Equation of motion from the action

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Discussion Overview

The discussion revolves around deriving the equations of motion from a specific action in the context of general relativity and gauge theory. Participants explore the appropriate methods for variation and the implications of different formulations of the action, particularly focusing on the relationship between the fields and their derivatives.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning
  • Homework-related

Main Points Raised

  • Emilie presents a complex action and expresses difficulty in deriving the corresponding equations of motion using the Euler-Lagrange equation.
  • Some participants suggest that the fundamental fields are not the ##F^I## fields but rather the ##A^I## potentials, indicating that variation should be performed with respect to ##A^I##.
  • There is a contention regarding the validity of varying the action with respect to ##F^I## when ##A## is not explicitly present in the action.
  • Participants discuss the nature of the equations of motion, with some clarifying that "algebraic" equations imply a lack of derivatives, which leads to a different form than expected.
  • Emilie shares her attempts to derive the equations of motion and expresses confusion over the results, particularly regarding the dual field ##\tilde{F}##.
  • There are suggestions to simplify the problem by starting with a more basic action to understand the derivation process better.
  • Questions arise about the appropriateness of the action Emilie is working with, considering her stated level of study in physics.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the correct approach to deriving the equations of motion from the given action. There are competing views on whether to vary with respect to ##F^I## or ##A^I##, and the implications of these choices remain unresolved.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about the fields involved, the definitions of the terms in the action, and the mathematical steps required to derive the equations of motion. Some participants suggest that the complexity of the action may not align with Emilie's current level of study.

Who May Find This Useful

This discussion may be useful for students and practitioners interested in the derivation of equations of motion in the context of gauge theories and general relativity, particularly those exploring the relationship between actions and field equations.

Emilie.Jung
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Hello Physics Forums!

Supposing that we have an action that says:
$$L=\frac{1}{2}R-g_{C\bar{D}}\partial_{\mu}z^C\partial^{\mu}\bar{z}^D+\frac{1}{4} + \frac{1}{4}ImM_{IJ}F^I_{\mu\nu}\cdot F^{J\mu\nu} +\frac{1}{4}ReM_{IJ}F^I_{\mu\nu}\cdot \tilde{F}^{J\mu\nu}$$
where $$\tilde{F}^I_{\mu\nu}=\frac{1}{2}\epsilon_{\mu\nu}^{\mu'\nu'}F^I_{\mu'\nu'}$$
If I want to find the equation of motion of this, I know I can start from action and use the Euler Lagrange equation or directly use d*F=0 (Maxwell's equation).

This is one of the very rare times where I encounter general relativity as I am still a second year physics student. I have seen this sort of action (but way simpler) in my classical mechanics course) where we almost always use the Euler-Lagrange equation or vary the action with respect to the functional term and set it equal to zero and VOILA! you get the equation of motion you need. Here though I am finding a little of difficulty. The thing is that what was found for this action was the following answer:
$$d(ReM_{IJ}F^J+ImM_{IJ}\tilde{F}^J)=0.$$
I have tried so manyy ways to derive this but failed at it.

First, I tried to do it in the general way thinking I would avoid mistakes so I started by transforming the ##\tilde{F}^{\mu\nu}## to ##\frac{1}{2}\epsilon^{\rho\sigma\mu\nu}F_{\rho\sigma}## to get rid of the tilde and then deriving the action with respect to ##F^{\kappa\lambda}## and then set it equal to zero. BUT the procedure seems to take forever and I am not getting the answer above(It is too long I couldn't write it down, but if it matters I could type few of the details). I guess there is a better track to take, but I have no idea what it might be. On some websites, I found that instead of ##\partial^{\mu}F_{\mu\nu}## that we usually use in Classical Mechanics, there is now a G term, for example they write the maxwell equation as ##\partial^{\mu}G_{\mu\nu}## or something like that. You might relate to this better than I am. I am only trying to tell you what I have searched for before finally creating an account on this forum.

I am trying to practice those from the web in a spontaneous manner as my professor said she will bring us a bonus part in the coming exam that has to do with general relativity after she taught us a little of einstein indices operations. I know she might not bring this tough level but I am curious to know how things work in General Relativity and why if I followed the very classical way, I am not getting the answer above for the equation of motion? Any advice will be useful.

Yours,
Emilie.
 
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The ##F^I## are not the fundamental fields. Presumably they are given by ##F^I \equiv d A^I##. You need to vary the action with respect to the ##A^I##, not the ##F^I##.
 
But I know that if A is not explicitly shown in the action, I can just go ahead and vary the action with respect to the F. Is this wrong?
 
Emilie.Jung said:
But I know that if A is not explicitly shown in the action, I can just go ahead and vary the action with respect to the F. Is this wrong?

Very wrong. For one, no derivatives of F appear in the action, so you'll just get algebraic equations of motion that way.
 
