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Solutions to I.E. Irodov's problems in general physics

Abhay Kumar Singh; I E Irodov

Chapter 3

Electrodynamics - all with Video Answers

Educators


Section 1

Constant Electric Field in Vacuum

01:43

Problem 1

$$
\begin{aligned}
&F_{d}(\text { for electorns })=\frac{q^{2}}{4 \pi \varepsilon_{0} r^{2}} \text { and } F_{8 r}=\frac{\gamma m^{2}}{r^{2}} \\
&\text { Thus } \quad \frac{F_{d}}{F_{g r}} \text { (for electrons) }=\frac{q^{2}}{4 \pi \varepsilon_{0} \gamma m^{2}} \\
&=\frac{\left(1-602 \times 10^{-19} \mathrm{C}\right)^{2}}{\left(\frac{1}{9 \times 10^{9}}\right) \times 6.67 \times 10^{-11} \mathrm{~m}^{3} /\left(\mathrm{kg} \cdot \mathrm{s}^{2}\right) \times\left(9 \cdot 11 \times 10^{-31} \mathrm{~kg}\right)^{2}}=4 \times 10^{42} \\
&\text { Similarly } \quad \frac{F_{d}}{F_{g r}}(\text { for proton })=\frac{q^{2}}{4 \pi \varepsilon_{0} \gamma m^{2}} \\
&=\frac{\left(1.602 \times 10^{-19} \mathrm{C}\right)^{2}}{\left(\frac{1}{9 \times 10^{9}}\right) \times 6.67 \times 10^{-11} \mathrm{~m}^{3} /\left(\mathrm{kg} \cdot \mathrm{s}^{2}\right) \times\left(1.672 \times 10^{-27} \mathrm{~kg}\right)^{2}}=1 \times 10^{36} \\
&\text { For } F_{d}=F_{g r} \\
&=\sqrt{\frac{6.67 \times 10^{-11} \mathrm{~m}^{3}\left(\mathrm{~kg}-\mathrm{s}^{2}\right)}{9 \times 10^{9}}}=0.86 \times 10^{-10} \mathrm{C} / \mathrm{kg}
\end{aligned}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
01:57

Problem 2

Total number of atoms in the sphere of mass $1 \mathrm{gm}=\frac{1}{63 \cdot 54} \times 6.023 \times 10^{23}$ So the total nuclear charge $\lambda=\frac{6.023 \times 10^{23}}{63 \cdot 54} \times 1.6 \times 10^{-19} \times 29$
Now the charge on the sphere = Total nuclear charge - Total electronic charge

Khoobchandra Agrawal
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04:15

Problem 3

Let the balls be deviated by an angle $\theta$, from the vertical when separtion between them equals $\boldsymbol{x}$. Applying Newton's second law of motion for any one of the sphere, we get, $T \cos \theta=m g$
and $\quad T \sin \theta=F_{e}$
From the Eqs. (1) and (2)
(3)
But from
(4)
From Eqs. (3) and (4) $F_{e}=\frac{m g x}{2 l}$ or $\frac{q^{2}}{4 \pi \varepsilon_{0} x^{2}}=\frac{m g x}{2 l}$
$q^{2}=\frac{2 \pi \varepsilon_{0} m g x^{3}}{l}$
Differentiating Eqn. (5) with respect to time $2 q \frac{d q}{d t}=\frac{2 \pi \varepsilon_{0} m g}{l} 3 x^{2} \frac{d x}{d t}$
According to the problem $\frac{d x}{d t}=v=a / \sqrt{x}$ (approach velocity is $\left.\frac{d x}{d t}\right)$
so, $\left(\frac{2 \pi \varepsilon_{0} m g}{l} x^{3}\right)^{1 / 2} \frac{d q}{d t}=\frac{3 \pi \varepsilon_{0} m g}{l} x^{2} \frac{a}{\sqrt{x}}$
Hence, $\frac{d q}{d t}=\frac{3}{2} a \sqrt{\frac{2 \pi e_{0} m g}{l}}$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
04:48

