Time dependence of field operators

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Discussion Overview

The discussion revolves around the time dependence of field operators in the context of field theory, particularly focusing on the definition and interpretation of conjugate momentum in relation to the Lagrangian density. Participants explore the implications of using total versus partial derivatives and the consistency of notation within the framework of scalar fields.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions the standard definition of conjugate momentum, suggesting that the notation may be an abuse since ##\dot{\phi}## (total derivative) and ##\partial_{0}\phi## (partial derivative) are not equivalent in general.
  • Another participant argues that the notation is not much of an abuse, asserting that in field theory, ##\dot{\phi}## is often defined as ##\partial\phi/\partial t##.
  • There is a discussion about whether the conjugate momentum should be defined with respect to the total time derivative or the partial derivative, with some participants expressing confusion over the implications of implicit versus explicit time dependence in fields.
  • One participant clarifies that a field is a function of independent space and time variables, and discusses the transition to Hamiltonian formulation where canonical field momenta are defined.
  • Another participant emphasizes that the time dependence of field operators is determined by the Heisenberg picture of time evolution, where operators carry full time dependence.
  • Some participants acknowledge the presence of explicit time dependence in the field operators due to the evolution operator, while others express uncertainty about the implications of this time dependence in the context of the discussion.
  • Clarifications are made regarding the canonical field momentum and its relation to the Lagrangian density, with some participants reiterating the role of exponential terms in the momentum-mode decomposition of the free field.

Areas of Agreement / Disagreement

Participants express differing views on the interpretation of conjugate momentum and the use of notation in field theory. There is no consensus on whether the notation constitutes an abuse or is acceptable within the framework of field theory. The discussion remains unresolved regarding the implications of total versus partial derivatives.

Contextual Notes

Limitations include potential misunderstandings regarding the definitions of total and partial derivatives, as well as the implications of time dependence in fields. The discussion also reflects varying interpretations of the role of explicit versus implicit time dependence in the context of field equations.

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In field theory we most of deal with theories whose Lagrangian densities are of the form (sticking to scalar fields for simplicity) $$\mathcal{L}= -\frac{1}{2}\partial_{\mu}\phi\partial^{\mu}\phi - \frac{1}{2}m_{\phi}^{2}\phi^{2} + \cdots$$ where ##\partial := \frac{\partial}{\partial x^{\mu}}## and the dots represent any interaction terms.

Given this, one normally proceeds to define a conjugate momentum, ##\pi_{\phi}##, conjugate to the field ##\phi##. Now, in all the introductory texts that I've read, it is defined as $$\pi_{\phi} = \frac{\partial\mathcal{L}}{\partial\dot{\phi}} = \frac{\partial\mathcal{L}}{\partial(\partial_{0}\phi)}$$ However, this seems to be an abuse of notation, since ##\dot{\phi}## and ##\partial_{0}\phi## are not equal in general (after the former is a total time derivative, and the latter is a partial derivative with respect to time).

This being the case, how is one meant to interpret this definition? Is the conjugate momentum of the field equal to the partial derivative of the Lagrangian with respect to the total time derivative of the field, i.e. ##\dot{\phi}##, or with respect to the partial derivative of the field with respect to time, i.e. ##\frac{\partial\phi}{\partial t}:=\partial_{t}\phi##?

If it is the case that the conjugate momentum of the field equal to the partial derivative of the Lagrangian with respect to the partial derivative of the field with respect to time, then I fail to see how the formulation is consistent, since in the free-field case ##\phi## can be expressed as $$\phi(x)=\int\frac{d^{3}k}{(2\pi)^{3}}\frac{1}{(2E_{k})}\left(a(\mathbf{k})e^{-ik\cdot x}+a^{\dagger}(\mathbf{k})e^{ik\cdot x}\right)$$ where ##k\cdot x= k^{0}t -\mathbf{k}\cdot\mathbf{x}##.
This clearly has no explicit time dependence in it, which leaves me confused as to what's the correct way to proceed?!

Is the point that when we transition to field theory, the Lagrangian density is actually a function of ##\phi##, ##\dot{\phi}=\frac{d\phi}{dt}## and ##\nabla\phi##, i.e. $$\mathcal{L}=\mathcal{L}(\phi, \dot{\phi},\nabla{\phi})$$ and we then abuse notation, symbolically writing ##\partial_{\mu}\phi =(\dot{\phi},\nabla\phi)##, such that $$\mathcal{L}=\mathcal{L}(\phi, \dot{\phi},\nabla{\phi})=\mathcal{L}(\phi,\partial_{\mu}\phi)$$ Then, for example, in the Euler-Lagrange equation $$\partial_{\mu}\left(\frac{\partial\mathcal{L}}{\partial(\partial_{\mu}\phi)}\right)=\left(\frac{d}{dt}\left(\frac{\partial\mathcal{L}}{\partial\dot{\phi}}\right),\nabla\left(\frac{\partial\mathcal{L}}{\partial(\nabla\phi)}\right)\right)$$ if this is the case, then it all makes sense to me (I think).
 
