Time Evolution of the Complex Scalar Field

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SUMMARY

The discussion focuses on the time evolution of the complex scalar field described by the Lagrangian \( L = \partial_{\mu}\phi^{*}(x)\partial^{\mu}\phi(x) - m^2\phi^{*}(x)\phi(x) \). The canonical commutation relations establish that the conjugate momenta \( \pi(x) \) and \( \pi^{*}(x) \) are defined as \( \pi(x) = \partial_0\phi^{*}(x) \) and \( \pi^{*}(x) = \partial_0\phi(x) \). The main question raised is why only the first commutator survives in the evaluation of the Hamiltonian, with the conclusion that the commutator \( [\phi(x), \phi(y)] \) vanishes for space-like separations, thus preserving causality.

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  • Understanding of Lagrangian mechanics and Hamiltonian formalism.
  • Familiarity with quantum field theory concepts, particularly commutation relations.
  • Knowledge of the Heisenberg picture of quantum mechanics.
  • Basic understanding of causality in quantum fields.
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  • Study the derivation of the Hamiltonian from the Lagrangian in quantum field theory.
  • Learn about canonical quantization and its implications for field operators.
  • Research the role of causality in quantum field theory, particularly in relation to commutation relations.
  • Examine the implications of space-like and time-like separations in quantum mechanics.
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This discussion is beneficial for graduate students in physics, particularly those specializing in quantum field theory, as well as researchers exploring the foundations of quantum mechanics and field theory dynamics.

Xenosum
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Homework Statement



Consider the Lagrangian, L, given by

L = \partial_{\mu}\phi^{*}(x)\partial^{\mu}\phi(x) - m^2\phi^{*}(x)\phi(x) .

The conjugate momenta to \phi(x) and \phi^{*}(x) are denoted, respectively, by \pi(x) and \pi^{*}(x). Thus,

\pi(x) = \frac{\partial L}{\partial(\partial_{0}\phi(x))} = \partial_0\phi^{*}(x)
\pi^{*}(x) = \frac{\partial L}{\partial(\partial_{0}\phi^{*}(x))} = \partial_0\phi(x) .

Upon quantizing the system, \phi(x) and \phi^{*}(x) are promoted to operators which satisfy the equal-time commutation relations:

[ \phi(x) , \pi(y) ] = i\delta^{(3)}(\vec{x} - \vec{y})
[ \phi^{*}(x) , \pi^{*}(y) ] = i\delta^{(3)}(\vec{x} - \vec{y})

(all others zero). In the Heisenberg regime, the time evolution of the operator \phi(x), i \partial_0 \phi(x), is given by

i \partial_0 \phi(x) = \left[ \phi(x) , H(y) \right].

The Hamiltonian may be derived from the Lagrangian, and we find that

i\frac{\partial \phi(x)}{\partial t} = \int d^{3}y \left( \left[ \phi(x) , \pi(y)\pi^{*}(y) \right] + \left[ \phi(x) , \nabla\phi^{*}(y) \cdot \nabla\phi(y) \right] + m^2 \left[ \phi(x) , \phi^{*}(y)\phi(y) \right] \right).

Now here's my question. When we evaluate the commutators both my professor and a solution manual to Peskin and Schroeder claim that only the first commutator survives, because \phi(x) commutes with everything except for the its conjugate momentum (by the canonical commutation relations). I don't see why. The canonical commutation relations only give us a relationship between \phi(x) and \pi(y), not e.g. \phi(x) and \phi(y). The point is pressed by the fact that one can only show that the commutator \left[ \phi(x) , \phi(y) \right] vanishes for space-like separation between the points x and y (this is the condition which preserves causality).

I guess it would be resolved if the commutator were instead \left[ \phi(x) , H(x) \right], but this doesn't seem to be how it's done.

Thanks for any help!

Homework Equations


The Attempt at a Solution

 
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Xenosum said:
In the Heisenberg regime, the time evolution of the operator ϕ(x) \phi(x) , i∂0ϕ(x) i \partial_0 \phi(x) , is given by

i∂0ϕ(x)=[ϕ(x),H(y)].​

The Hamiltonian really should be the Hamiltonian at time ##x^0 = y^0## (note that you are integrating over the spatial components of ##y##). As a result, ##x## and ##y## have space-like separation and the commutator ##[\phi(x),\phi(y)]## vanishes (they are even equal-time).
 
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Cool, thanks!
 

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