Problem 4

Let us choose coordinate axes as shown in the figure and fix three charges, $q_{1}, q_{2}$ and $q_{3}$ having position vectors $\overrightarrow{r_{1}}, \overrightarrow{r_{2}}$ and $\overrightarrow{r_{3}}$ respectively. Now, for the equilibrium of $q_{3}$ $\frac{+q_{2} q_{3}\left(\overrightarrow{r_{2}}-\overrightarrow{r_{3}}\right)}{\left|\overrightarrow{r_{2}}-\overrightarrow{r_{3}}\right|^{3}}+\frac{q_{1} q_{3}\left(\overrightarrow{r_{1}}-\overrightarrow{r_{3}}\right)}{\left|\overrightarrow{r_{1}}-\overrightarrow{r_{3}}\right|^{3}}=0$
or,
$$
\begin{gathered}
\frac{q_{2}}{\left|\vec{r}_{2}-\overrightarrow{r_{3}}\right|^{2}}=\frac{q_{1}}{\left|\overrightarrow{r_{1}}-\overrightarrow{r_{3}}\right|^{2}} \\
\frac{\overrightarrow{r_{2}}-\overrightarrow{r_{3}}}{\left|\overrightarrow{r_{2}}-\overrightarrow{r_{3}}\right|}=-\frac{\overrightarrow{r_{1}}-\overrightarrow{r_{3}}}{\left|\overrightarrow{r_{1}}-\overrightarrow{r_{3}}\right|}
\end{gathered}
$$
because
or,
$$
\sqrt{q_{2}}\left(\overrightarrow{r_{1}}-\overrightarrow{r_{3}}\right)=\sqrt{q_{1}}\left(\overrightarrow{r_{3}}-\overrightarrow{r_{2}}\right)
$$
or,
$$
\overrightarrow{r_{3}}=\frac{\sqrt{q_{2}} \overrightarrow{r_{1}}+\sqrt{q_{1}} \overrightarrow{r_{2}}}{\sqrt{q_{1}}+\sqrt{q_{2}}}
$$
Also for the equilibrium of $q_{1}$,
$$
\frac{q_{3}\left(\overrightarrow{r_{3}}-\overrightarrow{r_{1}}\right)}{\left|\overrightarrow{r_{3}}-\overrightarrow{r_{1}}\right|^{3}}+\frac{q_{2}\left(\overrightarrow{r_{2}}-\overrightarrow{r_{1}}\right)}{\left|\overrightarrow{r_{2}}-\overrightarrow{r_{1}}\right|^{3}}=0
$$
or,
$$
q_{3}=\frac{-q_{2}}{\left|\overrightarrow{r_{2}}-\overrightarrow{r_{1}}\right|^{2}}\left|\overrightarrow{r_{1}}-\overrightarrow{r_{3}}\right|^{2}
$$
Substituting the value of $\overrightarrow{r_{3}}$, we get,
$$
q_{3}=\frac{-q_{1} q_{2}}{\left(\sqrt{q_{1}}+\sqrt{q_{2}}\right)^{2}}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
03:51

Problem 5

When the charge $q_{0}$ is placed at the centre of the ring, the wire get stretched and the extra tension, produced in the wire, will balance the electric force due to the charge $q_{0}$. Let the tension produced in the wire, after placing the charge $q_{0}$, be $T$. From Newton's second law in projection form $F_{n}=m w_{n^{*}}$
$T d \theta-\frac{1}{4 \pi \varepsilon_{0}} \frac{q_{0}}{r^{2}}\left(\frac{q}{2 \pi r} r d \theta\right)=(d m) 0$
or, $T=\frac{q q_{0}}{8 \pi^{2} \varepsilon_{0} r^{2}}$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
00:45

Problem 6

Sought field strength
$$
\vec{E}=\frac{1}{4 \pi \varepsilon_{0}\left|\overrightarrow{r-} \overrightarrow{r_{0}}\right|^{2}}
$$
$=4.5 \mathrm{kV} / \mathrm{m}$ on putting the values.

Khoobchandra Agrawal
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Numerade Educator
03:23

Problem 7

Let us fix the coordinate system by taking the point of intersection of the diagonals as the origin and let $\vec{k}$ be directed normally, emerging from the plane of figure. Hence the sought field strength :
$$
\begin{aligned}
&\vec{E}=\frac{q}{4 \pi \varepsilon_{0}} \frac{l i+x \vec{k}}{\left(l^{2}+x^{2}\right)^{3 / 2}}+\frac{-q}{4 \pi \varepsilon_{0}} \frac{l(-\vec{i})+x \vec{k}}{\left(l^{2}+x^{2}\right)^{3 / 2}} \\
&+\frac{-q}{4 \pi \varepsilon_{0}} \frac{l \vec{j}+x \vec{k}}{\left(l^{2}+x^{2}\right)^{3 / 2}}+\frac{q}{4 \pi \varepsilon_{0}} \frac{l(-\vec{j})+x \vec{k}}{\left(l^{2}+x^{2}\right)^{3 / 2}} \\
&=\frac{q}{4 \pi \varepsilon_{0}\left(l^{2}+x^{2}\right)^{3 / 2}}[2 l i-2 l j] \\
&\text { Thus } E=\frac{q l}{\sqrt{2} \pi \varepsilon_{0}\left(l^{2}+x^{2}\right)^{3 / 2}}
\end{aligned}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:13

Problem 8

From the symmetry of the problem the sought field.
$$
E=\int d E_{x}
$$
where the projection of field strength along $x$ - axis due to an elemental charge is
$$
d E_{x}=\frac{d q \cos \theta}{4 \pi \varepsilon_{0} R^{2}}=\frac{q R \cos \theta d \theta}{4 \pi^{2} \varepsilon_{0} R^{3}}
$$
Hence
$$
E=\frac{q}{4 \pi^{2} \varepsilon_{0} R^{2}} \int_{\pi / 2} \cos \theta d \theta \frac{q}{2 \pi^{2} \varepsilon_{0} R^{2}}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
04:04

