Expectation of position and momentum at time t, pictures

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Homework Help Overview

The discussion revolves around calculating the expectation values of position and momentum for a charged particle in a uniform electric field using quantum mechanics, specifically within the Schrödinger picture. The problem involves the Hamiltonian of the system and the time evolution of the state vector.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants explore the use of the time evolution operator and the Hamiltonian to derive expectation values. There are discussions about the necessity of certain variables and equations, particularly regarding the time independence of operators in the Schrödinger picture. Questions arise about the commutation relations and how they affect the calculations.

Discussion Status

Participants are actively engaging with the problem, attempting to derive equations for the expectation values of position and momentum. Some have provided partial calculations and insights into the relationships between the variables, while others are questioning the assumptions and exploring different interpretations of the equations involved. There is no explicit consensus on the final approach yet.

Contextual Notes

Initial conditions for the expectation values are given as zero, and there is a focus on the implications of the Hamiltonian and the commutation relations in the context of the problem. Participants also note the need to solve coupled differential equations related to the expectation values.

ma18
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Homework Statement



Consider a particle, with mass m, charge q, moving in a uniform e-field with magnitude E and direction X_1.

The Hamiltonian is (where X, P, and X_1 are operators):
upload_2015-12-3_13-26-9.png


The initial expectation of position and momentum are <X(0)> = 0 and <P(0)>=0

Calculate the expectation of position and momentum oprator in the Schrödinger picture is X (t) = (X_1, X_2, X,3)

2. The attempt at a solution

I know the Hamiltonian and the initial condition. I am doing this in the Schrödinger picture, and that with the time evolution operator I can represent the ket as

|phi(t)> = U (t,0) |phi(0)>

Is H is time-independent? As P is squared and is the magnitude of the P? If so the time evolution operator can be represented as

U (t,0) = exp (-i*t*H/hbar)

Then

I can represent phi(t) in terms of those terms and phi(0) and proceed but I am not sure if that is correct.

I know that P = mv = m dx/dt so I think I can use the derivative of the expectation value of X when I get that, correct. According to the equation:

d/dt <O>_t = i/h <[H,O]>_t + <dO/dt>_t

but I have to find the expectation of the position first.

Any help would be much appreciated!
 
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ma18 said:
I can represent phi(t) in terms of those terms and phi(0) and proceed but I am not sure if that is correct.
You don't need to know φ(t).

ma18 said:
I know that P = mv = m dx/dt so I think I can use the derivative of the expectation value of X when I get that, correct.
That should not be necessary.

ma18 said:
d/dt <O>_t = i/h <[H,O]>_t + <dO/dt>_t
Start with that equation, and see what you get for P and X.
 
DrClaude said:
You don't need to know φ(t).That should not be necessary.Start with that equation, and see what you get for P and X.

Okay, plugging X into that equation (get rid of _t for legibility) I get

d/dt <X> = i/h <[H,X]> + <dX/dt>
= i/h <[(P^2/2m - E*q*X_1), X]>+<dX/dt>
= i/h (-E*q) <X,X1>+<dX/dt>

and I'm not sure where to go from here...
 
What if I just did:

U (t,0) = exp (-i*t*H/hbar)
= exp (-i*t*(P^2/2m - E*q*X_1)/hbar)

|phi (t)> = exp (-i*t*(P^2/2m - E*q*X_1)/hbar) |phi(0)>

<phi (t)|X|phi(t)> = <phi(0) exp (i*t*(P^2/2m - E*q*X_1/hbar) | X | exp (-i*t*(P^2/2m - E*q*X_1)/hbar) |phi(0)>

but I don't know where I would go next, could I just multiply it in? But they are operators.
 
ma18 said:
d/dt <X> = i/h <[H,X]> + <dX/dt>
= i/h <[(P^2/2m - E*q*X_1), X]>+<dX/dt>
= i/h (-E*q) <X,X1>+<dX/dt>
What is the commutator of X and P? What can you say about the time-dependence of an operator (not explicitly time dependent) in the Schrödinger picture?

ma18 said:
What if I just did:

