/itex] to point [itex]x_2[/itex] linearly, that means like

[tex] x(t) = \frac{x_2(t-t_0) + x_1(t_0+\Delta t - t)}{\Delta t}.[/tex]

Now [itex]x(t_0) = x_1[/itex] and [itex]x(t_0+\Delta t)=x_2[/itex]. The Lagrange's function is now defined along this path, in fact it is constant, and the action is integral of the L in time.

Analogously, I thought that in momentum space we should consider linear paths between points [itex]p_1[/itex] and [itex]p_2[/itex]. So the velocity of the particle along this path is

[tex] v(t) = \frac{v_2(t-t_0) + v_1(t_0+\Delta t - t)}{\Delta t}.[/tex]

So the action is

[tex] \int\limits_{t_0}^{t_0+\Delta t} L(t)dt = \int\limits_{t_0}^{t_0+\Delta t} \frac{m}{2}\Big| \frac{v_2(t-t_0) + v_1(t_0+\Delta t-t)}{\Delta t}\Big|^2 dt.[/tex]

If I did it correctly, then it is

[tex] S=\frac{m\;\Delta t}{2}\Big(\frac{1}{3}|v_2-v_1|^2 - v_2\cdot(v_2-v_1) + |v_2|^2\Big).[/tex]

(Written so that [itex]v_1[/itex] dependece is in form of [itex]v_2-v_1[/itex] dependece.)
 
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  • #10
I presume you mean to define L to be p^2/2m, and consider it a function of p and [tex]\dot{p}[/tex]. Unfortunately, as you can see for yourself, applying Euler-Lagrange doesn't give the desired result, giving only that p=0.

Although it is true that in the canonical, i.e. Hamiltonian, approach one can interchange position and momenta freely, it is not true in the Lagrangian aka action approach. In the latter you must define what is position and what is momentum. You can try the following: the interchange of position and momenta in the Hamiltonian will require a generating function, which will be added to the Hamiltonian. You can then try converting that back into a Lagrangian, which will be different to what the naive way will be, and see if you can derive an action that way.

I'm sorry to sound pessimistic -- I'm actually very much intrigue by this.

Good luck!
 
  • #11
genneth said:
I presume you mean to define L to be p^2/2m, and consider it a function of p and [tex]\dot{p}[/tex]. Unfortunately, as you can see for yourself, applying Euler-Lagrange doesn't give the desired result, giving only that p=0.

Good point. I never noticed this before.

Although it is true that in the canonical, i.e. Hamiltonian, approach one can interchange position and momenta freely, it is not true in the Lagrangian aka action approach. In the latter you must define what is position and what is momentum. You can try the following: the interchange of position and momenta in the Hamiltonian will require a generating function, which will be added to the Hamiltonian. You can then try converting that back into a Lagrangian, which will be different to what the naive way will be, and see if you can derive an action that way.

What is this generating function you are talking about?

I'm sorry to sound pessimistic -- I'm actually very much intrigue by this.

Good luck!

I noticed the calculation wasn't working. That's why I posted this! But I was hoping that it could be made to work, and I'm in fact still hoping so. Something should give the Shrodinger's equation in momentum space out of the Lagrange's function. It's just not the same action principle. It should be replaced with something else.
 
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  • #12
The canonical approach is all about transforming things into a more useful coordinate. In fact, the Hamilton function S is exactly that: it specifies a transform where all the position and momenta are constant! That is why we say that it encodes all the dynamics -- it's reduced them to the simplest possible form. I strongly encourage you to learn this stuff: the standard text is Goldstein, Classical Mechanics.
 
  • #13
jostpuur said:
Is it possible to derive the Shrodinger's equation

[tex] i\hbar\partial_t \Psi(t,p) = \frac{|p|^2}{2m}\Psi(t,p)[/tex]

in momentum representation directly from a path integral?

Yeah it is. Learn from the master himself:

R. P. Feynman (and Hibbs), "Quantum Mechanics and Path Integrals".
 
  • #14
genneth said:
the Hamilton function S is exactly that: it specifies a transform where all the position and momenta are constant!

I thought I knew this stuff when I knew the Hamilton's function H and the action S.

olgranpappy said:
Yeah it is. Learn from the master himself:

R. P. Feynman (and Hibbs), "Quantum Mechanics and Path Integrals".

You wouldn't bother giving some hints on what he does? I'm probably not buying more books very soon.
 
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  • #15
jostpuur said:
quetzalcoatl9, the way you insist that the integral is not needed remainds me of an equation that was something like this (it could be I remember some details wrong, I'm not checking now)

[tex] \int dx_2\; N^2 e^{iS(x_3,x_2)/\hbar} e^{iS(x_2,x_1)/\hbar} = N e^{iS(x_3,x_1)/\hbar}[/tex]

where [itex]S(y,x)[/itex] means action to move from x to y. Could it be that you are confusing this equation with my OP? Otherwise, I cannot understand what's the idea behind your response.

what i wrote was the propagator acting on the initial wavefunction, it's a standard result from QM
 
  • #16
jostpuur said:
You wouldn't bother giving some hints on what he does? I'm probably not buying more books very soon.

it's just as well, you can't get it anymore for less than $300 (out of print long ago, plus it's a fantastic book that covers things still, for some reason, neglected in other texts)
 
  • #17
jostpuur said:
You wouldn't bother giving some hints on what he does? I'm probably not buying more books very soon.