What do you mean by "algebraic"equations of motion? Does this mean, I get this form ##d(ReM_{IJ}F^J+ImM_{IJ}\tilde{F}^J)=0##? Is this the algebraic form? Because this is all I need.
 
Emilie.Jung said:
What do you mean by "algebraic"equations of motion?

I mean the EoM won't have any derivatives in them, and there are no dynamics.

Does this mean, I get this form ##d(ReM_{IJ}F^J+ImM_{IJ}\tilde{F}^J)=0##? Is this the algebraic form? Because this is all I need.

No, because ##d## is a derivative.

Try something simpler first, like this:

$$S = -\frac14 \int F_{\mu\nu} F^{\mu\nu} \, d^4x, \qquad F \equiv d A.$$
You should be able to obtain

$$d \star F = 0$$
 
I will present what I did here:

$$S=-\frac{1}{4}\int{F_{\mu\nu}F^{\mu\nu}d^4x}$$
$$=-\frac{1}{4}\int{\delta F_{\mu\nu}F^{\mu\nu}d^4x+F_{\mu\nu}\delta F^{\mu\nu}d^x}$$
$$=-\frac{1}{4}\int{\delta(\partial_{\mu}A_{\nu}-\partial_{\nu}A_{\mu})F^{\mu\nu}d^4x+F_{\mu\nu}\delta(\partial^{\mu}A^{\nu}-\partial^{\nu}A^{\mu})d^4x}$$
I then expand terms,
$$=-\frac{1}{4}\int{(\partial_{\mu}\delta A_{\nu}F^{\mu\nu}-\partial_{\mu}\delta A_{\nu}F^{\nu\mu}+F_{\mu\nu}\partial^{\mu}g^{\nu\nu}\delta A_{\nu} -g^{\nu\nu}F_{\nu\mu}\partial^{\mu}\delta A_{\nu})d^4x}$$
$$=-\frac{1}{2}\int{(F^{\mu\nu}\partial_{\mu}+F^{\mu\nu}\partial_{\mu})\delta A_{\nu}}$$
setting this equal to zero, I get
$$F^{\mu\nu}\partial_{\mu}+F^{\mu\nu}\partial_{\mu}=0$$
where I do not get
$$d*F=0$$
Maybe I did a mistake somewhere.. @Ben Niehoff
 
Emilie.Jung said:
I will present what I did here:

$$S=-\frac{1}{4}\int{F_{\mu\nu}F^{\mu\nu}d^4x}$$
$$=-\frac{1}{4}\int{\delta F_{\mu\nu}F^{\mu\nu}d^4x+F_{\mu\nu}\delta F^{\mu\nu}d^x}$$
$$=-\frac{1}{4}\int{\delta(\partial_{\mu}A_{\nu}-\partial_{\nu}A_{\mu})F^{\mu\nu}d^4x+F_{\mu\nu}\delta(\partial^{\mu}A^{\nu}-\partial^{\nu}A^{\mu})d^4x}$$
I then expand terms,
$$=-\frac{1}{4}\int{(\partial_{\mu}\delta A_{\nu}F^{\mu\nu}-\partial_{\mu}\delta A_{\nu}F^{\nu\mu}+F_{\mu\nu}\partial^{\mu}g^{\nu\nu}\delta A_{\nu} -g^{\nu\nu}F_{\nu\mu}\partial^{\mu}\delta A_{\nu})d^4x}$$
$$=-\frac{1}{2}\int{(F^{\mu\nu}\partial_{\mu}+F^{\mu\nu}\partial_{\mu})\delta A_{\nu}}$$

At this point, you need to integrate by parts, so that ##\delta A_\mu## appears without any derivatives acting on it
 
Oh, then:
$$-\frac{1}{2}\int{2F^{\mu\nu}\partial_{\mu}\delta A_{nu}}$$
$$=-\int{F^{\mu\nu}\partial_{\mu}\delta A_{\nu}}$$
integration by parts
$$-F^{\mu\nu}\delta A_{\nu}+\int{\partial_{\mu}F^{\mu\nu}\delta A_{\nu}}$$
first terms goes away, and we set the second equal to zero to get
$$\partial_{\mu}F^{\mu\nu}=0$$
I am afraid I am not getting the dual of F here.. @Ben Niehoff
 
  • #10
I don't suppose you considered writing out ##d \star F## in indices...
 
  • #11
Sorry I don't know what you mean. As I have mentioned, I am a second year student and haven't really taken a course in General Relativity. If you may explain more by what you mean? @Ben Niehoff
 
  • #12
Is this a homework problem? If you haven't done any GR, then how did you end up with an action for supergravity?
 
  • #13
No this is not a homework. I am practicing different actions from the web in order to be prepared from my exam that will have a bonus question in my advanced classical mechanics course related to those (I mentioned this in my question). This I picked from an arxiv paper. In any case, I am solving a problem you set for me with an action different than the one I presented in my question, isn't this right? @Ben Niehoff
 

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