# Conserved Noether charges for Lorentz symmetry of the action

• spaghetti3451

## Homework Statement

Consider the infinitesimal form of the Lorentz tranformation: ##x^{\mu} \rightarrow x^{\mu}+{\omega^{\mu}}_{\nu}x^{\nu}##.

Show that a scalar field transforms as ##\phi(x) \rightarrow \phi'(x) = \phi(x)-{\omega^{\mu}}_{\nu}x^{\nu}\partial_{\mu}\phi(x)## and hence show that the variation of the Lagrangian density is a total derivative ##\delta \mathcal{L}=-\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L})##.

Using Noether's theorem deduce the existence of the conserved current ##j^{\mu}=-{\omega^{\rho}}_{\nu}[{T^{\mu}}_{\rho}x^{\nu}]##.

The three conserved charges arising from spatial rotational invariance define the total angular momentum of the field. Show that these charges are given by ##Q_{i}=\epsilon_{ijk}\int d^{3}x (x^{j}T^{0k}-x^{k}T^{0j})##.

Derive the conserved charges arising from invariance under Lorentz boosts. Show that they imply ##\frac{d}{dt}\int d^{3}x (x^{i}T^{00})= \text{constant}## and interpret this equation.

## The Attempt at a Solution

Under the infinitesimal form of the Lorentz tranformation given by

##x^{\mu} \rightarrow x^{\mu}+{\omega^{\mu}}_{\nu}x^{\nu}={\delta^{\mu}}_{\nu}x^{\nu}+{\omega^{\mu}}_{\nu}x^{\nu}=({\delta^{\mu}}_{\nu}+{\omega^{\mu}}_{\nu})x^{\nu}={(\Lambda)^{\mu}}_{\nu}x^{\nu}##, so that ##{(\Lambda^{-1})^{\mu}}_{\nu}={\delta^{\mu}}_{\nu}-{\omega^{\mu}}_{\nu},##

a scalar field transforms as

##\phi(x) \rightarrow \phi'(x) = \phi(\Lambda^{-1}x) = \phi({(\Lambda^{-1})^{\mu}}_{\nu}x^{\nu}) = \phi(({\delta^{\mu}}_{\nu}-{\omega^{\mu}}_{\nu})x^{\nu}) = \phi(x^{\mu}-{\omega^{\mu}}_{\nu}x^{\nu}) = \phi(x)-{\omega^{\mu}}_{\nu}x^{\nu}\partial_{\mu}\phi(x),##

where in the last step, I used the following Taylor expansion of ##f(x+\delta x)## (where ##f## is a scalar and ##x## is a ##4##-vector):

##f(x+\delta x) = f(x) + x^{\nu}\frac{\partial f}{\partial x^{\nu}}+\dots##

and we ignore all the higher order terms since the transformation ##{\omega^{\mu}}_{\nu}## is infinitesimal.

Similarly,
##\mathcal{L}(x) \rightarrow \mathcal{L}'(x) = \mathcal{L}(\Lambda^{-1}x) = \mathcal{L}({(\Lambda^{-1})^{\mu}}_{\nu}x^{\nu}) = \mathcal{L}(({\delta^{\mu}}_{\nu}-{\omega^{\mu}}_{\nu})x^{\nu}) = \mathcal{L}(x^{\mu}-{\omega^{\mu}}_{\nu}x^{\nu}) = \mathcal{L}(x)-{\omega^{\mu}}_{\nu}x^{\nu}\partial_{\mu}\mathcal{L}(x)##

so that

##\delta \mathcal{L} = -{\omega^{\mu}}_{\nu}x^{\nu}\partial_{\mu}\mathcal{L}(x)##
##\implies \delta \mathcal{L} = -\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L}(x))+{\omega^{\mu}}_{\nu}\mathcal{L}(x)\partial_{\mu}x^{\nu}##
##\implies \delta \mathcal{L} = -\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L}(x))+{\omega^{\mu}}_{\nu}\mathcal{L}(x)\delta^{\nu}_{\mu}##
##\implies \delta \mathcal{L} = -\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L}(x))+{\omega^{\mu}}_{\mu}\mathcal{L}(x)##
##\implies \delta \mathcal{L} = -\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L}(x))##,

where the last line follows from the antisymmetry ##{\omega^{\mu}}_{\nu}=-{\omega^{\nu}}_{\mu}## of ##{\omega^{\mu}}_{\nu}## so that the diagonal elements, and by extension the sum of the diagonal elements ##{\omega^{\mu}}_{\mu}##, is ##0##.

Am I correct so far?

Looks ok to me. (A mathematican would barf on seeing ##\phi(x) = \phi(x^\mu)##, but physicists will know what you mean.)

(BTW, you should probably include the general formula for the energy-momentum tensor ##T## in the "relevant equations" section, since you'll need it for the next part.)

