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This is a question which wants us to find the variation of the action for the free scalar field under the field transformation

$\phi(x) \mapsto \phi’(x) = \phi(x) - a(x)\partial_\mu\phi(x)$

Deduce the Ward identities generated by translation invariance.

So the solution goes:

$x \mapsto x’^\mu = x^\mu + a^\mu$

$ \phi(x) \mapsto \phi’(x’) = \phi(x)$

$a^\mu = \epsilon \delta^{\mu\rho}$

$\phi’(x) = \phi(x-a) = \phi(x) - a^\mu\partial_\mu\phi(x) = \phi(x) - \epsilon\partial_\rho\phi(x)$

I am struggling to understand the last term on the RHS with $\epsilon\partial_\rho\phi(x)$.

How do we get from $a^\mu\partial_\mu\phi(x)$ to $\epsilon\partial_\rho\phi(x)$.

Any comments would be greatly appreciated.

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1 Answer 1

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It is just simple: substituting $a^\mu = \epsilon \delta^{\mu\rho}$, $a^{\mu}\partial_\mu \phi(x) = \epsilon \delta^{\mu\rho}\partial_\mu \phi(x) = \epsilon \partial^\rho \phi(x)$. Recall that we are using Einstein convention for the $\mu$-contraction with the Kronecker delta $\delta^{\mu\rho}$: \begin{align} \sum_{\mu} \delta^{\mu\rho} \partial_\mu = \sum_{\mu} \big(\text{1 if $\mu=\rho$, 0 otherwise}\big) \partial_\mu = \partial_\mu \,. \end{align}

By the way, I would like to say that the index notation here is somewhat sloppy, treating the index $\rho$ as a fixed number or otherwise a "dangling pointer." I suppose writing down equations just by $a^\mu$ (assumed infinitesimal) will be fine.

[Additional comments: there's no such thing as "$\delta^{\mu\rho}$", if you are not assuming Euclidean spacetime and have the inverse Euclidean metric $g^{\mu\nu} = \delta^{\mu\nu}$. Only $\delta^\mu{}_\nu$ is the "true" Kronecker delta: the identity map on tangent spaces. I recommend $a^\mu = \delta^\mu{}_\rho \epsilon^\rho$ or, allowing some sloppiness, at least $a^\mu = \epsilon\delta^\mu{}_\rho$.]

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  • $\begingroup$ Thanks so much, you are right about the indices on the Kronecker delta. Seems like a typo by the author. Cheers $\endgroup$
    – Han
    Commented Nov 2, 2021 at 0:56

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