Time correlation of an observable in the Schrödinger picture

In summary, the unitary transformation between the Schrödinger and Heisenberg pictures is given by ##\hat{U}##. This expression can be derived by looking at the Schrödinger and Heisenberg pictures for the special case of looking at the Schrödinger and Heisenberg pictures at ##t=0##.
  • #1
kith
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This has come up in a number of threads, so I made this thread to talk about it.
A. Neumaier said:
To define a time correlation ##\langle A(s)A(t)\rangle## one needs a family of operators ##A(s)## that depend on time, hence the Heisenberg picture. One can convert the expression into one in the Schroedinger picture, but the resulting expression has no meaning without its interpretation in the Heisenberg picture!
I think that an interpretation of this in the Schrödinger picture should be possible at least in the style of Feynman. This would go something like this.

##\begin{eqnarray*}
\langle A(s)A(t)\rangle_\psi &=& \langle \psi| U^\dagger (s) A U(s) U^\dagger(t) A U(t)|\psi\rangle\\
&=& \langle \psi(s)| A U(s-t) A |\psi(t)\rangle\\
&=& \langle \psi(s)| \left( \sum_i |a_i\rangle \langle a_i| \right) A U(s-t) A \left( \sum_j |a_j\rangle \langle a_j| \right) \psi(t)\rangle\\
&=& \sum_{i,j} a_i a_j \langle \psi(s)| a_i\rangle \langle a_i| U(s-t) |a_j\rangle \langle a_j| \psi(t)\rangle\\
\end{eqnarray*}##

For each term in the sum, we have an initial probability amplitude ##\langle a_j| \psi(t)\rangle##, a propagator-like quantity ##\langle a_i| U(s-t) |a_j\rangle## and a final probability amplitude ##\langle \psi(s)| a_i\rangle##, and we sum over all possibilities weighted with the product of the corresponding eigenvalues. This doesn't look completely meaningless to me, although I'm scratching my head a bit about what it's actual meaning could be. ;-)

Any thoughts?
 
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  • #2
kith said:
This doesn't look completely meaningless to me, although I'm scratching my head a bit about what it's actual meaning could be. ;-)
Maybe one can relate it to consistent histories?
 
  • #3
A. Neumaier said:
Maybe one can relate it to consistent histories?
I am not really familiar with this approach but it seems to be a second step to me. I don't yet understand what one such a history or path is, i.e. how the elements in the mathematical expression above could be interpreted. And maybe how this relates to the path integral about which I also have only superficial knowledge.
 
  • #4
I think that the next step would be to break down the propagator into many terms and inserting many complete terms of energy eigenstates.
 
  • #5
Very nice, but you should really indicate the quantities in different pictures with different symbols. Obviously you start with the Heisenberg picture with a system prepared in the pure state represented by the state vector
$$|\psi \rangle_H$$
which is constant in time. The observable ##A## is represented by the operator ##\hat{A}_H(t)## obeying the equation of motion
$$\dot{\hat{A}}_H(t)=\frac{1}{\mathrm{i}} [\hat{A}_H(t),\hat{H}_H],$$
where I assume that ##\hat{A}## is not explicitly time dependent and that ##\hat{H}_H## is time independent (closed system, energy conserved). The solution reads
$$\hat{A}_H(t)=\hat{U}(t) \hat{A}_H(0) \hat{U}^{\dagger}(t)=\hat{U}(t) \hat{A}_S \hat{U}^{\dagger}(t)$$
with
$$\hat{U}(t)=\exp(\mathrm{i} \hat{H}_H t).$$
I assumed that the Schrödinger picture coincides with the Heisenberg picture at ##t=0##. We obviously have ##\hat{H}_H=\hat{H}_S## in this case. The unitary transformation from one to the other picture is given by ##\hat{U}##:
$$\hat{A}_H=\hat{U} \hat{A}_S \hat{U}^{\dagger}, \quad |\psi,t \rangle_H= |\psi,0 \rangle_H=|\psi,0 \rangle_{S}=\hat{U}(t) |\psi,t \rangle_S.$$
Now indeed you have
$$C_{AA}(s,t)=_H\langle \psi,0|\hat{A}_H(s) \hat{A}_H(t)|\psi,0 \rangle_H=_S \langle \psi,t|\hat{U}^{\dagger}(t) \hat{U}(s) \hat{A}_S \hat{U}^{\dagger}(s) |\hat{U}(t) \psi,t \rangle= _S \langle \psi,t| \hat{U} (s-t) \hat{A}_S \hat{U}^{\dagger}(s-t)|\psi,t \rangle_S.$$
This is the picture independent expression. You have to read ##\hat{U}## as the unitary matrix transforming from the arbitrary picture you like to use (here the Schrödinger picture) to the Heisenberg picture. The direct derivation of this is a bit lengthy but as simple as this one for the special case of looking at the Schrödinger and Heisenberg pictures.

