Coefficients in expansions of a vector potential

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Discussion Overview

The discussion revolves around the differences in coefficients found in two expansions of a vector potential in the context of Fourier transforms. Participants explore the implications of these coefficients and their relation to different conventions used in physics and mathematics.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • One participant notes two different expansions of a vector potential, highlighting the differing coefficients of ##(2 \pi)^{3/2}## and ##(2 \pi)^3##.
  • Another participant suggests that the constant coefficients are merely a matter of convenience and reflect differing preferences among authors.
  • It is proposed that the differences arise from various normalization conventions in the Fourier mode decomposition across different fields of physics.
  • A participant explains that physicists and mathematicians have distinct definitions of the Fourier transform, which contributes to the variation in coefficients.
  • One participant elaborates on the diversity of conventions in different subfields of physics, providing examples from non-relativistic quantum mechanics and relativistic quantum field theory.
  • Another participant reassures that the constants in question are dimensionless and should not cause concern.

Areas of Agreement / Disagreement

Participants generally agree that the differences in coefficients are due to conventions and preferences among authors, but no consensus is reached on a single standard or resolution of the issue.

Contextual Notes

The discussion highlights the complexity and variability of definitions and conventions in the use of Fourier transforms across different disciplines, with no resolution on which convention is superior or more widely accepted.

Haorong Wu
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TL;DR
Why the coefficients in expansions of a vector potential are different in different papers?
I have seen two expansions of a vector potential,

$$\mathbf A=\sum_\sigma \int \frac{d^3k}{(16 \pi^3 |\mathbf k|)^{1/2}} [\epsilon_\sigma(\mathbf k) \alpha_\sigma (\mathbf k) e^{i \mathbf k \cdot \mathbf x}+c.c.],$$
and
$$\mathbf A=\sum_\sigma \int \frac{d^3k}{ (2 \pi)^3(2 |\mathbf k|)^{1/2}} [\epsilon_\sigma(\mathbf k) \alpha_\sigma (\mathbf k) e^{i \mathbf k \cdot \mathbf x}+c.c.],$$
where ##\epsilon_\sigma## are polarizations, ##\alpha_\sigma (\mathbf k)## are amplitudes.

My problem is the two coefficients ## (2 \pi)^{3/2}## and ## (2 \pi)^3## in these two expressions, respectively. Why they are different?

I do not remember where I have read something about it, that it is related to the definition of Fourier transform.

Thanks for any hints.
 
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The constant coefficients don’t matter. They are only there for convenience. They are different because the two different authors disagreed on which was most convenient.
 
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It's just a question of conventions. You have as many normalization conventions in the Fourier mode decomposition of (quantum) fields you have authors of textbooks and papers (or even more ;-)).
 
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Physicists usually define the FT as ##f(x)=\int...F(k)##,and mathematicians
use ##f(x)=(2\pi)^{-1/2}\int##.
 
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Well, there are many types of physicists and all define their FTs differently. Sometimes the convention changes even in different subfields of physics.

E.g., in non-relativistic quantum mechanics one usually defines the FT between position and momentum (or rather "wave-vector") representation in a symmetric way, i.e., as unitary transformations from ##\mathrm{L}^2 \rightarrow \mathrm{L}^2## (for 1D motion):
$$\psi(x)=\int_{-\infty}^{\infty} \mathrm{d} k \frac{1}{\sqrt{2 \pi}} \tilde{\psi}(k) \exp(\mathrm{i} k x) \; \Leftrightarrow \; \tilde{\psi}(k)=\int_{-\infty}^{\infty} \mathrm{d} x \frac{1}{\sqrt{2 \pi}} \psi(x) \exp(-\mathrm{i} k x).$$
In relativistic (Q)FT most physicists use
$$\psi(x)=\int_{-\infty}^{\infty} \mathrm{d} k \frac{1}{2 \pi} \tilde{\psi}(k) \exp(\mathrm{i} k x) \; \Leftrightarrow \; \tilde{\psi}(k)=\int_{-\infty}^{\infty} \mathrm{d} x \psi(x) \exp(-\mathrm{i} k x).$$
For the FT wrt. time vs. angular frequency you have the same conventions but with the opposite signs in the exponentials. That's because one usually has to solve wave equations and likes to have ##k## the direction of the wave's phase velocity and not ##-k##.

In many engineering texts this signs in the exponential are reversed ;-)).

In short, it's a mess, and one must be careful when reading texts to make sure to figure out, which convention is used.
 
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Thank you all! It is clear now.
 
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The different constants shouldn't trouble you a lot. Unless of course the constants present in formulas have dimensions. In this case they are plain numbers, no dimensions involved.
 

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