Graduate Covariance of equal time commutation relations

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The discussion centers on the covariance of equal time commutation relations in relativistic quantum field theory, specifically for scalar fields. It highlights that the commutator between the field and its conjugate momentum is zero outside the light cone, yet raises concerns about the invariance of the equal time commutation relations expressed as derivatives of invariant quantities. The participant notes that the delta function involved is also not invariant, questioning how a covariant theory can emerge from non-invariant second quantization rules. References to further literature are sought to clarify these issues and provide deeper insights into the topic. The conversation underscores the complexities of maintaining covariance in quantum field theory formulations.
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I have a question regarding the covariance of the equal time commutation relations in relativistic quantum field theory. In the case of a scalar field one has that the commutator is (see Peskin, pag. 28 eq. (2.53) )
$ [\phi(0), \phi(y)] = D(-y) - D(y) $
is an invariant function, which is zero outside the light cone.

The commutator between the field and the conjugate momentum is

$[\phi(0), \pi(y)] = [\phi(0), \dot \phi(y)] = \partial_{y^0} [\phi(0), \phi(y)] , $

which also implies that $ [\phi(0), \pi(y)] = 0 $ outside the light cone. The equal time commutation rules which lead to second quantization read

$[\phi(0), \pi(y)] = \partial_{y^0} [\phi(0), \phi(y)] = i \delta^3(\vec{y})$ for $ y^0 = 0 $.

However this point seems to me a little bit odd, since this relation, being expressed as the derivative of an invariant quantity, is not invariant. This is also confirmed by the fact that the $\delta^3$ is also not invariant. Therefore, I wonder how we get a covariant theory starting from second quantization rules which are not invariant, or why this fact does not lead to any contradiction.
 
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Thank you for your comments. I had a look to Eq. (13) in http://de.arxiv.org/abs/hep-th/0202204 and this (the result of (13) shouldn't be $$ i \chi(x)/\sqrt(g_{00})$$ ?) just confirms that the formulation of the equal time commutation relations depends on the choice of $$ \Sigma $$. Even if one expresses the relation in an invariant form as $$n^\mu \partial_\mu [\phi(0),\phi(x)] = i \frac{\delta(x)}{\sqrt{g_{00} g^3}}$$ the quantity on the r.h.s. is not an invariant unless $$ g_{0i}=0$$.

There is some other reference where this topic is treated more in detail?
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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