- #1
LeoJakob
- 24
- 2
Electrostatic potential $$ \Phi(\vec{r})=k \int \mathrm{d}^{3} r \frac{\rho\left(\vec{r}^{\prime}\right)}{\left|\vec{r}-\vec{r}^{\prime}\right|} (i) $$ with $$ k=\frac{1}{4\pi\epsilon_{0}} $$ in SI units.
What work is required to move a point charge q from infinity to the center of the through $$ \rho(\vec{r})=\rho_{0}\mathrm{e}^{-a r} (ii) $$ given charge distribution, where $$ a \text{ and } \rho_{0} $$ are constants? Work in Gaussian units.
To solve the problem I would use spherical coordiantes. The potential only depends on the radial difference between the charge q with position
$$\vec{r} = r\hat{e}_r \text{ and the location vector of the charge distribution element } \vec{r'} = r' \hat{e}_r \text{ such that }\\
\left|\vec{r}-\vec{r'}\right| = \sqrt{(r-r')^2}
$$
$$\text{Define } \Phi(\infty)=0 \text{ then the work is given by } W= q \Phi(\vec r)=q \Phi(r)$$
$$W= q\Phi(\vec{r})=k \int \mathrm{d}^{3} r' \frac{\rho\left(\vec{r}^{\prime}\right)}{\left|\vec{r}-\vec{r}^{\prime}\right|}= \int \mathrm{d}^{3} r' \frac{\rho(r^{\prime})}{\sqrt{(r-r')^2}}=4\pi\int \limits_\infty^0 (r')^3 \frac{\rho(r^{\prime})}{\sqrt{(r-r')^2}}dr^{\prime}$$
The factor 4pi comes from the integration in spherical coordinates and k=1 in Gaussian units.
Is my approach right?
What work is required to move a point charge q from infinity to the center of the through $$ \rho(\vec{r})=\rho_{0}\mathrm{e}^{-a r} (ii) $$ given charge distribution, where $$ a \text{ and } \rho_{0} $$ are constants? Work in Gaussian units.
To solve the problem I would use spherical coordiantes. The potential only depends on the radial difference between the charge q with position
$$\vec{r} = r\hat{e}_r \text{ and the location vector of the charge distribution element } \vec{r'} = r' \hat{e}_r \text{ such that }\\
\left|\vec{r}-\vec{r'}\right| = \sqrt{(r-r')^2}
$$
$$\text{Define } \Phi(\infty)=0 \text{ then the work is given by } W= q \Phi(\vec r)=q \Phi(r)$$
$$W= q\Phi(\vec{r})=k \int \mathrm{d}^{3} r' \frac{\rho\left(\vec{r}^{\prime}\right)}{\left|\vec{r}-\vec{r}^{\prime}\right|}= \int \mathrm{d}^{3} r' \frac{\rho(r^{\prime})}{\sqrt{(r-r')^2}}=4\pi\int \limits_\infty^0 (r')^3 \frac{\rho(r^{\prime})}{\sqrt{(r-r')^2}}dr^{\prime}$$
The factor 4pi comes from the integration in spherical coordinates and k=1 in Gaussian units.
Is my approach right?