Maxwell field commutation relations

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SUMMARY

The discussion centers on the canonical momentum and commutation relations for the Maxwell field as presented in Aitchison and Hey's Quantum Field Theory book. The canonical momentum is defined as \(\pi^0=\partial_\mu A^\mu\) and \(\pi^i=-\dot{A}^i+\partial^i A^0\). The key commutation relation is \([\hat{A}_\mu(\boldsymbol{x},t),\hat{\pi}_\nu(\boldsymbol{y},t)]=ig_{\mu\nu}\delta^3(\boldsymbol{x}-\boldsymbol{y})\). The discussion clarifies that spatial derivatives of the field operators \(\hat{A}_\mu\) commute with each other and with the operators themselves at equal times, a point that some participants initially found non-obvious.

PREREQUISITES
  • Understanding of canonical momentum in quantum field theory
  • Familiarity with commutation relations in quantum mechanics
  • Knowledge of Hamiltonian formalism
  • Basic concepts of Lorentz covariance
NEXT STEPS
  • Study the canonical quantization of the Maxwell field in detail
  • Explore the implications of commutation relations in quantum field theory
  • Learn about the role of Lorentz covariance in Hamiltonian mechanics
  • Investigate the differences between time and spatial derivatives in quantum fields
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Physicists, particularly those specializing in quantum field theory, students studying Aitchison and Hey's QFT, and researchers interested in the mathematical foundations of electromagnetism in a quantum context.

eudo
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Maxwell field commutation relations

I'm looking at Aitchison and Hey's QFT book. I see in Chapter 7, (pp. 191-192), they write down the canonical momentum for the Maxwell field A^\mu(x):

<br /> \pi^0=\partial_\mu A^\mu \\<br /> \pi^i=-\dot{A}^i+\partial^i A^0<br />

and then write down the commutation relations

<br /> [\hat{A}_\mu(\boldsymbol{x},t),\hat{\pi}_\nu(\boldsymbol{y},t)]=ig_{\mu\nu}\delta^3(\boldsymbol{x}-\boldsymbol{y})<br />

and state that if you assume the commutation relations

<br /> [\hat{A}_\mu(\boldsymbol{x},t),\hat{A}_\nu(\boldsymbol{y},t)]=[\hat{\pi}_\mu(\boldsymbol{x},t),\hat{\pi}_\nu(\boldsymbol{y},t)]=0<br />

we see that the spatial derivatives of the \hat{A}'s commute with the \hat{A}'s, and with each other, at equal times.

They state it as if it's obvious, so maybe I'm missing something, but I don't see why the spatial derivatives of the \hat{A}'s commute with the \hat{A}'s, and with each other.
 
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You just take the derivatives with respect to spatial components ##\vec{x}## or ##\vec{y}##, and you see that the equatl-time commutators stay 0. It's different for the time derivative, because here you have the same time argument in both entries of the commutator. It's the specialty of time vs. space coordinates in the Hamiltonian formalism, which is never manifestly Lorentz covariant!
 
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Ah, I see. The spatial arguments of the A_\mu and A_\nu are different, of course... I seem to have overlooked that. Thanks!
 

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