Lorentz transformation for derivatives

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Discussion Overview

The discussion revolves around the Lorentz transformation of derivatives in the context of quantum field theory (QFT). Participants explore how derivatives of scalar fields transform under Lorentz transformations, including the implications for tensor notation and the use of the metric tensor.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions how to transform partial derivatives when a scalar field is transformed under Lorentz transformations, specifically whether ##\frac {\partial} {\partial x ^{\mu}}## should change to ##\frac {\partial} {\partial y ^{\mu}}##.
  • Another participant provides an example using specific transformations of time and space coordinates to illustrate how the derivatives of the field relate to the transformed coordinates.
  • A participant expresses confusion regarding the equations in David Tong's notes and finds clarity after rewriting them, concluding that the transformation of derivatives follows from the chain rule and the transformation properties of coordinates.
  • Several participants discuss the calculation of derivatives in tensor forms, providing specific equations and seeking validation for their results.
  • One participant acknowledges the utility of the derivatives they calculated but expresses uncertainty about their correctness and seeks further information.
  • Another participant discusses the implications of using the metric tensor in QFT, questioning its importance in certain contexts while acknowledging the need for proper index notation.
  • There are corrections made to earlier equations, with participants acknowledging mistakes and refining their understanding of the relationships between different tensor forms.

Areas of Agreement / Disagreement

Participants show varying levels of agreement on the transformation of derivatives, with some expressing confidence in their calculations while others remain uncertain. The discussion includes corrections and refinements, indicating that consensus on certain points is still developing.

Contextual Notes

Some participants note that the transformations and calculations depend on the proper use of the metric tensor and the conventions of raising and lowering indices, which may not be universally agreed upon in all contexts.

Who May Find This Useful

Readers interested in quantum field theory, Lorentz transformations, tensor calculus, and the mathematical foundations of physics may find this discussion relevant.

Haorong Wu
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TL;DR
should ##\frac {\partial} {\partial x ^{\mu}}## transform to ##\frac {\partial} {\partial y ^{\mu}}## or remain unchanged?
Hello again. I am sorry I got another problem when learning QFT regarding the Lorentz transformation of derivatives.

In David Tong's notes, he says
Consider a real scalar field transformed as ##\phi \left ( x \right ) \rightarrow \phi ^{'} \left ( x \right ) =\phi \left ( \Lambda ^{-1 }x \right )##.

Then the derivative of the scalar field transforms as a vector, meaning
##\left ( \partial _{\mu} \phi \right ) \left ( x \right ) \rightarrow \left ( \Lambda ^{-1 }\right ) ^{\nu} {}_{\mu} \left ( \partial _{\nu} \phi \right ) \left ( y \right )## where ##y=\Lambda ^{-1 }x ##

I am not sure how to transform the partial derivatives. Explicitly, should ##\frac {\partial} {\partial x ^{\mu}}## transform to ##\frac {\partial} {\partial y ^{\mu}}## or remain unchanged? And why?

At first, I think since ##x## is transformed to ##y##, then ##\partial x^\mu## should transform to ##\partial y^\mu## as well. However, after I tried the calculation, I found that, the derivative does not transform and it is still ##\partial x^\mu##. I could not find a proper explanation to convince myself.
 
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Let's take an example:
$$t = \gamma(t' + vx'), \ \ \ x = \gamma(x' + vt')$$
We need the value of the field at the transformed coordinates to be the same physical value as the original field at the original coordinates. Hence:
$$\phi'(t', x') = \phi(t, x) = \phi(\gamma(t' + vx'), \gamma(x' + vt'))$$
Now the derivatives of the field are:
$$\frac{\partial\phi'(t', x')}{\partial t'} = \frac{\partial\phi(\gamma(t' + vx'), \gamma(x' + vt'))}{\partial t'} = \frac{\partial\phi(t, x)}{\partial t}\gamma + \frac{\partial\phi(t, x)}{\partial x}\gamma v$$
Hence:
$$\frac{\partial\phi'(t', x')}{\partial t'} = \gamma \frac{\partial\phi(t, x)}{\partial t} + \gamma v\frac{\partial\phi(t, x)}{\partial x}$$
Now, you just have to generalise that using ##\Lambda## and upper and lower indices on the spacetime coordinates.
 
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Thank you very much, @PeroK !I never think it in this way,especially your equation ##\phi'(t', x') = \phi(t, x) ## guide me through the problem. I also learn from them that ##\partial _ \mu \phi^{'}## means ##\frac {\partial \phi \left ( y \right )} {\partial y^\mu}##.

I think the equations in David Tong's note are somehow confusing. After I rewrite it , everything works out.