U (t,0) = exp (-i*t*H/hbar)
= exp (-i*t*(P^2/2m - E*q*X_1)/hbar)

|phi (t)> = exp (-i*t*(P^2/2m - E*q*X_1)/hbar) |phi(0)>

<phi (t)|X|phi(t)> = <phi(0) exp (i*t*(P^2/2m - E*q*X_1/hbar) | X | exp (-i*t*(P^2/2m - E*q*X_1)/hbar) |phi(0)>

but I don't know where I would go next, could I just multiply it in? But they are operators.
You can't go anywhere with that. Note also that you do not know what |φ(0)>, only that <φ(0)|X|φ(0)> = <φ(0)|P|φ(0)> = 0.
 
I know that the commutator of x and p is i*hbar and that in the Schrödinger picture the operators are time independent
 
ma18 said:
I know that the commutator of x and p is i*hbar and that in the Schrödinger picture the operators are not time dependent. However here I have x_1 and p^2
X1 is only one of the spatial dimensions (if I understand correctly "X (t) = (X_1, X_2, X,3)"), and p2 is simply pp, so
$$
\begin{align*}
[p^2,x] &= p^2x-xp^2 \\&= ppx - xpp \\
&= ppx - xpp - pxp + pxp \\
&= ppx - pxp + pxp - xpp \\
&= p[p,x] + [p,x]p
\end{align*}
$$
 
DrClaude said:
X1 is only one of the spatial dimensions (if I understand correctly "X (t) = (X_1, X_2, X,3)"), and p2 is simply pp, so
$$
\begin{align*}
[p^2,x] &= p^2x-xp^2 \\&= ppx - xpp \\
&= ppx - xpp - pxp + pxp \\
&= ppx - pxp + pxp - xpp \\
&= p[p,x] + [p,x]p
\end{align*}
$$

Ah ok so then, assuming that the commutator of x and x_1 is 0 I would get:

d/dt <X> = i/h <[H,X]> + <dX/dt>
= i/h <[(P^2/2m - E*q*X_1), X]>+<dX/dt>
= i/h <[X*P^2/2m -X*P^2/2m]>+<dX/dt>
= i/(2mh) <[X,P^2]>+<dX/dt>
= i/(2mh) <2*i*h*p>+<dX/dt>
= i/(2mh)*(2*i*h) <p>+<dX/dt>
= -1/m<p> +<dX/dt>

==>
<p> = m (d/dt <X> - <dX/dt>)

But that still has a lot of unknows for a final answer as I have to find out <X> as well
 
If I did the same procedure for P then it would be d/dt <P> = i/h <[H,P]> + <dP/dt>
= i/h <[(P^2/2m - E*q*X_1), P]>+<dP/dt>
= i/h <[P*-E*q*X_1 -E*q*X_1*P]>+<dP/dt>
= i(-E*q)/h <[P,X_1]>+<dP/dt>
= i/(2mh) <i*h>+<dP/dt>

But then if [P,X_1] = ih then this doesn't really make sense...
 
  • #10
Sorry for butting in, just a short intervention to remind the OP that dX/dt = dp/dt = 0.
 
  • #11
blue_leaf77 said:
Sorry for butting in, just a short intervention to remind the OP that dX/dt = dp/dt = 0.

Ah, thank you.

So then

<p> = m (d/dt <X>)

and

d/dt <P>= i(-E*q)/h <[P,X_1]>

Is that the final answer?
The second portion of the question is to, with the same Hamiltonian, knowing that in the Heisenberg Picture , X_H = (X_1H,X_2H,X_3H), find the commutator

[X_aH (t), X_bH (0)]

where all the X are operators

I know that in the Heisenberg picture the operators evolve with time as U^+ (t,0) O U(t,0)
 
Last edited:
  • #12
So then for the Heisenberg picture, because e^(0) = 1 and thus for X_bH (0), U would equal 1. I would get (where U_d represents U dagger)

U_d X_aH U X_b - X_b U_d X_aH U

then I don't know what to do
 
  • #13
ma18 said:
Is that the final answer?
No, you still have to solve those two coupled differential equations.
 