• topsquark
Looks ok to me. (A mathematican would barf on seeing ##\phi(x) = \phi(x^\mu)##, but physicists will know what you mean.)

Thanks!

(BTW, you should probably include the general formula for the energy-momentum tensor ##T## in the "relevant equations" section, since you'll need it for the next part.)

The general formula for the energy-momentum tensor ##{T^{\mu}}_{\nu}## is

##{T^{\mu}}_{\nu}=\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}\partial_{\nu}\phi(x)-\delta^{\mu}_{\nu}\mathcal{L}##

(I am not able to include the general formula for the energy-momentum tensor ##{T^{\mu}}_{\nu}## in the "relevant equations" section, since I don't have the editing privilege for my first post anymore.)

Next, I need to use Noether's theorem to deduce the existence of the conserved current ##j^{\mu}=-{\omega^{\rho}}_{\nu}[{T^{\mu}}_{\rho}x^{\nu}]##:

##\delta\phi=-{\omega^{\mu}}_{\nu}x^{\nu}\partial_{\mu}\phi(x)## and ##\delta\mathcal{L}=-\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L})##

so that

##\delta\mathcal{L}=\partial_{\mu}\Big(\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}\delta\phi\Big)##
##\implies -\partial_{\mu}({\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L})=-\partial_{\mu}\Big(\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}{\omega^{\rho}}_{\nu}x^{\nu}\partial_{\rho}\phi(x)\Big)##
##\implies \partial_{\mu}\Big(-\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}{\omega^{\rho}}_{\nu}x^{\nu}\partial_{\rho}\phi(x)+{\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L}\Big)=0##
##\implies \partial_{\mu}j^{\mu}=0##

where

##j^{\mu}=-\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}{\omega^{\rho}}_{\nu}x^{\nu}\partial_{\rho}\phi(x)+{\omega^{\mu}}_{\nu}x^{\nu}\mathcal{L}##
##\implies j^{\mu}=-\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}{\omega^{\rho}}_{\nu}x^{\nu}\partial_{\rho}\phi(x)+\delta^{\mu}_{\rho}{\omega^{\rho}}_{\nu}x^{\nu}\mathcal{L}##
##\implies j^{\mu}=-{\omega^{\rho}}_{\nu}x^{\nu}\Big(\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}\partial_{\rho}\phi(x)-\delta^{\mu}_{\rho}\mathcal{L}\Big)##
##\implies j^{\mu}=-{\omega^{\rho}}_{\nu}x^{\nu}{T^{\mu}}_{\rho}##
##\implies j^{\mu}=-{\omega^{\rho}}_{\nu}[{T^{\mu}}_{\rho}x^{\nu}]##

What do you think?

The general formula for the energy-momentum tensor: ##{T^{\mu}}_{\nu}=\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}\partial_{\nu}\phi(x)-\delta^{\mu}_{\nu}\mathcal{L}##
[...]

so that

##\delta\mathcal{L}=\partial_{\mu}\Big(\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\phi)}\delta\phi\Big)##
It's not clear how you got the last line. Which textbook (or other source) are you using?

I am using David Tong's lecture notes on QFT. In particular, I'm referring to equation (1.37) on page 14.

I missed the following couple of lines:

##\delta\mathcal{L}=\frac{\partial\mathcal{L}}{\partial\phi}\delta\phi+\frac{\partial\mathcal{L}}{\partial (\partial_{\mu}\phi)}\partial_{\mu}(\delta\phi)##

##\implies \delta\mathcal{L}=\Big[\frac{\delta\mathcal{L}}{\delta\phi}-\partial_{\mu}\Big(\frac{\delta\mathcal{L}}{\partial (\partial_{\mu}\phi)}\Big)\Big]\delta\phi+\partial_{\mu}\Big(\frac{\partial\mathcal{L}}{\partial (\partial_{\mu}\phi)}\delta\phi\Big)##

##\implies \delta\mathcal{L}=\partial_{\mu}\Big(\frac{\partial\mathcal{L}}{\partial (\partial_{\mu}\phi)}\delta\phi\Big)##, using the Euler-Lagrange field equations.

Oh, OK. It's a long time since I looked at Tong's notes. I should probably refresh my memory.

I learned this stuff from Greiner & Reinhardt "Field Quantization". But their formulas seem consistent with what you've done, since you're only working with a scalar field.

Edit: Dammit. Tong's proof of Noether's Thm takes less than a page, whereas G&R take more than 3 pages since they do it far more carefully. Tong just considers symmetries of the Lagrangian but G&R consider invariance of the action integral, which is more involved (and also leads to a slightly larger class of symmetries). Now I'm going to have to totally refresh my memories of both. But not today.

Last edited:

Let me try and solve the remaining parts of the problem.

The three conserved charges arising from spatial rotational invariance define the total angular momentum of the field. Show that these charges are given by ##Q_{i}=\epsilon_{ijk}\int d^{3}x (x^{j}T^{0k}-x^{k}T^{0j})##.