It's in Feynman's paper: "Space time approach to non-relativistic quantum mechanics"

The paper is included in many books. probably the most useful of these books is:

"Selected papers on Quantum Electrodynamics" edited by Julian Schwinger, which is a
"must have" collection of historical papers and it goes for as cheap as $6 on Amazon.com :

https://www.amazon.com/dp/0486604446/?tag=pfamazon01-20The paper is also included in "Feynman's Thesis" a book recently brought to the market
by Laurie Brown, (who wrote papers together with Feynman). Feynman's thesis is on
the principle of least action in Quantum Mechanics:

https://www.amazon.com/dp/9812563806/?tag=pfamazon01-20Regards, Hans
 
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  • #18
quetzalcoatl9 said:
what i wrote was the propagator acting on the initial wavefunction, it's a standard result from QM

For two fixed points [itex]x_i[/itex] and [itex]x_f[/itex], [itex]\exp(\frac{i}{\hbar}S(\Delta t,x_f,x_i))[/itex] is a number. It is not an operator you can put on the left side of the initial wave function alone. You must integrate over the [itex]x_i[/itex] to get the amplitude [itex]\psi(t+\Delta t,x_f)[/itex].
 
  • #19
jostpuur said:
For two fixed points [itex]x_i[/itex] and [itex]x_f[/itex], [itex]\exp(\frac{i}{\hbar}S(\Delta t,x_f,x_i))[/itex] is a number. It is not an operator you can put on the left side of the initial wave function alone. You must integrate over the [itex]x_i[/itex] to get the amplitude [itex]\psi(t+\Delta t,x_f)[/itex].

S is the action associated with the path from i to f

[tex]\Psi_f = e^{\frac{i}{\hbar}S} \Psi_i[/tex]

[tex]\frac{\partial \Psi_f}{\partial t_f} = \frac{i}{\hbar} \frac{\partial S}{\partial t_f}e^{\frac{i}{\hbar}S} \Psi_i[/tex]

[tex]\frac{\partial \Psi_f}{\partial t_f} = \frac{i}{\hbar} \frac{\partial S}{\partial t_f} \Psi_f[/tex]

[tex]\frac{\partial S}{\partial t_f} = -E_f[/tex]

[tex]\frac{\partial \Psi_f}{\partial t_f} = -\frac{i}{\hbar} E_f \Psi_f[/tex]

[tex]i \hbar \frac{\partial \Psi_f}{\partial t_f} = E_f \Psi_f[/tex]
 
  • #20
quetzalcoatl9 said:
S is the action associated with the path from i to f

[tex]\Psi_f = e^{\frac{i}{\hbar}S} \Psi_i[/tex]

I was talking about action to go from location [itex]x_i[/itex] to location [itex]x_f[/itex], but you have an action to move from quantum mechanical state [itex]\Psi_i[/itex] to state [itex]\Psi_f[/itex]. How is this action defined?

If S is still a number, then [itex]\exp(iS/\hbar)[/itex] is also number, and I don't think that in general [itex]\Psi_i[/itex] and [itex]\Psi_f[/itex] are linearly dependent so that we can get the final state by multiplying the initial state with a number.
 
  • #21
solution?

Now when genneth made the remark that action principle is not even supposed to work the same way in the momentum representation, as it does in the position representation, I think that the answer to the question "how do you solve SE in momentum representation?" is nothing else but "move onto position representation, solve SE, and move back to momentum representation!" :biggrin: :rolleyes:

The result is this

[tex] \psi(t+\Delta t,p) = N\int\frac{d^3x\; d^3x'\; d^3p'}{(2\pi\hbar)^3} e^{iS(x,x')/\hbar} e^{i(p'\cdot x' - p\cdot x)/\hbar} \psi(t,p') + O(\Delta t^2).[/tex]

Edit: hmhm.. I made it sound funnier than it really was. That's not yet "solving SE". Anyway, something like that... "write down the time evolution in position representation".
 
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  • #22
jostpuur said:
If S is still a number, then [itex]\exp(iS/\hbar)[/itex] is also number, and I don't think that in general [itex]\Psi_i[/itex] and [itex]\Psi_f[/itex] are linearly dependent so that we can get the final state by multiplying the initial state with a number.

What our Aztec friend wrote is not correct, but neither is what you wrote; certainly, I may obtain the time-evolved state of an eigenstate of the Hamiltonian by simple "multiplication... with a number". I.e., by [tex]e^{-iE(t_2-t_1)}[/tex].

In general the Schrödinger equation is exactly equivalent to an integral equation:

[tex] \Psi(\vec x;t_f)=\int d^3 y K(\vec x,\vec y;t_f-t_i)\Psi(\vec y;t_i)[/tex]

where the integration is only over space and thus, as far as time is concerned, this is also in a sense just "multiplication... with a number"... of course, it is much more than that really, and is not at all simply the same as multiplying by e^{iS}. The other important thing to note is that the kernal (K) is homogeneous in time.

Anyways, now the whole problem of quantum mechanics is to calculate K... so what is K, exactly... it's something like:

[tex] K(x,y;t)=\int_x^y Dq e^{-iS[q]}[/tex]

where the paths q which I am integrating over have endpoints fixed at q(0)=x and q(t)=y.

Oh, another name for K is a "Green's function".

Cheers.
 
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  • #23
olgranpappy said:
W but neither is what you wrote; certainly, I may obtain the time-evolved state of an eigenstate of the Hamiltonian by simple "multiplication... with a number". I.e., by [tex]e^{-iE(t_2-t_1)}[/tex].

To be fully precise, I said that initial and final states are not linearly dependent in general. They may be linearly dependent in some special cases, though, which is not a contradiction.
 

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