Let ##\phi \left ( x \right ) \rightarrow \phi ^{'} \left ( x^{'} \right ) =\phi \left ( x \right )## where ##x^{'}=\Lambda x##. Then
##\left ( \partial _{\mu} \phi \right ) \left ( x \right ) = \frac {\partial \phi \left ( x \right )} {\partial x^\mu} \rightarrow \frac {\partial \phi^{'} \left ( x^{'} \right )} { \partial x^{' \mu}}=\frac {\partial \phi \left ( x \right )} { \partial x^{' \mu}}=\frac {\partial \phi \left ( x \right )} { \partial x^{ \sigma}} \frac {\partial x^{ \sigma}} {\partial x^{' \mu}}=\left ( \Lambda ^{-1} \right ) ^\sigma {} _\mu \partial _\sigma \phi##

Cheers!
 
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Hello, @PeroK. I would like to ask some advice about the derivatives in tensor forms.

Given ##\partial _ \mu \phi ^ \nu##, how to calculate ##\partial ^ \mu \phi ^ \nu##, ##\partial _ \mu \phi _ \nu##, and ##\partial ^ \mu \phi _ \nu##?

I have done the calculation. I have
##\partial ^ \mu \phi ^ \nu = \eta_{\mu \lambda} \partial _ {\lambda} \phi ^ \nu##,
##\partial _ \mu \phi _ \nu = \eta_{\nu \lambda} \partial _ {\mu} \phi ^ \lambda##, and
##\partial ^ \mu \phi _ \nu = \eta_{\mu \sigma} \eta_{\nu \lambda} \partial _ {\sigma} \phi ^ \lambda##.

I find these derivatives quite useful, but I do not know whether I have the right derivatives, and I do not know where to go to check them. Do you have any information about them?

Thanks!
 
\phi^{\nu,\mu}=\eta^{\mu \lambda} \phi^{\nu}_{\ \ ,\lambda}
\phi_{\nu\ ,\mu}=\eta_{\nu\lambda} \phi^{\lambda}_{\ \ ,\mu}
\phi^{\ \ ,\mu}_{\nu}=\eta^{\sigma \mu} \eta^\nu_\lambda\phi^\lambda_{\ \ ,\sigma}
where
X_{,\mu}=\frac{\partial X}{\partial x^\mu}
X^{,\mu}=\frac{\partial X}{\partial x_\mu}

EDIT correction of the third equation
\phi^{\ \ ,\mu}_{\nu}=\eta^{\sigma \mu} \eta_{\nu\lambda}\phi^\lambda_{\ \ ,\sigma}
as pointed out.
 
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anuttarasammyak said:
\phi^{\nu,\mu}=\eta^{\mu \lambda} \phi^{\nu}_{\ \ ,\lambda}
\phi_{\nu\ ,\mu}=\eta_{\nu\lambda} \phi^{\lambda}_{\ \ ,\mu}
\phi^{\ \ ,\mu}_{\nu}=\eta^{\sigma \mu} \eta^\nu_\lambda\phi^\lambda_{\ \ ,\sigma}
where
X_{,\mu}=\frac{\partial X}{\partial x^\mu}
X^{,\mu}=\frac{\partial X}{\partial x_\mu}

Thanks, @anuttarasammyak .

If I use the metric tensor ##\eta ^{\mu \nu}= \begin{pmatrix} 1 & 0 & 0 & 0 \\ 0 & -1 & 0 & 0\\0 & 0 &-1 & 0\\0 & 0 & 0 & -1 \end{pmatrix} ##, then whether the indices are upper or lower would be irrelavent. After checking with your equations, I think I got them right.

Thanks!
 
Haorong Wu said:
Hello, @PeroK. I would like to ask some advice about the derivatives in tensor forms.

Given ##\partial _ \mu \phi ^ \nu##, how to calculate ##\partial ^ \mu \phi ^ \nu##, ##\partial _ \mu \phi _ \nu##, and ##\partial ^ \mu \phi _ \nu##?

I have done the calculation. I have
##\partial ^ \mu \phi ^ \nu = \eta_{\mu \lambda} \partial _ {\lambda} \phi ^ \nu##,
##\partial _ \mu \phi _ \nu = \eta_{\nu \lambda} \partial _ {\mu} \phi ^ \lambda##, and
##\partial ^ \mu \phi _ \nu = \eta_{\mu \sigma} \eta_{\nu \lambda} \partial _ {\sigma} \phi ^ \lambda##.

I find these derivatives quite useful, but I do not know whether I have the right derivatives, and I do not know where to go to check them. Do you have any information about them?

Thanks!

You need to find a reference on tensor notation. The free indices must match on each side of the equation, and you sum over pairs of one upper and one lower index. Your formulas will work out because the metric tensor is the same in upper and lower format.