I've given the formulation of the transformations of states and observable-operators as well as transformations between arbitay pictures in

https://www.physicsforums.com/threa...n-the-heisenberg-picture.859478/#post-5393704
 
Last edited:
  • #6
vanhees71 said:
Very nice, but you should really indicate the quantities in different pictures with different symbols.
Please excuse my sloppiness. ;-) I think omitting the indices is ok as long as we don't deal with operators which are time-dependent even in the Schrödinger picture.

vanhees71 said:
$$C_{AA}(s,t)=_H\langle \psi,0|\hat{A}_H(s) \hat{A}_H(t)|\psi,0 \rangle_H=_S \langle \psi,t|\hat{U}^{\dagger}(t) \hat{U}(s) \hat{A}_S \hat{U}^{\dagger}(s) |\hat{U}(t) \psi,t \rangle= _S \langle \psi,t| \hat{U} (s-t) \hat{A}_S \hat{U}^{\dagger}(s-t)|\psi,t \rangle_S.$$
Hmm, how did you arrive at the second identity?
 
  • #7
My next step would be to consider a simple spin-1/2 example but unfortunately, I'm really busy right now.
 

Related to Time correlation of an observable in the Schrödinger picture

1. What is the Schrödinger picture in quantum mechanics?

The Schrödinger picture is one of the two commonly used pictures in quantum mechanics, along with the Heisenberg picture. In the Schrödinger picture, the state of a quantum system is represented by a time-dependent wave function, which evolves according to the Schrödinger equation. This picture is useful for studying the time evolution of a system.

2. What is an observable in the Schrödinger picture?

In the Schrödinger picture, an observable is a physical quantity that can be measured or observed in a quantum system. It is represented by a Hermitian operator, which acts on the wave function to give the possible outcomes of a measurement. Examples of observables include position, momentum, and energy.

3. How is the time correlation of an observable calculated in the Schrödinger picture?

The time correlation of an observable is calculated by taking the expectation value of the observable at two different points in time and then subtracting the product of the two expectation values. Mathematically, it can be expressed as C(t, t') = ⟨A(t)A(t')⟩ - ⟨A(t)⟩⟨A(t')⟩, where A is the observable and t, t' are the different points in time.

4. What does the time correlation of an observable tell us?

The time correlation of an observable provides information about how the observable changes over time. It can reveal patterns or trends in the behavior of the observable, such as whether it is constant, oscillating, or decaying. It is also used to calculate other important quantities in quantum mechanics, such as the autocorrelation function and the power spectrum.

5. How does the Schrödinger picture differ from the Heisenberg picture in terms of time correlation?

In the Schrödinger picture, time correlation is calculated using the wave function, while in the Heisenberg picture, it is calculated using the time-dependent operators. This leads to different expressions for the time correlation, although both approaches give the same physical results. Additionally, in the Heisenberg picture, the operators themselves do not change with time, while in the Schrödinger picture, the wave function evolves with time.

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