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I do not think this is much of an abuse. How would you define the total derivative? You would need the field along a path, which is generally not what you have. In field theory we often simply define our notation as ##\dot\phi = \partial\phi/\partial t##.
 
Orodruin said:
I do not think this is much of an abuse. How would you define the total derivative? You would need the field along a path, which is generally not what you have. In field theory we often simply define our notation as ##\dot\phi = \partial\phi/\partial t##.

Yes, I appreciate that it's not much of an abuse of notation, but I just want to check that I've understood it all correctly. Would what I put in my last paragraph be correct at all?

My problem with it is that ##\partial_{t}\phi## will be zero unless ##\phi## has explicit time dependence, however, if it has implicit time dependence, then ##\frac{d\phi}{dt}## (which classical one would denote as ##\dot{\phi}## would be non-zero.
 
The last expression in your OP does not make sense. You have written that a divergence, which is a scalar, is equal to some sort of vector.

You will generally not see d/dt in field theory. I do not think there is any room for confusion.

So what if ##\phi## is not time dependent? This should be determined from the field equations.
 
Orodruin said:
The last expression in your OP does not make sense. You have written that a divergence, which is a scalar, is equal to some sort of vector.

Yes, apologies for that. I meant to write $$\partial_{\mu}\left(\frac{\partial\mathcal{L}}{\partial(\partial_{\mu}\phi)}\right)= \frac{d}{dt}\left(\frac{\partial\mathcal{L}}{\partial\dot{\phi}}\right) + \nabla_{i}\left(\frac{\partial\mathcal{L}}{\partial(\nabla_{i}\phi)}\right)$$
Where ##\nabla_{i}=\frac{\partial}{\partial x^{i}}=\partial_{i}##

Orodruin said:
So what if ϕϕ\phi is not time dependent? This should be determined from the field equations.

Fair enough, but how then does one determine the conjugate momentum ##\pi =\frac{\partial\mathcal{L}}{\partial(\partial_{0}\phi)}## of a field ##\phi## expressed as $$\phi(x)=\int\frac{d^{3}k}{(2\pi)^{3}}\frac{1}{(2E_{k})}\left(a(\mathbf{k})e^{-ik\cdot x}+a^{\dagger}(\mathbf{k})e^{ik\cdot x}\right)$$ Am I just being silly here and the explicit time dependence is contained in the exponentials ##e^{\pm ik\cdot x}##, i.e. ##\partial_{0}(e^{\pm ik\cdot x})=\pm ik^{0}te^{\pm ik\cdot x}##?
 
I don't understand the confusion. A field is a function of space and time arguments which are independent variables. In the Lagrange density you have the fields and their first partial derivatives (or covariant derivatives in General Relativity) as independent variables.

Then you can transform to the Hamiltonian formulation with the canonical field momenta defined as
$$\Pi=\frac{\partial \mathcal{L}}{\partial (\partial_0 \phi)}$$
and quanize the theory assuming the canonical equal-time commutators (or anti-commutators) for bosons (fermions). This leads to the time dependence according to the Heisenberg picture of the time evolution (i.e., operators defining observables carry the full time dependence.
 
vanhees71 said:
I don't understand the confusion. A field is a function of space and time arguments which are independent variables. In the Lagrange density you have the fields and their first partial derivatives (or covariant derivatives in General Relativity) as independent variables.

Then you can transform to the Hamiltonian formulation with the canonical field momenta defined as
$$\Pi=\frac{\partial \mathcal{L}}{\partial (\partial_0 \phi)}$$
and quanize the theory assuming the canonical equal-time commutators (or anti-commutators) for bosons (fermions). This leads to the time dependence according to the Heisenberg picture of the time evolution (i.e., operators defining observables carry the full time dependence.
Apologies, I think I was just being really stupid here. Of course, in the Heisenberg picture the field operators have explicit time dependence (due to the explicit time dependence contained in the evolution operator ##\hat{U}(t)=e^{-i\hat{H}t}##).

Is what I put in the last part of my previous post correct then (i.e. the explicit time dependence in ##\hat{\phi}(x)## is contained in the exponentials, such that ##\partial_{0}(e^{\pm ik\cdot x})=\pm ik^{0}e^{\pm ik\cdot x}##)?!
 