##j^{\mu}=-{\omega^{\rho}}_{\nu}[{T^{\mu}}_{\rho}x^{\nu}]##

##=-\omega_{\rho\nu}[T^{\mu\rho}x^{\nu}]## [I've raised the ##\rho## index on ##T## and lowered the ##\rho## index on ##\omega## since ##T## in the final expression for ##Q_i## has both upper indices.]

##=(-\omega_{0i}[T^{\mu 0}x^i]-\omega_{i0}[T^{\mu i}x^0])+(-\omega_{ij}[T^{\mu i}x^j]-\omega_{ji}[T^{\mu j}x^i])##, for ##i<j## in the third and fourth terms

##=(-\omega_{0i}[T^{\mu 0}x^i]+\omega_{0i}[T^{\mu i}x^0])+(-\omega_{ij}[T^{\mu i}x^j]+\omega_{ij}[T^{\mu j}x^i])##, for ##i<j## in the third and fourth terms

##=(\omega_{0i}[-T^{\mu 0}x^i+T^{\mu i}x^0])+(\omega_{ij}[-T^{\mu i}x^j+T^{\mu j}x^i])##, for ##i<j## in the third and fourth terms

##=(\omega_{\rho\sigma}[-T^{\mu\rho}x^{\sigma}+T^{\mu\sigma}x^{\rho}]),## for ##\rho < \sigma##

Defining ##(\mathcal{J}^{\mu})^{\rho\sigma}=-T^{\mu\rho}x^{\sigma}+T^{\mu\sigma}x^{\rho}## for ##\rho < \sigma##,

we see that ##\partial_{\mu}(\mathcal{J}^{\mu})^{\rho\sigma}=-(\partial_{\mu}T^{\mu\rho})x^{\sigma}+(\partial_{\mu}T^{\mu\sigma})x^{\rho}=0,## because ##\partial_{\mu}T^{\mu\nu}=0##.

Therefore, for ##\rho\sigma=\{01,02,03,12,13,23\}##, ##(\mathcal{J}^{\mu})^{\rho\sigma}## corresponds to six conserved Noether currents which sum to give the Noether current ##j^{\mu}##.

The Noether currents ##(\mathcal{J}^{\mu})^{12},(\mathcal{J}^{\mu})^{13}## and ##(\mathcal{J}^{\mu})^{23}## correspond to the invariance of the action under the spatial rotation of the spacetime coordinates.

Therefore, the conserved Noether charges ##(\mathcal{J}^{0})^{12},(\mathcal{J}^{0})^{13}## and ##(\mathcal{J}^{0})^{23}## arise as a consequence of the invariance of the action under the spatial rotation of the spacetime coordinates.

Therefore, the conserved Noether charges are ##Q^{jk}=-T^{0j}x^{k}+T^{0k}x^{j}=x^{j}T^{0k} - x^{k}T^{0j}## for ##j < k##

so that ##Q_{i}=\epsilon_{ijk}x^{j}T^{0k}## for ##j < k##.

Am I correct? My answer looks different from what they require and I'm also having difficulty understanding the concept of the total angular momentum.

Defining ##(\mathcal{J}^{\mu})^{\rho\sigma}=-T^{\mu\rho}x^{\sigma}+T^{\mu\sigma}x^{\rho}## for ##\rho < \sigma##,

we see that ##\partial_{\mu}(\mathcal{J}^{\mu})^{\rho\sigma}=-(\partial_{\mu}T^{\mu\rho})x^{\sigma}+(\partial_{\mu}T^{\mu\sigma})x^{\rho}=0,## because ##\partial_{\mu}T^{\mu\nu}=0##.
I suspect you're missing something here. I get: $$\partial_{\mu}(\mathcal{J}^{\mu})^{\rho\sigma}~=~ -(\partial_{\mu}T^{\mu\rho})x^{\sigma} - T^{\mu\rho} \delta^\sigma_\mu + (\partial_{\mu}T^{\mu\sigma})x^{\rho} + T^{\mu\sigma} \delta^\sigma_\mu .$$ The derivatives vanish as you said, but that still leaves ##-T^{\sigma\rho} + T^{\rho\sigma},## which only vanishes if ##T## is symmetric. Usually, that requires an additional argument, wherein one adds a particular total derivative to ##T## which preserves the conservation rule, but also guarantees that its integrals over all space are unchanged. (This might also be the source of your uncertainty about "total angular momentum", which involves such an integral.)

Can you access a copy of Greiner & Reinhardt? They explain quite a bit more detail than what's in Tong's notes -- far more than I can reasonably reproduce in a PF post.

• vanhees71
=(ω0i[−Tμ0xi+Tμix0])+(ωij[−Tμixj+Tμjxi]), for i<j in the third and fourth terms

=(ωρσ[−Tμρxσ+Tμσxρ]), for

How did you get to the last line from the previous line?