EoM from action, indices confused, (QFT)

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Homework Help Overview

The discussion revolves around deriving the equations of motion (EoM) from the action using the Euler-Lagrange (E-L) equations in the context of quantum field theory (QFT). Participants are examining the implications of various terms in the Lagrangian, particularly focusing on the correct treatment of indices and the notation used in expressing derivatives of fields.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants are attempting to clarify the correct form of the E-L equations and the treatment of terms involving derivatives of fields. There is confusion regarding the notation used for the kinetic term and how it relates to the indices involved. Questions arise about the implications of treating covariant and contravariant indices, as well as the role of the metric in these expressions.

Discussion Status

The discussion is ongoing, with participants providing insights and questioning each other's reasoning. Some have offered clarifications regarding the notation and the treatment of indices, while others express uncertainty about specific derivative terms and their implications in the context of the E-L equations. There is no explicit consensus yet, but productive dialogue is occurring.

Contextual Notes

Participants are navigating the complexities of field theory notation and the implications of different types of fields (real vs. complex) on the presence of factors such as 1/2 in the Lagrangian. The discussion also touches on the assumptions made when working in Minkowski space versus curved backgrounds.

binbagsss
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Homework Statement



Using the E-L equations to get the EoM from the action.


Homework Equations



I am using E-L equations in the form:

## \frac{\partial}{\partial_u} \frac{\partial L}{\partial_u \phi}-\frac{\partial L}{\partial \phi} ##

where ##L ## is the Lagrangian

The Attempt at a Solution



I am a bit confused with the term ## \frac{1}{2} \partial_u \phi \partial^u \phi ## of a lot of actions.

The correct answer is ## \frac{1}{2} \partial_u \partial^u \phi ##

As it is for the first term of the EoM from [1] I get:

## \frac{\partial}{\partial_u} \frac{1}{2} \partial^u \phi = \frac{1}{2}\partial_u \partial^u \phi ##

However if I write it as ##\frac{1}{2}(\partial_u \phi)^2 ## , the factor of half cancels, but my indices don't work out :

## \frac{\partial}{\partial_u} \partial_u \phi = \partial_u \partial_u \phi ##Many thanks
 
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Writing it as ##(\partial_u \phi)^2/2## is a bastard notation often used in physics. At face value you might think it means what you are taking it to mean, but what it really means is ##g^{ab}(\partial_a\phi)(\partial_b \phi)/2##.
 
Orodruin said:
Writing it as ##(\partial_u \phi)^2/2## is a bastard notation often used in physics. At face value you might think it means what you are taking it to mean, but what it really means is ##g^{ab}(\partial_a\phi)(\partial_b \phi)/2##.
i don't understand the differnce, the metric in your expression raises the index to get the same expression, no?
 
Yes, the point being that the expression ##(\partial_a \phi)^2## while seemingly containing two covariant indices really contains a contraction between a covariant and a contravariant index and needs to be treated as such.
 
Orodruin said:
Yes, the point being that the expression ##(\partial_a \phi)^2## while seemingly containing two covariant indices really contains a contraction between a covariant and a contravariant index and needs to be treated as such.
oh so as in when i differentiate what i have done is treated them as separate indices but i need to apply some sort of chain rule instead?
 
Right. ##\partial^a\phi## is not indepentent from ##\partial_a\phi##.
 
binbagsss said:
linked via the metric, so i need to differentiate the metric wrt x?
You mean when you take the derivative ##\partial_u## of ##\partial L/\partial(\partial_u\phi)##? In general yes, but in most cases QFT is done on a Minkowski space background meaning that that term vanishes. In a curved background (or in curvilinear coordinates) you will generally not obtain ##\partial_a\partial^a\phi =0## but ##\nabla_a\partial^a\phi =0##, which is fortunate since the first expression is not invariant whereas the second is.
 
Orodruin said:
You mean when you take the derivative ##\partial_u## of ##\partial L/\partial(\partial_u\phi)##? In general yes, but in most cases QFT is done on a Minkowski space background meaning that that term vanishes. .

so looking at the OP, what is the term coming from the chain rule I am missing that you have hinted at.
From the above discussion all I have is:

##\frac{1}{2} \partial_u (g^{ua} \partial_{a} \phi )
=\frac{1}{2} ( g^{ua} \partial_u \partial_{a} \phi + \partial_{a} \phi \partial_u g^{ua} ) ##

this is equal to what I had previously , sincce the 2nd term is zero...

Please can I have more guidance,

thanks
 
Why do you still have the 1/2?
 
  • #10
Also I am not sure I understand what you think the problem is ...
 