Problem 9

From the symmetry of the condition, it is clear that, the field along the normal will be zero i.e. $\quad E_{n}=0$ and $E=E_{l}$
Now $\quad d E_{l}=\frac{d q}{4 \pi \varepsilon_{0}\left(R^{2}+l^{2}\right)} \cos \theta$
But $\quad d q=\frac{q}{2 \pi R} d x$ and $\cos \theta=\frac{l}{\left(R^{2}+l^{2}\right)^{1 / 2}}$
Hence
or
charge,
$$
\begin{aligned}
&\text { For } E_{\max }, \text { we should have } \frac{d E}{d l}=0\\
&\text { So, }\left(l^{2}+R^{2}\right)^{3 / 2}-\frac{3}{2} l\left(l^{2}+R^{2}\right)^{1 / 2} 2 l=0 \quad \text { or } \quad l^{2}+R^{2}-3 l^{2}=0\\
&\text { Thus } l=\frac{R}{\sqrt{2}} \text { and } E_{\max }=\frac{q}{6 \sqrt{3} \pi \varepsilon_{0} R^{2}}
\end{aligned}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
03:10

Problem 10

The electric potential at a distance $x$ from the given ring is given by,
$$
\varphi(x)=\frac{q}{4 \pi \varepsilon_{0} x}-\frac{q}{4 \pi \varepsilon_{0}\left(R^{2}+x^{2}\right)^{1 / 2}}
$$
Hence, the field strength along $x$ -axis (which is the net field strength in 'our case),
$$
\begin{aligned}
E_{x}=&-\frac{d \varphi}{d x}=\frac{q}{4 \pi \varepsilon_{0}} \frac{1}{x^{2}}-\frac{q x}{4 \pi \varepsilon_{0}\left(R^{2}+x^{2}\right)^{3 / 2}} \\
&=\frac{\frac{q}{4 \pi \varepsilon_{0}} x^{3}\left[\left(1+\frac{R^{2}}{x^{2}}\right)^{3 / 2}-1\right]}{x^{2}\left(R^{2}+x^{2}\right)^{3 / 2}} \\
=& \frac{q}{4 \pi \varepsilon_{0}} x^{3}\left[1+\frac{3}{2} \frac{R^{2}}{x^{2}}+\frac{3}{8} \frac{R^{4}}{x^{4}}+\ldots\right] \\
x^{2}\left(R^{2}+x^{2}\right)^{3 / 2}
\end{aligned}
$$
Neglecting the higher power of $R / x$, as $x \gg>R$
$$
E=\frac{3 q R^{2}}{8 \pi \varepsilon_{0} x^{4}}
$$
Note : Instead of $\varphi(x)$, we may write $E(x)$ directly using $3.9$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:23

Problem 11

From the solution of $3.9$, the electric field strength due to ring at a point on its axis (say $x$ -axis) at distance $\dot{x}$ from the centre of the ring is given by:
And from symmetry $\vec{E}$ at every point on the axis is directed along the $x$ -axis (Fig.). Let us consider an element $(d x)$ on thread which carries the charge $(\lambda d x) .$ The electric force experienced by the element in the field of ring. $d F=(\lambda d x) E(x)=\frac{\lambda q x d x}{4 \pi \varepsilon_{0}\left(R^{2}+x^{2}\right)^{3 / 2}}$
Thus the sought interaction $\infty$
On integrating we get, $F=\frac{\lambda q}{4 \pi \varepsilon_{0} R}$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
09:23

Problem 12

(a) The given charge distribution is shown in Fig. The symmetry of this distribution implies that vector $\vec{E}$ at the point $O$ is directed to the right, and its magnitude is equal to the sum of the projection onto the direction of $\vec{E}$ of vectors $d \vec{E}$ from elementary charges $d q$. The projection of vector $d \vec{E}$ onto vector $\vec{E}$ is $\varphi=\frac{1}{4 \pi \varepsilon_{0}} \frac{d q}{R^{2}} \cos \varphi$
where $d q=\lambda R d \varphi=\lambda_{0} R \cos \varphi d \varphi$.
Integrating (1) over $\varphi$ between 0 and $2 \pi$ we find the magnitude of the vector $E$ :

It should be noted that this integral is evaluated in the most simple way if we take into account that $\left\langle\cos ^{2} \varphi\right\rangle=1 / 2$. Then
$2 \pi$
(b) Take an element $S$ at an azimuthal angle $\varphi$ from the $x$ -axis, the element subtending an angle $d \varphi$ at the centre. The elementary field at $P$ due to the element is $\frac{\lambda_{0} \cos \varphi d \varphi R}{4 \pi \varepsilon_{0}\left(x^{2}+R^{2}\right)}$ along $S P$ with components
$\frac{\lambda_{0} \cos \varphi d \varphi R}{4 \pi \varepsilon_{0}\left(x^{2}+R^{2}\right)} \times\{\cos \theta$ along $O P,$,
along OS $\}$
where $\quad \cos \theta=\frac{x}{\left(x^{2}+R^{2}\right)^{1 / 2}}$
$2 \pi$
The component along $O P$ vanishes on integration as $\int_{0} \cos \varphi d \varphi=0$ The component alon $O S$ can be broken into the parts along $O X$ and $O Y$ with $\frac{\lambda_{0} R^{2} \cos \varphi d \varphi}{4 \pi \varepsilon_{0}\left(x^{2}+R^{2}\right)^{3 / 2}} \times\{\cos \varphi$ along $O X, \sin \varphi$ along OY $\}$
On integration, the part along $O Y$ vanishes. Finally
For