In flat spacetime we have a four vector in upper and lower index notation:
$$a^{\mu} = (a^0, a^1, a^2, a^3), \ \text{and} \ a_{\mu} = (a_0, a_1, a_2, a_3)$$
Where ##a^0 = a_0 = a_t, a^1 = -a_1 = a_x , a^2 = -a_2 = a_y, a^3 = -a_3 = a_z##

This can be written using the metric tensor ##\eta^{\mu\nu} = \eta_{\mu\nu} = diag(1, -1, -1, -1)##:
$$a^{\mu} = \eta^{\mu\nu} a_{\nu}$$
The derivatives are defined by:
$$\partial_{\mu} = \frac{\partial}{\partial x^{\mu}} \ \text{and} \ \partial^{\mu} = \frac{\partial}{\partial x_{\mu}}$$
And these are related:
$$\partial^{\mu} = \eta^{\mu\nu}\partial_{\mu}$$
The derivative of a scalar is a four-vector:
$$\partial^{\mu} \phi = \eta^{\mu\nu}\partial_{\mu}\phi$$
And the derivative of a four-vector has upper and lower components:
$$\partial^{\mu} \phi^{\lambda} = \eta^{\mu\nu} \eta^{\lambda\rho}\partial_{\mu}\phi_{\rho}$$
 
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Thanks, @PeroK .

I intentially misuse the upper and lower indices since the metric tensor in QFT seems not to play an important role. (Am I right? I have not met the situations where they are important.)

However, I will use your expression since they would be much more easier to memorize.

Thanks!

From now on, I would just use a metric tensor to lower or raise a indice in the partial derivatives.
 
Haorong Wu said:
If I use the metric tensor ημν=(10000−10000−10000−1), then whether the indices are upper or lower would be irrelavent.
And
\eta_{\mu}^\nu=<br /> \begin{pmatrix}<br /> 1 &amp; 0 &amp; 0&amp; 0 \\<br /> 0 &amp; 1 &amp; 0&amp; 0 \\<br /> 0 &amp; 0 &amp; 1&amp; 0 \\<br /> 0 &amp; 0 &amp; 0&amp; 1 \\<br /> \end{pmatrix}=\delta_{\mu}^\nu
 
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  • #10
anuttarasammyak said:
And
\eta_{\mu}^\nu=<br /> \begin{pmatrix}<br /> 1 &amp; 0 &amp; 0&amp; 0 \\<br /> 0 &amp; 1 &amp; 0&amp; 0 \\<br /> 0 &amp; 0 &amp; 1&amp; 0 \\<br /> 0 &amp; 0 &amp; 0&amp; 1 \\<br /> \end{pmatrix}=\delta_{\mu}^\nu

But...I do not understand this equation
##\phi^{\ \ ,\mu}_{\nu}=\eta^{\sigma \mu} \eta^\nu_\lambda\phi^\lambda_{\ \ ,\sigma}##

I only get
##\partial ^ \mu \phi _\nu = \frac {\partial \phi _\nu} {\partial x_\mu}=\frac {\eta _{\nu \lambda} \partial \phi ^ \lambda} {\eta_{\mu \sigma} \partial x^ \sigma}=\eta _{\nu \lambda} \eta ^{\mu \sigma} \partial _\sigma \phi ^ \lambda##
 
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  • #11
You are right. I wrote it with mistake.
 
  • #12
anuttarasammyak said:
You are right. I wrote it with mistake.
OK. Thanks, @anuttarasammyak .
 
  • #13
@Haorong Wu another important point is the defining property of a Lorentz Transformation:

\eta_{\mu\nu}\Lambda^{\mu}{}_{\rho}\Lambda^{\nu}{}_{\sigma} = \eta_{\rho \sigma}
 
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  • #14
PeroK said:
@Haorong Wu another important point is the defining property of a Lorentz Transformation:

\eta_{\mu\nu}\Lambda^{\mu}{}_{\rho}\Lambda^{\nu}{}_{\sigma} = \eta_{\rho \sigma}

Oh, yes. David Tong mentioned it in his note. Also, I derived that ##\eta_{\mu\nu} \left ( \Lambda ^{-1} \right )^{\mu}{}_{\rho}\left ( \Lambda ^{-1} \right )^{\nu}{}_{\sigma} = \eta_{\rho \sigma}##, hoping this would be correct.
 
  • #15
Haorong Wu said:
Oh, yes. David Tong mentioned it in his note. Also, I derived that ##\eta_{\mu\nu} \left ( \Lambda ^{-1} \right )^{\mu}{}_{\rho}\left ( \Lambda ^{-1} \right )^{\nu}{}_{\sigma} = \eta_{\rho \sigma}##, hoping this would be correct.
Well, ##\Lambda ^{-1}## is also a Lorentz Transformation, so that equation must hold!
 
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