For retarded scalar potential of arbigtrary source around origin:(adsbygoogle = window.adsbygoogle || []).push({});

[tex]V(\vec r, t) = \frac 1 {4\pi\epsilon_0}\int \frac { \rho(\vec r\;',t-\frac {\eta}{c}) }{\eta} d\;\tau' \;\hbox { where }\;\eta =\sqrt{r^2 + r'^2 - 2 \vec r \cdot \vec r\;' }[/tex]

Where [itex]\;\vec r \;[/itex] point to the field point where V is measured. And [itex]\;\vec r\;' \;[/itex] points to the source point.

For [itex]\;\vec r\;' \;[/itex] << [itex]\;\vec r \;[/itex]:

[tex] \eta \approx \; r- \hat r \cdot \vec r\;' \Rightarrow \rho(\vec r\;',\;t-\frac {\eta}{c}) \approx \rho (\vec r\;',\;t-\frac {r}{c} + \frac {\vec r \cdot \vec r\;'}{c}) [/tex]

This next step is where I don't understand how the book do the Taylor expansion. I am going to type the exact word from the book:

Expanding [itex]\rho \;[/itex] as a Taylor series in t about the retarded time at the origin,

[tex]t_0=t-\frac r c [/tex]

We have

[tex]\rho(\vec r\;',\;t-\frac {\eta}{c}) \approx \rho (\vec r\;',\; t_0) + \dot{\rho} (\vec r\;',\; t_0)\left ( \frac {\vec r \cdot \vec r\;'}{c}\right ) + \frac 1 {2!} \ddot{\rho} \left ( \frac {\vec r \cdot \vec r\;'}{c}\right )^2 + \frac 1 {3!} \rho^{...}_{ } \left ( \frac {\vec r \cdot \vec r\;'}{c}\right )^3 ........[/tex]

Why are they use [itex]\left ( \frac {\vec r \cdot \vec r\;'}{c}\right )\;[/itex] as x for the expansion. I just don't follow this. Please help.

thanks

Alan

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# Please explain Taylor expansion in radiation.

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