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
06:16

Problem 13

(a) It is clear from symmetry considerations that vector $\vec{E}$ must be directed as shown in the figure. This shows the way of solving this problem : we must find the component $d E_{r}$ of the field created by the element $d l$ of the rod, having the charge $d q$ and then integrate the result over all the elements of the rod. In this case
$$
d E_{r}=d E \cos \alpha=\frac{1}{4 \pi \varepsilon_{0}} \frac{\lambda d l}{r_{0}^{2}} \cos \alpha
$$
where $\lambda=\frac{q}{2 a}$ is the linear charge density. Let us reduce this equation of the form convenient
for integration. Figure shows that $d l \cos \alpha=r_{0} d \alpha$ and $r_{0}=\frac{r}{\cos n}$; Consequently, $d E_{r}=\frac{1}{4 \pi \varepsilon_{0}} \frac{\lambda r_{0} d \alpha}{r_{0}^{2}}=\frac{\lambda}{4 \pi \varepsilon_{0} r} \cos \alpha d \alpha$
This expression can be easily integrated :
$\alpha_{0}$
$E=\frac{\lambda}{4 \pi \varepsilon_{0} r} 2 \int_{0} \cos \alpha d \alpha=\frac{\lambda}{4 \pi \varepsilon_{0} r} 2 \sin \alpha_{0}$
where $\alpha_{0}$ is the maximum value of the angle $\alpha$, $\sin \alpha_{0}=a / \sqrt{a^{2}+r^{2}}$
Thus, $E=\frac{q / 2 a}{4 \pi \varepsilon_{0} r} 2 \frac{a}{\sqrt{a^{2}+r^{2}}}=\frac{q}{4 \pi \varepsilon_{0} r \sqrt{a^{2}+r^{2}}}$
Note that in this case also $E \sim \frac{q}{4 \pi \varepsilon_{0} r^{2}}$ for $r>>a$ as of the field of a point charge.
(b) Let, us consider the element of length $d l$ at a distance $l$ from the centre of the rod, as shown in the figure. Then field at $P$, due
if the element lies on the side, shown in the diagram, and $d E=\frac{\lambda d l}{4 \pi \varepsilon_{0}(r+l)^{2}}$, if it lies on
other side.
Hence $E=\int d E=\int_{0}^{a} \frac{\lambda d l}{4 \pi \varepsilon_{0}(r-l)^{2}}+\int_{0}^{a} \frac{\lambda d l}{4 \pi \varepsilon_{0}(r+l)^{2}}$
On integrating and putting $\lambda=\frac{q}{2 a}$, we get, $E=\frac{q}{4 \pi \varepsilon_{0}} \frac{1}{\left(r^{2}-a^{2}\right)}$
For $\quad r \gg>a, \quad E \sim \frac{q}{4 \pi \varepsilon_{0} r^{2}}$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
04:09

Problem 14

The problem is reduced to finding $E_{x}$ and $E_{y}$ viz. the projections of $\vec{E}$ in Fig, where it is assumed that $\lambda>0$ Let us start with $E_{x^{\prime}}$ The contribution to $E_{x}$ from the charge element of the segment $d x$ is
Let us reduce this expression to the form convenient for integration. In our case, $d x=r d \alpha / \cos \alpha, r=y / \cos \alpha$. Then
$$
d E_{x}=\frac{\lambda}{4 \pi \varepsilon_{0} y} \sin \alpha d \alpha
$$
Integrating this expression over $\alpha$ between
$\theta$ and $\pi / 2$, we find $E_{x}=\lambda / 4 \pi \varepsilon_{0} y .$
In order to find the projection $E_{y}$ it is sufficient to recall that $d E_{y}$ differs from $d E_{x}$ in that $\sin \alpha$ in (1) is simply replaced by $\cos \alpha$
This gives $d E_{y}=(\lambda \cos \alpha d \alpha) / 4 \pi \varepsilon_{0} y$ and $E_{y}=\lambda / 4 \pi \varepsilon_{0} y$
We have obtained an interesting result :
$E_{x}=E_{y}$ independently of $y$,
i.e. $\vec{E}$ is oriented at the angle of $45^{\circ}$ to the rod. The modulus of $\vec{E}$ is
$$
E=\sqrt{E_{x}^{2}+E_{y}^{2}}=\lambda \sqrt{2} / 4 \pi \varepsilon_{0} y .
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
03:47

