Expanding delta in Field Theory Derivation of Euler-Lagrange Equations

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The forum discussion focuses on the derivation of the Euler-Lagrange Equations in classical field theory as presented in Peskin & Schroeder's text. The key equation discussed is the manipulation of the term involving the Lagrangian density, specifically the expression \(\frac{∂L}{∂(∂_{μ}\phi)} δ(∂_{μ}\phi)\). The user seeks clarification on extracting terms within the delta function, leading to an explanation of how variations in the field \(\phi\) relate to changes in derivatives of \(\phi\). The discussion emphasizes the application of the product rule in calculus to rearrange terms effectively.

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  • Familiarity with Lagrangian densities and their notation
  • Basic calculus, specifically the product rule for derivatives
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  • Study the derivation of the Euler-Lagrange Equations in Peskin & Schroeder, focusing on section 2.2
  • Learn about the properties of delta functions in the context of field theory
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chuchi
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Every time I try to read Peskin & Schroeder I run into a brick wall on page 15 (section 2.2) when they quickly derive the Euler-Lagrange Equations in classical field theory. The relevant step is this:

\frac{∂L}{∂(∂_{μ}\phi)} δ(∂_{μ}\phi)

= -∂_{μ}( \frac{∂L}{∂(∂_{μ}\phi)}) δ(\phi) + ∂_{μ} (\frac{∂L}{∂(∂_{μ}\phi)} δ(\phi))

How can we even extract anything within that delta? How does that even work? I feel like I'm missing some basic calculus here, but can't find anything in my textbooks or google.

(those "L"s are supposed to be Lagrangian densities, I just don't know the curly script for L in latex. all of this is inside an integral and there's another term, but neither of those change. I also posted to calculus but no one knew enough.)
 
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I don't understand what you're asking, but here's what's going on.

First of all, for the purposes of this equation, we don't need any properties of \frac{∂L}{∂(∂_{μ}\phi)}, so I will just call it V^\mu.

Now, the meaning of \delta X, where X is anything that depends on the field \phi, is this: we take the field \phi(x) and replace it with \phi(x)+\delta\phi(x), where \delta\phi(x) is "small". Then X becomes X+\delta X, and we have to work out what \delta X is in terms of \delta\phi.

For your equation, we take X=\partial_\mu\phi(x). Now this is very simple: \delta X=\partial_\mu\delta\phi. Stare at that until you are sure you understand it.

The next important fact is that what I am calling \delta X for X=\partial_\mu\phi is what P&S call \delta(\partial_\mu\phi).

The rest is trivial calculus. By the product rule for derivatives, \partial_\mu(V^\mu\delta\phi)=(\partial_\mu V^\mu)\delta\phi+V^\mu(\partial_\mu\delta\phi). Rearrange that to get your equation.
 
Last edited:
Adding a small thing: it's \mathcal{L} that produces \mathcal{L} to denote either the Lorentz group, or the Lagrangian density.
 

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