General Case
The action functional in ordinary spacetime looks like the one from classical physics:
<br />
\mathcal{S}[\phi] = \int d^4x \, \mathcal{L}[\phi, \partial_\mu \phi; x^\mu] \, \quad \mapsto<br />
\quad S = \int dt \, L(q(t), \dot{q(t)}; t) \, .<br />
The most general way to write \delta \mathcal{S} -- without imposing any symmetries -- is to just vary the Lagrangian with respect to the field(s) \phi,
its derivative \partial_\mu \phi, and the coordinates x^\mu:
<br />
\delta \mathcal{S} = \int \delta \phi \frac{\partial \mathcal{L}}{\partial \phi} <br />
+ \delta(\partial_\mu \phi) \frac{\partial \mathcal{L}}{\partial (\partial_\mu \phi)}<br />
+ \delta x^\mu \frac{\partial \mathcal{L}}{\partial x^\mu} \, .<br />
If you are dealing with global Poincare invariance, the variation with respect to the coordinates vanishes. Have you dealt with
<br />
\mathcal{L} = \frac{1}{2} |\partial_\mu \phi|^2 + \frac{1}{2}m^2 \phi^2<br /> yet?