A How can I take the derivative?

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The action considered is \begin{align*}
S[\Phi] = \int_M dt d^3 x \sqrt{-g} \left( -\frac{1}{2}g^{ab} \partial_a \Phi \partial_b \Phi - \frac{1}{2}m^2 \Phi^2\right)
\end{align*}I can "see" unrigorously that variation with respect to ##\partial_t \Phi(x)## it is going to be\begin{align*}
\frac{\delta S}{\delta(\partial_t \Phi(x))} &= -\frac{1}{2}\sqrt{-g} g^{ab} \frac{\delta}{\delta(\partial_t \Phi(x))} \left( \partial_a \Phi \partial_b \Phi \right) \\

&= -\frac{1}{2}\sqrt{-g} g^{ab} \cdot 2 \partial_a \Phi \delta^t_b \\

&= -\sqrt{-g} g^{at} \partial_a \Phi \\

&= \sqrt{h} n^{a} \partial_a \Phi
\end{align*}How do I do this calculation properly? For instance to find the functional variation with respect to ##\Phi## I could consider ##\lim_{\epsilon \rightarrow 0} \frac{1}{\epsilon}\left( S[\Phi + \epsilon \alpha] - S[\Phi] \right)##. But how do I write it when considering the functional derivative of ##S## with respect to ##\partial_t \Phi##; do I let the action have a second argument ##S = S[\Phi, \partial_a \Phi]## and proceed from there?
 
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Why do you need such a strange derivative? I don't really see how such a derivative would be defined, maybe if you give me some more context I can help
 
##(M, g_{ab})## is a globally hyperbolic spacetime and the metric is here written ##ds^2 = -N^2 dt^2 + h_{ij} (dx^i + N^i dt)(dx^j + N^j dt)## with ##t## a global time coordinate labelling the cauchy surfaces ##\Sigma_t## of normal ##-N(dt)_a## and induced metric ##h_{ab}##, such that ##\sqrt{-g} = N\sqrt{h}##.

The aim is to find the canonical momentum ##\Pi(x)## conjugate to ##\Phi## by varying ##S## with respect to ##\partial_t \Phi(x)##
 
Ok, usually when one has an action of the form
$$S = \int \mathscr{L}(\Phi, \partial_\mu \Phi, t) d^4 x$$
the canonical momentum is defined as
$$\Pi(x)=\frac{\partial \mathscr{L}(\Phi, \partial_\mu \Phi, t)}{\partial(\partial_0\Phi)}$$
This one is almost immediate to compute and indeed gives the answer you have in #1. But, otherwise, I don't know how one is supposed to define something like
$$\frac{\delta S[\Phi]}{\delta (\partial_0 \Phi)}$$
At first, something like that seems nonsensical to me, but maybe there's a way to properly define such a thing...
 
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Yeah, it's a bit strange. Landau & Lifshitz explained similar sorts of things, e.g. varying the action with respect to the co-ordinates (i.e. considering only admissible trajectories between ##a \longrightarrow b## and keeping ##(\delta x^i)_a = 0## but ##(\delta x^i)_b## variable) then you can show that$$\delta S = -mcu_i \delta x^i \implies p_i = - \frac{\partial S}{\partial x^i}$$so the time-component of the momentum four-vector would just be ##p_t = - \partial S / \partial t##.

I figured the motivation for ##\Pi(x) = \delta S / \delta (\partial_t \Phi)## in the OP would be analogous to that but I don't know how to formalise that at all. I don't know any field theory, really :frown:
 
Indeed, now that I think about it, since functional derivatives have the chain rule, maybe we can write it like
$$\frac{\delta S[\Phi]}{\delta (\partial_0 \Phi)} = \frac{\delta S[\Phi]}{\delta \Phi}\frac{\delta \Phi}{\delta (\partial_0 \Phi)}$$
Then the first derivative is the usual one that is used to derive E-L equations, the problem is the second term.
We know that $$\frac{\delta (\partial_0 \Phi)(y)}{\delta \Phi(x)}=-\partial_0 \delta^{(4)}(x-y),$$ but I don't know if there exists a property for functional derivatives that allow us to invert this, similar to normal derivatives.
 
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I asked a question here, probably over 15 years ago on entanglement and I appreciated the thoughtful answers I received back then. The intervening years haven't made me any more knowledgeable in physics, so forgive my naïveté ! If a have a piece of paper in an area of high gravity, lets say near a black hole, and I draw a triangle on this paper and 'measure' the angles of the triangle, will they add to 180 degrees? How about if I'm looking at this paper outside of the (reasonable)...
From $$0 = \delta(g^{\alpha\mu}g_{\mu\nu}) = g^{\alpha\mu} \delta g_{\mu\nu} + g_{\mu\nu} \delta g^{\alpha\mu}$$ we have $$g^{\alpha\mu} \delta g_{\mu\nu} = -g_{\mu\nu} \delta g^{\alpha\mu} \,\, . $$ Multiply both sides by ##g_{\alpha\beta}## to get $$\delta g_{\beta\nu} = -g_{\alpha\beta} g_{\mu\nu} \delta g^{\alpha\mu} \qquad(*)$$ (This is Dirac's eq. (26.9) in "GTR".) On the other hand, the variation ##\delta g^{\alpha\mu} = \bar{g}^{\alpha\mu} - g^{\alpha\mu}## should be a tensor...

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