It's much simpler. For the KG field you wrote you have (with your sign convention, i.e., east coast)
$$\mathcal{L}=-\frac{1}{2} \partial_{\mu} \phi \partial^{\mu} \phi+V(\phi)=\frac{1}{2} (\dot{\phi}^2-(\vec{\nabla} \phi)^2)+V(\phi).$$
Then the canonical field momentum is
$$\Pi=\frac{\partial \mathcal{L}}{\partial \dot{\phi}}=\dot{\phi}.$$
For the free field you get the momentum-mode decomposition you've written down, and the space-time dependence is of course in the exponentials.
 
vanhees71 said:
For the free field you get the momentum-mode decomposition you've written down, and the space-time dependence is of course in the exponentials.

Yes, apologies. That is what I was trying to get at, but in a bit of a round-about way :sorry:
 
  • #10
vanhees71 said:
It's much simpler. For the KG field you wrote you have (with your sign convention, i.e., east coast)
$$\mathcal{L}=-\frac{1}{2} \partial_{\mu} \phi \partial^{\mu} \phi+V(\phi)=\frac{1}{2} (\dot{\phi}^2-(\vec{\nabla} \phi)^2)+V(\phi).$$
Then the canonical field momentum is
$$\Pi=\frac{\partial \mathcal{L}}{\partial \dot{\phi}}=\dot{\phi}.$$
For the free field you get the momentum-mode decomposition you've written down, and the space-time dependence is of course in the exponentials.

Just a quick follow-up question (which is I guess essentially what my original question boils down to), do the field operators ##\hat{\phi}(x)## in the Heisenberg picture evolve as $$ \dot{\hat{\phi}}(x) = i\left[\hat{H},\hat{\phi}(x)\right] + \partial_{t}\hat{\phi}(x)$$ (in units where ##\hbar = c = 1##), or as $$ \dot{\hat{\phi}}(x) = i\left[\hat{H},\hat{\phi}(x)\right]$$ If the latter is true, what is the reasoning for why the field operator ##\hat{\phi}(x)## (and its conjugate momentum ##\hat{\pi}_{\phi}(x)##) contain no explicit time dependence (i.e. why we can take ##\partial_{t}\hat{\phi}(x) = 0##)? Is it simply because, quantizing in the Schrödinger picture, the field operators have no time dependence and thus, since $$\partial_{t}\hat{\phi}_{H}(t,\mathbf{x}) =\hat{U}^{\dagger}(t)\partial_{t}\hat{\phi}_{S}(\mathbf{x})\hat{U}(t)$$ where the subscripts denote the two different pictures. Clearly, ##\partial_{t}\hat{\phi}_{S}(\mathbf{x})=0## and so ##\partial_{t}\hat{\phi}_{H}(t,\mathbf{x}) =0##.
 
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  • #11
By definition the fields obey
$$\dot{\hat{\phi}}(x) = \mathrm{i} \left[\hat{H},\hat{\phi}(x)\right].$$
Explicit time dependence comes in if you have functions of the "fundamental operators" of the theory, and the "fundamental operators" here is the field. So by definition its only time dependence in the Heisenberg picture is due to the equation of motion and not additionally "explicit" somehow.
 
  • #12
vanhees71 said:
By definition the fields obey
$$\dot{\hat{\phi}}(x) = \mathrm{i} \left[\hat{H},\hat{\phi}(x)\right].$$
Explicit time dependence comes in if you have functions of the "fundamental operators" of the theory, and the "fundamental operators" here is the field. So by definition its only time dependence in the Heisenberg picture is due to the equation of motion and not additionally "explicit" somehow.

So it's by construction then?! Is there any physical intuition for why they shouldn't have explicit time dependence?

vanhees71 said:
Explicit time dependence comes in if you have functions of the "fundamental operators" of the theory, and the "fundamental operators" here is the field.

By this, do you mean that ##\hat{\phi}## and ##\hat{\pi_{\phi}}## are in a sense, the fundamental variables of the theory and so any explicit time can only arise through functions of these fundamental variables, i.e. ##f(\hat{\phi},\hat{\pi_{\phi}},t)##?
 
  • #13
Yes, in QFT the field operators are the fundamental operators out of which you build all observables, and by definition the fundamental operators "move" with some time-local operator (which one you choose defines the picture of time evolution; for the Heisenberg picture it's ##\hat{H}##, for the Schrödinger picture it's ##0##, for the interaction picture it's the non-interacting part of the Hamilltonian, ##\hat{H}_0##, etc.). So your last sentence nails it to the answer to your question :-).
 

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