Canonical quantization of scalar fields

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Discussion Overview

The discussion revolves around the canonical quantization of scalar fields, specifically focusing on the transition from a position representation of the Hamiltonian to a momentum representation. Participants explore the implications of commutation relations between operators and functions in this context.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant questions whether the transition from the Hamiltonian in position space to momentum space is straightforward or if it requires considering commutation relations, particularly between the operators involved.
  • Another participant provides a mode decomposition of the scalar field in the Heisenberg picture and confirms the form of the Hamiltonian, emphasizing the need to distinguish between operators and numbers.
  • A participant seeks clarification on the commutation between the operator \(P^{2}\) and the exponential function \(e^{ipx}\), indicating uncertainty about how to perform this commutation.
  • Another participant asserts that \(P^{2}\) is a real number in the context of the discussion, which commutes with all operators, but notes a lack of access to the original text for further context.

Areas of Agreement / Disagreement

Participants express differing views on the necessity of considering commutation relations in the transition between representations, indicating that the discussion remains unresolved regarding the implications of these relations.

Contextual Notes

There is an assumption that participants are familiar with the mathematical formalism of quantum field theory, but specific steps in the manipulation of operators and functions remain unclear or unresolved.

Higgsy
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In the srednicki notes he goes from

$$H = \int d^{3}x a^{\dagger}(x)\left( \frac{- \nabla^{2}}{2m}\right) a(x) $$ to
$$H = \int d^{3}p\frac{1}{2m}P^{2}\tilde{a}^{\dagger}(p)\tilde{a}(p) $$

Where $$\tilde{a}(p) = \int \frac{d^{3}x}{(2\pi)^{\frac{3}{2}}}e^{-ipx}a(x)$$

Is this as simple as substituting or isn't there a commutator to get to
$$H = \int d^{3}p\frac{1}{2m}P^{2}\tilde{a}^{\dagger}(p)\tilde{a}(p)$$ ?

Do $$e^{ipx}$$ and $$P^{2}$$ commute? What about $$\nabla$$ and $$ a(x)$$?

This is really bugging me any help would be greatly appreciated!
 
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This is obviously non-relativistic QFT. Then the scalar field (quantized Schrödinger field) in the Heisenberg picture has a mode decomposition
$$\hat{\psi}(t,\vec{x})=\int_{\mathbb{R}^3} \frac{\mathrm{d}^3 \vec{p}}{(2 \pi)^{3/2}} \exp[-\mathrm{i} (\omega_{\vec{p}}t-\vec{x} \cdot \vec{p})] \hat{a}(\vec{p}), \quad \omega_{\vec{p}}=\frac{\vec{p}^2}{2m}.$$
The free Hamiltonian is indeed given by
$$\hat{H}=\int_{\mathbb{R}^3} \mathrm{d}^3 \vec{x} \hat{\psi}^{\dagger}(t,\vec{x}) \left (-\frac{\Delta}{2m} \right ) \hat{\psi}(t,\vec{x}).$$
Now you can plug in the mode decomposition for ##\hat{\psi}(t,\vec{x})##. After some simple but lengthy manipulations, using
$$\int_{\mathbb{R}} \mathrm{d}^3 \vec{x} \exp(\mathrm{i} \vec{p} \vec{x})=(2 \pi)^3 \delta^{(3)}(\vec{p})$$
you indeed find that
$$\hat{H}=\int_{\mathbb{R}^3} \mathrm{d}^3 \vec{p} \omega_{\vec{p}} \hat{a}^{\dagger}(\vec{p}) \hat{a}(\vec{p}).$$
It's important, particularly in the beginning to somehow distinguish between usual real or complex numbers and operators. Above, I've written a hat above operators. Of course the operators are all linear operators on Hilbert space and thus commute with all usual real or complex numbers!
 
But does $$P^{2}$$ commute with$$e^{ipx}$$ or how can I perform this commutation?
 
In the above equation ##P^2## is obviously ##\vec{p}^2## and thus a real number, which commutes with all operators. Unfortunately I don't have my copy of Srednicky's book here; so I can't look at the context right now.
 

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