Problem 15

(a) Using the solution of $3.14$, the net electric field strength at the point $O$ due to straight parts of the thread equals zero. For the curved part (arc) let us derive a general expression
i.e. let us calculate the field strength at the centre of arc of radius $R$ and linear charge density $\lambda$ and which subtends angle $\theta_{0}$ at the centre.
From the symmetry the sought field strength will be directed along the bisector of the angle $\theta_{0}$ and is given by
$+\theta_{0} / 2$
$E=\int_{-\theta_{\sigma} / 2} \frac{\lambda(R d \theta)}{4 \pi \varepsilon_{0} R^{2}} \cos \theta=\frac{\lambda}{2 \pi \varepsilon_{0} R} \sin \frac{\theta_{0}}{2}$
In our problem $\theta_{0}=\pi / 2$, thus the field strength due to the turned part at the point $E_{0}=\frac{\sqrt{2} \lambda}{4 \pi \varepsilon_{0} R}$ which is also the sought result.
(b) Using the solution of $3.14$ (a), net field strength at $O$ due to stright parts equals $\sqrt{2}\left(\frac{\sqrt{2} \lambda}{4 \pi \varepsilon_{0} R}\right)=\frac{\lambda}{2 \pi \varepsilon_{0} R}$ and is directed vertically down. Now using the solution of $3.15$
(a), field strength due to the given curved part (semi-circle) at the point $O$ becomes $\frac{\lambda}{2 \pi \varepsilon_{0} R}$ and is directed vertically upward. Hence the sought net field strengh becomes zero.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
04:14

Problem 16

Given charge distribution on the surface $\sigma=\vec{a} \cdot \vec{r}$ is shown in the figure. Symmetry of this distribution implies that the sought $\vec{E}$ at the centre $O$ of the sphere is opposite to $\vec{a}$ $d q=\sigma(2 \pi r \sin \theta) r d \theta=(\vec{a} \cdot \vec{r}) 2 \pi r^{2} \sin \theta d \theta=2 \pi a r^{3} \sin \theta \cos \theta d \theta$
Again from symmetry, field strength due to any ring element $d E$ is also opposite to $\vec{a}$ i.e. $d \vec{E} \uparrow \downarrow \vec{a}$. Hence
$d \vec{E}=\frac{d q r \cos \theta}{4 \pi \varepsilon_{0}\left(r^{2} \sin ^{2} \theta+r^{2} \cos ^{2} \theta\right)^{3 / 2}} \frac{-\vec{a}}{a}$ (Using the result of 3.9)
$=\frac{\left(2 \pi a r^{3} \sin \theta \cos \theta d \theta\right) r \cos \theta}{4 \pi \varepsilon_{0} r^{3}} \frac{(-\vec{a})}{a}$
$=\frac{-\overrightarrow{a r}}{2 \varepsilon_{0}} \sin \theta \cos ^{2} d \theta$
Thus $\vec{E}=\int d \vec{E}=\frac{(-\vec{a}) r}{2 \varepsilon_{0}} \int_{0}^{\pi} \sin \theta \cos ^{2} \theta d \theta$
Integrating, we get $\vec{E}=-\frac{\overrightarrow{a r}}{2 \varepsilon_{0}} \frac{2}{3}=-\frac{\vec{a} r}{3 \varepsilon_{0}}$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
06:33

Problem 17

We start from two charged spherical balls each of radius $R$ with equal and opposite charge densities $+\rho$ and $-\rho .$ The centre of the balls are at $+\frac{\vec{a}}{2}$ and $-\frac{\vec{a}}{2}$ respectively so the equation of their surfaces are $\left|\vec{r}-\frac{\vec{a}}{2}\right|=R$ or $r-\frac{a}{2} \cos \theta=R$ and $r+\frac{a}{2} \cos \theta \sim R$, considering
$a$ to be small. The distance between the two surfaces in the radial direction at angle $\theta$ is $a \cos \theta \mid$ and does not depend on the azimuthal angle. It is seen from the diagram that the surface of the sphere has in effect a surface density $\sigma=\sigma_{0} \cos \theta$ when
$\sigma_{0}=\rho a .$
Inside any uniformly charged spherical ball, the field is radial and has the magnitude given by Gauss's theorm
or
In vector notation, using the fact the $V$ must be measured from the centre of the ball, we get, for the present case
$$
=-\rho \vec{a} / 3 \varepsilon_{0}=\frac{\sigma_{0}}{3 \varepsilon_{\mathrm{o}}} \vec{k}
$$
When $\vec{k}$ is the unit vector along the polar axis from which $\theta$ is measured.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
01:01

Problem 18

Let us consider an elemental spherical shell of thickness $d r$. Thus surface charge density of the shell $\sigma=\rho d r=(\vec{a} \cdot \vec{r}) d r$
Thus using the solution of $3.16$, field strength due to this sperical shell
$$
d \vec{E}=-\frac{\overrightarrow{a r}}{3 \varepsilon_{0}} d r
$$
Hence the sought field strength
$$
\vec{E}=-\frac{\vec{a}}{3 \varepsilon_{0}} \int_{0}^{R} r d r=-\frac{\vec{a} R^{2}}{6 \varepsilon_{0}}
$$