  • #14
blue_leaf77 said:
No, you still have to solve those two coupled differential equations.
ah, okay. Plus I still need to find <[P,X_1]> right. Could you help me with that commutator?

Thanks
 
  • #15
ma18 said:
Plus I still need to find <[P,X_1]> right.
Is P actually a vector in your notation? Is it actually ##\mathbf{P} = P_1\hat{i} + P_2\hat{j} + P_3\hat{k}##?
 
  • #16
It doesn't specify but I would assume it is a vector
 
  • #17
In that case, it will be ##[P_1\hat{i} + P_2\hat{j} + P_3\hat{k},X_1] = [P_1,X_1]\hat{i} + [P_2,X_1]\hat{j} + [P_3,X_1]\hat{k}##. You know the value of each term, don't you?
 
  • #18
Yes so then it would just be [P,X_1] = ih ?

Then the equation would be, as I put in post 9

d/t <P> = = i/(2mh) <i*h>
 
  • #19
ma18 said:
Yes so then it would just be [P,X_1] = ih ?
Don't forget the unit vector, ##[P,X_1] = i\hbar\hat{i}##.
ma18 said:
d/t <P> = = i/(2mh) <i*h>
That equation will then disperse into three equations, each for the momentum components and it should be easily solvable.
 
  • #20
As ih is a constant wouldn't <ih> just be equal to ih since the exponentials of the U term would become 1 and the phi(0) would as well.

And then I could sub in the first equation to get the value for <x>?
 
  • #21
ma18 said:
As ih is a constant wouldn't <ih> just be equal to ih
Yes, it is.
The equation for ##\langle \mathbf{X} \rangle## in post #8 also contains three further equations for each components of the position, so you need all values of ##\langle P_i \rangle##'s.
 
  • #22
But the whole thing has been done with the whole X anyway and the only reason the X_1 is being used is because it is in the Hamiltonian so isn't it fine?

Then

d/dt <p> = Eq i_hat

<p> = Eq t i_hat + C

using the first equation then:

d/dt <x> = (Eq t i_hat + C)/m

<x> = t(Eq t i_hat + C)/m + C_1
 
  • #23
ma18 said:
<p> = Eq t i_hat + C
Find C from the initial conditions for ##\mathbf{P}##.
ma18 said:
<x> = t(Eq t i_hat + C)/m + C_1
Find C_1 from the initial conditions for ##\mathbf{X}##, also check again if any constant number is missing in the first term proportional to ##t^2##.
 
  • #24
From the initial conditions

<p(0)> = 0 = C = 0

<x(0) = 0 = C_1 = 0

so

<p> = Eqt i_hat

<x> = t (Eq t i_hat)/m = <p> *t/m
 
  • #25
ma18 said:
<x> = t (Eq t i_hat)/m
You did the integration wrong, ##d<\mathbf{X}>/dt = -<\mathbf{P}>/m = -1Eqt/m \hat{i}##. How do you integrate ##- Eqt/m## over ##t##?
 
  • #26
Ah of course, silly mistake

d/dt <x> = (Eq t i_hat + C)/m
<x> = (E q t^2 i_hat )/(2m) + C_1

and then C_1 is zero from the IC so

<x> = (E q t^2 i_hat )/(2m)
 
  • #27
Yes, I think that's the correct answer, only that remember that ##\langle \mathbf{X} \rangle = \langle X_1 \rangle\hat{i} + \langle X_2 \rangle\hat{j} + \langle X_3 \rangle\hat{k}##.
 
  • #28
Thank you for your help!

Onto the Heisenberg picture portion of the question :)
 
  • #29
I feel like there is a way to manipulate the terms so as to put them back into a known relationship but I am not seeing it

I know that

[X_aH (t), X_bH (0)] = [U_d (t,0) X(t)_aH U (t,0),U_d (0,0) X (0)_bH U (0,0)] = U_d (t,0) X(t)_aH U (t,0) X (0)_b - X (0)_b U (t,0)_d X (t)_aH U (t,0)

Where
U (t,0) = exp (-i*t*H/hbar)
= exp (-i*t*(P^2/2m - E*q*X_1)/hbar)
 

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