The Energy-Momentum Tensor

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Discussion Overview

The discussion revolves around the relationship between the stress-energy tensor as defined in General Relativity and the energy-momentum tensor encountered in Quantum Field Theory (QFT). Participants explore the definitions, equivalences, and distinctions between these tensors, as well as their implications in different contexts.

Discussion Character

  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants express confusion regarding the terminology and definitions of the stress-energy tensor and energy-momentum tensor, citing different sources.
  • One participant notes that the general definition of the symmetrical energy-momentum tensor is given by $$T_{\mu\nu}=\frac{2}{\sqrt{-g}}\frac{\delta(\mathcal{L} \sqrt{-g})}{\delta g_{\mu\nu}}$$ and contrasts it with the canonical energy-momentum tensor $$T^{\mu\nu}=\frac{\partial\mathcal{L}}{\partial( \partial_\mu\phi_{a})}\partial^\nu\phi_a -g^{\mu\nu}\mathcal{L}$$.
  • Another participant argues that the two forms of the energy-momentum tensor are not generally the same, but they can lead to the same energy-momentum 4-vector under certain conditions.
  • It is mentioned that in QFT, the stress-energy tensor is not unique, as additional terms can be added without affecting conservation laws, and a modified tensor, the Belinfante–Rosenfeld stress-energy tensor, can align with the Hilbert stress-energy tensor used in General Relativity.
  • A reference to Wald's discussion is made, highlighting that the first form of the tensor arises naturally from formulating General Relativity as a Lagrangian theory.

Areas of Agreement / Disagreement

Participants do not reach a consensus on whether the stress-energy tensor and energy-momentum tensor are equivalent in all cases, indicating that multiple competing views remain regarding their definitions and applications.

Contextual Notes

Some limitations are noted, such as the dependence on definitions and the context in which the tensors are applied, particularly in relation to different fields and formulations.

agostino981
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I am a bit confused here.

In the Einstein Field Equation, there is a tensor called stress-energy tensor in wikipedia and energy-momentum tensor in some books or papers which is $$T_{\mu\nu}=\frac{2}{\sqrt{-g}}\frac{\delta(\mathcal{L} \sqrt{-g})}{\delta g_{\mu\nu}}$$

Is it equivalent to the energy-momentum tensor I came across in QFT?

$$T^{\mu\nu}=\frac{\partial\mathcal{L}}{\partial( \partial_\mu\phi_{a})}\partial^\nu\phi_a -g^{\mu\nu}\mathcal{L}$$

Thanks in advance.
 
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agostino981 said:
I am a bit confused here.

In the Einstein Field Equation, there is a tensor called stress-energy tensor in wikipedia and energy-momentum tensor in some books or papers which is $$T_{\mu\nu}=\frac{2}{\sqrt{-g}}\frac{\delta(\mathcal{L} \sqrt{-g})}{\delta g_{\mu\nu}}$$
This is the general definition of the SYMMETRICAL energy-momentum tensor.

$$T^{\mu\nu}=\frac{\partial\mathcal{L}}{\partial( \partial_\mu\phi_{a})}\partial^\nu\phi_a -g^{\mu\nu}\mathcal{L}$$
Thanks in advance.

This is the CANONICAL energy-momentum tensor. For scalar fields, the two are identical. For other fields they differ by a total divergence. They are equivalent in the sense that both leads to the same energy-momentum 4-vector
P^{ \mu } = \int d^{ 3 } x T^{ 0 \mu } ( x )
 
agostino981 said:
I am a bit confused here.

In the Einstein Field Equation, there is a tensor called stress-energy tensor in wikipedia and energy-momentum tensor in some books or papers which is $$T_{\mu\nu}=\frac{2}{\sqrt{-g}}\frac{\delta(\mathcal{L} \sqrt{-g})}{\delta g_{\mu\nu}}$$

Is it equivalent to the energy-momentum tensor I came across in QFT?

$$T^{\mu\nu}=\frac{\partial\mathcal{L}}{\partial( \partial_\mu\phi_{a})}\partial^\nu\phi_a -g^{\mu\nu}\mathcal{L}$$

Thanks in advance.

They are not, in general, the same. However, in QFT, the stress-energy tensor is not unique, because you can add additional terms to it that have no effect on conservation laws. There is a procedure for tweaking the canonical stress-energy tensor to get a modified tensor, the Belinfante–Rosenfeld stress–energy tensor, that (according to Wikipedia, at least) agrees with the Hilbert stress-energy tensor used by General Relativity:
http://en.wikipedia.org/wiki/Belinfante–Rosenfeld_stress–energy_tensor
 
Wald has a good discussion of this, and shows that the first form arises naturalliy from formulating GR as a Lagrangian theory.
 
Thanks! That clears things up.
 

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