Narayan Hari
Narayan Hari
Numerade Educator
03:31

Problem 19

From the solution of $3.14$ field strength at a perpendicular distance $r<R$ from its left end $\vec{E}(r)=\frac{\lambda}{4 \pi \varepsilon_{0} r}(-\vec{i})+\frac{\lambda}{4 \pi \varepsilon_{0} r}\left(\hat{e}_{r}\right)$
Here $\hat{e}_{r}$ is a unit vector along radial direction.
Let us consider an elemental surface, $d S=d y d z=d z(r d \theta)$ a $\quad$ figure. Thus flux of $\vec{E}(r)$ over the element $d \vec{S}$ is given by $d \Phi=\vec{E} \cdot d \vec{S}=\left[\frac{\lambda}{4 \pi \varepsilon_{0} r}(\overrightarrow{-i})+\frac{\lambda}{4 \pi \varepsilon_{0} r}\left(\hat{e}_{r}\right)\right] \cdot d r(r d \theta) \vec{i}$
$=-\frac{\lambda}{4 \pi \varepsilon_{0}} d r d \theta\left(\right.$ as $\left.\overrightarrow{e_{r}} \perp \vec{i}\right)$
The sought flux, $\Phi=-\frac{\lambda}{4 \pi \varepsilon_{0}} \int_{0}^{R} d r \int_{0}^{2 \pi} d \theta=-\frac{\lambda R}{2 \varepsilon_{0}}$.
If we have taken $d \vec{S} \uparrow \uparrow(-\vec{i})$, then $\Phi$ were $\frac{\lambda R}{2 \varepsilon_{0}}$
Hence $\quad|\Phi|=\frac{\lambda R}{2 \varepsilon_{0}}$

Narayan Hari
Narayan Hari
Numerade Educator
02:38

Problem 20

Let us consider an elemental surface area as shown in the figure. Then flux of the vector $\vec{E}$ through the elemental area,
$$
\begin{array}{r}
d \Phi=\vec{E} \cdot d \vec{S}=E d S=2 E_{0} \cos \varphi d S(\text { as } \vec{E} \uparrow \uparrow d \vec{S}) \\
=\frac{2 q}{4 \pi \varepsilon_{0}\left(l^{2}+r^{2}\right)} \frac{l}{\left(l^{2}+r^{2}\right)^{1 / 2}}(r d \theta) d r=\frac{2 q l r d r d \theta}{4 \pi \varepsilon_{0}\left(r^{2}+l^{2}\right)^{3 / 2}}
\end{array}
$$
where $E_{0}=\frac{q}{4 \pi \varepsilon_{0}\left(l^{2}+r^{2}\right)}$ is magnitude of field strength due to any point charge at the point of location of considered elemental area. $\boldsymbol{R}$
$2 \pi$
Thus $\Phi=\frac{2 q l}{4 \pi \varepsilon_{0}} \int_{0} \frac{r d r}{\left(r^{2}+l^{2}\right)^{3 / 2}} \int_{0} d \theta$
$\boldsymbol{R}$
$=\frac{2 q l \times 2 \pi}{4 \pi \varepsilon_{0}} \int_{0} \frac{r d r}{\left(r^{2}+l^{2}\right)^{3 / 2}}=\frac{q}{\varepsilon_{0}}\left[1-\frac{l}{\sqrt{l^{2}+R^{2}}}\right]$
It can also be solved by considering a ring element or by using solid angle.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:50

Problem 21

Let us consider a ring element of radius $x$ and thickness $d x$, as shown in the figure. Now, flux over the considered element, $d \Phi=\vec{E} \cdot d \vec{S}=E_{r}$$$
\begin{aligned}
&d \Phi=\vec{E} \cdot d \vec{S}=E_{r} d S \cos \theta\\
&\text { But } E_{r}=\frac{\rho r}{3 \varepsilon_{0}} \text { from Gauss's theorem, }\\
&\text { and } d S=2 \pi x d x, \cos \theta=\frac{r_{0}}{r}\\
&\text { Thus } \quad d \Phi=\frac{\rho r}{3 \varepsilon_{0}} 2 \pi x d x \frac{r_{0}}{r}=\frac{\rho r_{0}}{3 \varepsilon_{0}} 2 \pi x d x\\
&\begin{aligned}
&\text { Hence sought flux } \\
&\qquad \sqrt{R^{2}-r_{0}^{2}}
\end{aligned}\\
&\Phi=\frac{2 \pi \rho r_{0}}{3 \varepsilon_{0}} \int_{0} x d x=\frac{2 \pi \rho r_{0}}{3 \varepsilon_{0}} \frac{\left(R^{2}-r_{0}^{2}\right)}{2}
\end{aligned}
$$ $$
=\frac{\pi \rho r_{0}}{3 \varepsilon_{0}}\left(R^{2}-r_{0}^{2}\right)
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:53