  • #11
Orodruin said:
Why do you still have the 1/2?

becuse in genreal the action will include other terms such as ## m^2 \phi ^2 + \lambda \frac{\phi}{4!} ## i.e ##\frac{\partial L}{\partial \phi } \neq 0 ##
 
  • #12
Are you dealing with a complex scalar field or a real scalar field? The 1/2 should disappear in the case of a real scalar field because you have two derivative terms. In the case of a complex field you do not have the factor of 1/2 from the beginning. In the case of a real scalar field, the mass term also comes with a 1/2.
 
  • #13
Orodruin said:
Are you dealing with a complex scalar field or a real scalar field? The 1/2 should disappear in the case of a real scalar field because you have two derivative terms. In the case of a complex field you do not have the factor of 1/2 from the beginning. In the case of a real scalar field, the mass term also comes with a 1/2.
yep the m^2 term comes with a half.
no i mean I am stil struggling with this derivative term.

ok so I want ## \frac{\partial }{\partial_u} (\partial_u \phi \partial^u \phi) = \frac{\partial }{\partial_u} (\partial_u \phi g^{au} \partial_a \phi)= g^{au}\partial_a \phi (1) + g^{au}\partial_u \phi \frac{\partial}{\partial_u \phi} (\partial_a \phi) + 0 ##

using the product rule

for the 2nd term I get ## \frac{\partial}{\partial_u \phi} (\partial_a \phi) =\delta^{au} ##

this must be wrong since this then gives me a factor of ##4## via the trace of the metric and so the index is not raised as required also.
 
  • #14
binbagsss said:
yep the m^2 term comes with a half.
no i mean I am stil struggling with this derivative term.

ok so I want ## \frac{\partial }{\partial_u} (\partial_u \phi \partial^u \phi) = \frac{\partial }{\partial_u} (\partial_u \phi g^{au} \partial_a \phi)= g^{au}\partial_a \phi (1) + g^{au}\partial_u \phi \frac{\partial}{\partial_u \phi} (\partial_a \phi) + 0 ##

using the product rule

for the 2nd term I get ## \frac{\partial}{\partial_u \phi} (\partial_a \phi) =\delta^{au} ##

this must be wrong since this then gives me a factor of ##4## via the trace of the metric and so the index is not raised as required also.
please can somebody help with my working here, is the delta term wrong? thanks
 
  • #15
You're using very confusing notation, which I think is the reason people are not responding. I fix your notation and get

## \frac{\partial }{\partial_c} (\partial_b \phi \partial^b \phi) = \partial_c \Bigl(\eta^{ab} \partial_a \phi \partial_b \phi \Bigr) = \eta^{ab} \Bigl( (\partial_c \partial_a) \phi \partial_b \phi + \partial_a \phi ( \partial_c \partial _b \phi ) \Bigr) = \Bigl( (\partial_c \partial_a) \phi \partial^a \phi + \partial^a \phi ( \partial_c \partial_a \phi ) \Bigr)##

This equals

## 2 \Bigl( (\partial_c \partial_a) \phi \partial^a \phi \Bigr)##
 
  • #16
binbagsss said:
ok so I want ## \frac{\partial }{\partial_u} (\partial_u \phi \partial^u \phi) = \frac{\partial }{\partial_u} (\partial_u \phi g^{au} \partial_a \phi)= g^{au}\partial_a \phi (1) + g^{au}\partial_u \phi \frac{\partial}{\partial_u \phi} (\partial_a \phi) + 0 ##

Why do you want that? The Euler-Lagrange equations of motion are:

\partial_u \frac{\partial \mathcal{L}}{\partial (\partial_u \phi)} = \frac{\partial \mathcal{L}}{\partial \phi}

But \frac{\partial \mathcal{L}}{\partial (\partial_u \phi)} = \partial^u \phi (assuming \mathcal{L} = \frac{1}{2} \partial_u \phi \partial^u \phi + terms involving powers of \phi)

So unless you have a strange Lagrangian, you shouldn't have to compute \partial_u (\partial_v \phi \partial^v \phi)
 
  • #17
stevendaryl said:
Why do you want that? The Euler-Lagrange equations of motion are:

\partial_u \frac{\partial \mathcal{L}}{\partial (\partial_u \phi)} = \frac{\partial \mathcal{L}}{\partial \phi}

But \frac{\partial \mathcal{L}}{\partial (\partial_u \phi)} = \partial^u \phi (assuming \mathcal{L} = \frac{1}{2} \partial_u \phi \partial^u \phi + terms involving powers of \phi)

So unless you have a strange Lagrangian, you shouldn't have to compute \partial_u (\partial_v \phi \partial^v \phi)
okay well I was trying to incrorporate Oroduin's hints since, as said in the OP, i can't get rid of the factor of 1/2 in the derivative term.

