Derivation of energy-momentum tensor in "QFT and the SM" by Schwartz

  • #1
Hill
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How the contraction leads to ##g_{\mu \nu}## rather than ##\delta_{\mu \nu}##?
My question is about this step in the derivation:
1708892121220.png

When the ##\partial_\nu \mathcal L## in 3.33 moves under the ##\partial_\mu## in 3.34 and gets contracted, I'd expect it to become ##\delta_{\mu \nu} \mathcal L##. Why is it rather ##g_{\mu \nu} \mathcal L## in the 3.34?
(In this text, ##g_{\mu \nu}=\eta_{\mu \nu}##)
 
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  • #2
I think that eq.(3.34) contains a typo and you're (nearly) correct: in standard tensor notation, the ##g_{\mu\nu}## in (3.34) should actually be ##\delta^{\mu}_{\nu}##.
 
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  • #3
renormalize said:
I think that eq.(3.34) contains a typo and you're (nearly) correct: in standard tensor notation, the ##g_{\mu\nu}## in (3.34) should actually be ##\delta^{\mu}_{\nu}##.
Yes. The derivative has a lower mu in the denominator and hence acts like an upper index. This means the mu on the metric should also be upper, making it a kronecker delta.
 
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  • #4
Be careful when using this book as Schwartz employs a strange convention for contracting Lorentz tensors - namely, he ignores the positioning of the tensor indices (i.e., whether they are "upper" or "lower" indices), as he explains in this passage:

Zrzut ekranu z 2024-02-25 22-27-37.png


With this convention you get ambiguous expressions such as ##\partial_\mu (g_{\mu\nu} \mathcal{L})##, which you've encountered here, and which are impossible to interpret as they stand. Besides, there is always the possibility of there being a typo in a particular formula. All this can lead to unnecessary frustration, so it is best that you supplement the Schwartz's text with other books on QFT that you can always consult. Never let a textbook gaslight you while studying! :-p
 
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FAQ: Derivation of energy-momentum tensor in "QFT and the SM" by Schwartz

What is the energy-momentum tensor in quantum field theory (QFT)?

The energy-momentum tensor, often denoted as \( T^{\mu\nu} \), is a tensor quantity in quantum field theory that encapsulates the density and flux of energy and momentum in spacetime. It plays a crucial role in the formulation of conservation laws and is essential for describing the dynamics of fields and particles in both classical and quantum theories.

How is the energy-momentum tensor derived in Schwartz's "QFT and the SM"?

In Schwartz's "Quantum Field Theory and the Standard Model," the energy-momentum tensor is derived using Noether's theorem, which relates symmetries of the action to conserved quantities. For a given Lagrangian density \( \mathcal{L} \), the energy-momentum tensor can be obtained by considering the invariance of the action under spacetime translations and applying the resulting conserved current.

What role does the energy-momentum tensor play in the Standard Model of particle physics?

In the Standard Model of particle physics, the energy-momentum tensor is crucial for understanding the interactions and dynamics of fundamental particles and fields. It provides a way to describe how energy and momentum are distributed and conserved in particle interactions, and it is essential for formulating the equations of motion for fields and particles within the framework of the Standard Model.

How does the energy-momentum tensor relate to the conservation laws in QFT?

The energy-momentum tensor is directly related to the conservation laws in quantum field theory through Noether's theorem. The conservation of energy and momentum arises from the invariance of the action under spacetime translations. This invariance leads to the conservation of the energy-momentum tensor, expressed mathematically as \( \partial_\mu T^{\mu\nu} = 0 \), indicating that the divergence of the tensor is zero.

What is the significance of the symmetric form of the energy-momentum tensor?

The symmetric form of the energy-momentum tensor is significant because it ensures that the tensor correctly represents the physical properties of the system, such as the stress and energy flux. In many cases, the canonical energy-momentum tensor derived from Noether's theorem is not symmetric. However, it can be symmetrized using the Belinfante-Rosenfeld procedure, which involves adding a divergence-free term to the tensor. The symmetric form is particularly important in the context of general relativity, where it couples to the spacetime metric in Einstein's field equations.

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