Problem 22

The field at $P$ due to the threads at $A$ and $B$ are both of magnitude $\frac{1}{2 \pi \varepsilon_{0}\left(x^{2}+l^{2} / 4\right)^{1 / 2}}$
and directed along $A P$ and $B P .$ The resultant is along $O P$ with
$$
\begin{aligned}
&E=\frac{2 \lambda \cos \theta}{2 \pi \varepsilon_{0}\left(\pi^{2}+\pi^{1 / 2}\right)^{1 / 2}}=\frac{\lambda x}{\pi \varepsilon_{0}\left(x^{2}+l^{2} / 4\right)}\\
&=\frac{\lambda}{\pi \varepsilon_{0}\left[x+\frac{l^{2}}{4 x}-2 \cdot \frac{l}{2 \sqrt{x}} \cdot \sqrt{x}+l\right]}\\
&=\\
&1\\
&=\frac{\lambda}{\pi \varepsilon_{0}\left[\left(\sqrt{x}-\frac{l}{2 \sqrt{x}}\right)^{2}+l\right]} \quad A\\
&1\\
&\text { This is maximum when } x=l / 2 \text { and then } E=E_{\max }=\frac{\lambda}{\pi \varepsilon_{0} l}
\end{aligned}
$$

Narayan Hari
Narayan Hari
Numerade Educator
02:43

Problem 23

Take a section of the cylinder perpendicular to its axis through the point where the electric field is to be calculated. (All points on the axis are equivalent.) Consider an element $S$ with azimuthal angle $\varphi .$ The length of the element is $R, d \varphi, R$ being the radius of cross section of the cylinder. The element itself is a section of an infinite strip. The electric field at $O$ due to this strip isalong $S O$
This can be resolved into $\frac{\sigma_{0} \cos \varphi d \varphi}{2 \pi \varepsilon_{0}}\left\{\begin{array}{c}\cos \varphi \text { along } O X \text { towards } \\ \sin \varphi \text { along } Y O\end{array}\right.$
On integration the component along vanishes. What remains is
along $X O$ i.e. along the direction $\varphi=\pi$.

Narayan Hari
Narayan Hari
Numerade Educator
02:23

Problem 24

Since the field is axisymmetric (as the field of z uniformly charged filament), we conclude that the flux through the sphere of radius $R$ is equal to the flux through the lateral surface of a cylinder having the same radius and the height $2 R$, as arranged in the figure. Now, $\quad \Phi=\oint \vec{E} \cdot d \vec{S}=E_{r} S$
But $\quad E_{r}=\frac{a}{R}$
Thus $\Phi=\frac{a}{R} S=\frac{a}{R} 2 \pi R \cdot 2 R=4 \pi a R$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
03:27

Problem 25

(a) Let us consider a sphere of radius $r<R$ then charge, inclosed by the considered sphere,
$$
q_{\text {inclased }}=\int_{0}^{r} 4 \pi r^{2} d r \rho=\int_{0}^{r} 4 \pi r^{2} \rho_{0}\left(1-\frac{r}{R}\right) d r
$$
Now, applying Gauss' theorem, $E_{r} 4 \pi r^{2}=\frac{q_{\text {inclased }}}{\varepsilon_{0}}$, (where $E_{r}$ is the projection of electric field along the radial line.)
or,
$$
\begin{gathered}
=\frac{\rho_{0}}{\varepsilon_{0}} \int_{0} 4 \pi r^{2}\left(1-\frac{r}{R}\right) d r \\
E_{r}=\frac{\rho_{0}}{3 \varepsilon_{0}}\left[r^{2}-\frac{3 r^{2}}{4 R}\right]
\end{gathered}
$$
And for a point. outside the sphere $r>R$. $\boldsymbol{R}$
$q_{\text {inclosed }}=\int_{0} 4 \pi r^{2} d r \rho_{0}\left(1-\frac{r}{R}\right)$ (as there is no charge outside the ball) Again from Gauss' theorem,
or,
$$
\begin{gathered}
E_{r} 4 \pi r^{2}=\int_{0}^{R} \frac{4 \pi r^{2} d r \rho_{0}\left(1-\frac{r}{R}\right)}{\varepsilon_{0}} \\
E_{r}=\frac{\rho_{0}}{r^{2} \varepsilon_{0}}\left[\frac{R^{3}}{3}-\frac{R^{4}}{4 R}\right]=\frac{\rho_{0} R^{3}}{12 r^{2} \varepsilon_{0}}
\end{gathered}
$$
(b) As'magnitude of electric field decreases with increasing $r$ for $r>R$, field will be maximum for $r<R .$ Now, for $E_{r}$ to be maximum,
$$
\frac{d}{d r}\left(r-\frac{3 r^{2}}{4 R}\right)=0 \quad \text { or } \quad 1-\frac{3 r}{2 R}=0 \quad \text { or } \quad r=r_{m}=\frac{2 R}{3}
$$
Hence
$$
E_{\max }=\frac{\rho_{0} R}{9 \varepsilon_{0}}
$$