To give a specfic example if I consider: ##-1/2 \partial_u \phi \partial^u \phi - 1/2 m^2 \phi^2 ##
then, my previous method, before making this thread was:
##\frac{\partial L}{\partial \phi}= m^2 \phi##
##\frac{\partial L}{\partial_u \phi}= \partial^u \phi (-1/2) ##

therefore yielding ## \partial_u \frac{\partial L}{\partial_u \phi} - \frac{\partial L}{\partial \phi} = -1/2 \partial^u\partial_u \phi + m^2 \phi ##
whereas the EoM is : ## \partial^u \partial_u \phi -m^2 \phi^2 ##

But now, trying to use Oroduin's hint I rewrite as ## L=-1/2 \partial_u \phi g^{au} \partial_a \phi +m^2term... ##
Now looking at the derivative term I get ## \frac{\partial L}{\partial_u \phi} = =-1/2g^{au} ( \partial_a \phi \frac{\partial}{\partial_u \phi}(\partial_u \phi) + \partial_u \phi \frac{\partial}{\partial_u \phi}(\partial_a \phi))=-1/2 g^{au} ( \partial_a \phi (1) + \partial_u \phi \delta_{au}) ##
where I have used the product rule, and taken out the metric since it is the minkoski...

##= -1/2 (\partial^u \phi + g^{uu}\partial_u \phi) ##...
 
Last edited:
  • #18
binbagsss said:
okay well I was trying to incrorporate Oroduin's hints since, as said in the OP, i can't get rid of the factor of 1/2 in the derivative term.

To give a specfic example if I consider: ##-1/2 \partial_u \phi \partial^u \phi - 1/2 m^2 \phi^2 ##
then, my previous method, before making this thread was:
##\frac{\partial L}{\partial \phi}= m^2 \phi##
##\frac{\partial L}{\partial_u \phi}= \partial^u \phi (-1/2) ##

therefore yielding ## \partial_u \frac{\partial L}{\partial_u \phi} - \frac{\partial L}{\partial \phi} = -1/2 \partial^u\partial_u \phi + m^2 \phi ##
whereas the EoM is :

But now, trying to use Oroduin's hint I rewrite as ## L=-1/2 \partial_u \phi g^{au} \partial_a \phi +m^2... ##
Now looking at the derivative term I get ## \frac{\partial L}{\partial \phi} = =-1/2g^{au} ( \partial_a \phi \frac{\partial}{\partial_u \phi}(\partial_u \phi) + \partial_u \phi \frac{\partial}{\partial_u \phi}(\partial_a \phi))=-1/2 g^{au} ( \partial_a \ phi (1) + \partial_u \delta_{au} ##
where I have used the product rule, and taken out the metric since it is the minkoski...

##= -1/2 (\partial^u + g^{aa}\partial_a) ##...

You have to be careful about indices. If you look at just the term \frac{1}{2} g^{au} (\partial_a \phi) (\partial_u \phi) and you take a derivative with respect to \partial_u \phi, you have to realize that in \frac{1}{2} g^{au} (\partial_a \phi) (\partial_u \phi), u is a dummy index. You can replace it by v, say. So you have:

\frac{\partial}{\partial(\partial_u \phi)} \frac{1}{2} g^{av} (\partial_a \phi) (\partial_v \phi)Now, \frac{\partial}{\partial(\partial_u \phi)} (\partial_a \phi) = 0 unless a=u. So we can summarize it as:

\frac{\partial}{\partial(\partial_u \phi)} (\partial_a \phi) = \delta^u_a

Similarly,

\frac{\partial}{\partial(\partial_u \phi)} (\partial_v \phi) = \delta^u_v

So using the product rule gives you:

\frac{\partial}{\partial(\partial_u \phi)} \frac{1}{2} g^{av} (\partial_a \phi) (\partial_v \phi) = \frac{1}{2} g^{av} (\delta^u_a \partial_v \phi + \delta^u_v \partial_a \phi)

Then we can use g^{av} \delta^u_a = g^{uv} \delta^u_a. Summing over a gives g^{uv}. Similarly, g^{av} \delta^u_v = g^{au} \delta^u_v. Summing over v gives g^{au}. So this simplifies to:\frac{1}{2} (g^{uv} \partial_v \phi + g^{au} \partial_a \phi)

Those two terms are the same, since a and v are dummies and g^{au} = g^{ua}. So we have:
g^{uv} \partial_v \phi

The EoM are just:

\partial_u (g^{uv} \partial_v \phi) = \pm m^2 \phi

(I don't remember whether the right side is a + or a -)
 
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  • #19
stevendaryl said:
The EoM are just:
\partial_u (g^{uv} \partial_v \phi) = \pm m^2 \phi

In flat spacetime, you can take the g^{uv} outside the derivative.
 

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