General solution to the wave equation of electromagnetic field

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Discussion Overview

The discussion revolves around the general solution to the wave equation of the electromagnetic field, specifically focusing on the four-vector potential and the mathematical formulation of the solution. Participants explore the transition from summation to integration in the context of the wave equation and the implications of using different variables in the integration process.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant questions the origin of the term $$\frac {d^3 \mathbf{k}}{(2 \pi)^3}$$ in the solution, suggesting it should be $$d^3\mathbf{x}$$ instead.
  • Another participant responds that the term arises from the density of states in $$\mathbf{k}$$-space and argues that integrating over $$d^3\mathbf{x}$$ would not yield the vector potential as a function of $$\mathbf{x}$$.
  • A different participant inquires why the superposition is expressed as an integral rather than a sum, questioning the transformation from discrete to continuous variables.
  • Another participant raises a point about the nature of $$k$$ being a continuous variable, questioning the validity of summing over its continuous values.

Areas of Agreement / Disagreement

Participants express differing views on the mathematical formulation of the wave equation solutions, particularly regarding the use of integration versus summation and the implications of the variable $$k$$. There is no consensus reached on these points.

Contextual Notes

Participants have not fully resolved the implications of using $$d^3\mathbf{k}$$ versus $$d^3\mathbf{x}$$, nor have they clarified the transition from summation to integration in the context of continuous variables.

victorvmotti
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Suppose that we have the four-vector potential of the electromagnetic field, [texA^i[/tex]

The wave equation is given by $$(\frac {1}{c^2} \frac {\partial^2}{\partial t^2}-\nabla^2) A^i=0$$

Now the solution, for a purely spatial potential vector, is given by

$$\mathbf{A}(t, \mathbf{x})=\mathbf{a_k} \exp{i(\pm \omega_{\mathbf{k}}t-\mathbf{k}.\mathbf{x}}); \mathbf{k}.\mathbf{a}=0$$

To find the general solution we write the superposition as

$$\mathbf{A}(t, \mathbf{x})=\int (\mathbf{f(k)}\exp{i( \omega_{\mathbf{k}}t-\mathbf{k}.\mathbf{x}})+\mathbf{g(k)}\exp{-i( \omega_{\mathbf{k}}t+\mathbf{k}.\mathbf{x}})) \frac {d^3 \mathbf{k}}{(2 \pi)^3}$$

My question is that where this $$\frac {d^3 \mathbf{k}}{(2 \pi)^3}$$

comes from? Shouldn't it be $$d^3\mathbf{x}$$
 
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victorvmotti said:
My question is that where this $$\frac {d^3 \mathbf{k}}{(2 \pi)^3}$$

comes from? Shouldn't it be $$d^3\mathbf{x}$$
It comes from the density of states in ##\mathbf{k}##-space. If you were to integrate over ##d^3\mathbf{x}##, you wouldn't get the vector potential as a function of ##\mathbf{x}##, would you?
 
Why we do not say that $$\mathbf{A}(t, \mathbf{x})=\sum_{\mathbf{f(k)}\mathbf{g(k)}} (\mathbf{f(k)}\exp{i( \omega_{\mathbf{k}}t-\mathbf{k}.\mathbf{x}})+\mathbf{g(k)}\exp{-i( \omega_{\mathbf{k}}t+\mathbf{k}.\mathbf{x}})) $$

Isn't superposition simply given by the above sum? Why and how we transform to the integral?
 
Isnt' k a continuous variable? How could you sum after its continuous values?
 

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