Narayan Hari
Narayan Hari
Numerade Educator
01:47

Problem 26

Let the charge carried by the sphere be $q$, then using Gauss' theorem for a spherical surface having radius $r>R$, we can write.
$E 4 \pi r^{2}=\frac{q_{\text {inclosed }}}{\varepsilon_{0}}=\frac{q}{\varepsilon_{0}}+\frac{1}{\varepsilon_{0}} \int_{R} \frac{\alpha}{r} 4 \pi r^{2} d r$
On integrating we get, $E 4 \pi r^{2}=\frac{\left(q-2 \pi \alpha R^{2}\right)}{\varepsilon_{0}}+\frac{4 \pi \alpha r^{2}}{2 \varepsilon_{0}}$
The intensity $E$ does not depend on $r$ when the experession in the parentheses is equal to zero. Hence
$q=2 \pi \alpha R^{2}$ and $E=\frac{\alpha}{2 \varepsilon_{0}}$

Narayan Hari
Narayan Hari
Numerade Educator
02:03

Problem 27

Let us consider a spherical layer of radius $r$ and thickness $d r$, having its centre coinciding with the centre of the system. Then using Gauss' theorem for this surface,
$$
\begin{gathered}
E_{r} 4 \pi r^{2}=\frac{q_{\text {inclosed }}}{\varepsilon_{0}}=\int_{0} \frac{\rho d V}{\varepsilon_{0}} \\
=\frac{1}{\varepsilon_{0}} \int_{0}^{r} \rho_{0} e^{-\alpha r^{3}} 4 \pi r^{2} d r
\end{gathered}
$$
After integration
$$
\begin{array}{r}
E_{r} 4 \pi r^{2}=\frac{\rho 4 \pi}{3 \varepsilon_{0} \alpha}\left[1-e^{-\alpha r^{3}}\right] \\
\text { or, } \quad E_{r}=\frac{\rho_{0}}{3 \varepsilon \alpha r^{2}}\left[1-e^{-\alpha r^{3}}\right]
\end{array}
$$
Now when $\alpha r^{3}<<1, E_{r}=\frac{\rho_{0} r}{3 \varepsilon_{0}}$
And when $\alpha r^{3}>>1, E_{r} \sim \frac{\rho_{0}}{3 \varepsilon_{0} \alpha r^{2}}$

Narayan Hari
Narayan Hari
Numerade Educator
01:09

Problem 28

Using Gauss theorem we can easily show that the electric field strength within a uniformly. charged sphere is $\vec{E}=\left(\frac{\rho}{3 \varepsilon_{0}}\right) \vec{r}$
The cavity, in our problem, may be considered as the superposition of two balls, one with the charge density $\rho$ and the other with $-\rho$.
Let $P$ be a point inside the cavity such that its position vector with respect to the centre of cavity be $\vec{r}_{-}$ and with respect to the centre of the ball $\overrightarrow{r_{+}}$. Then from the principle of superposition, field inside the cavity, at an arbitrary point $P$ $\vec{E}=\vec{E}_{+}+\vec{E}_{-}$
$=\frac{\rho}{3 \varepsilon_{0}}\left(\overrightarrow{r_{+}}-\overrightarrow{r_{-}}\right)=\frac{\rho}{3 \varepsilon_{0}} \vec{a}$
Note : Obtained expression for $\vec{E}$ shows that it is valid regardless of the ratio between the radii of the sphere and the distance between their centres.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:02

Problem 29

Let us consider a cylinderical Gaussian surface of radius $r$ and height $h$ inside an infinitely long charged cylinder with charge density $\rho$. Now from Gauss theorem :
$E_{r} 2 \pi r h=\frac{q_{\text {inclosed }}}{\varepsilon_{0}}$
(where $E_{r}$ is the field inside the cylinder at a distance $r$ from its axis.)
or, $E_{r} 2 \pi r h=\frac{\rho \pi r^{2} h}{\varepsilon_{0}}$ or $E_{r}=\frac{\rho r}{2 \varepsilon_{0}}$
Now, using the method of $3.28$ field at a point $P$, inside the cavity, is $\vec{E}=\vec{E}_{+}+\overrightarrow{E_{-}}=\frac{\rho}{2 \varepsilon_{0}}\left(\overrightarrow{r_{+}}-\overrightarrow{r_{-}}\right)=\frac{\rho}{2 \varepsilon_{0}} \vec{a}$

Narayan Hari
Narayan Hari
Numerade Educator
02:57

Problem 30

The arrangement of the rings are as shown in the figure. Now, potential at the point 1 , $\varphi_{1}=$ potential at 1 due to the ring $1+$ potential at 1 due to the ring $2 .$
$$
\begin{aligned}
&=\frac{q}{4 \pi \varepsilon_{0} R}+\frac{-q}{4 \pi \varepsilon_{0}\left(R^{2}+a^{2}\right)^{1 / 2}} \\
&\text { ilarly, the potential at point } 2, \\
&P_{2}=\frac{-q}{4 \pi \varepsilon_{0} R}+\frac{q}{4 \pi \varepsilon_{0}\left(R^{2}+a^{2}\right)^{1 / 2}} \\
&\text { ace, the sought potential difference, } \\
&-\varphi_{2}=\Delta \varphi=2\left(\frac{q}{4 \pi \varepsilon_{0} R}+\frac{-q}{4 \pi \varepsilon_{0}\left(R^{2}+a^{2}\right)}\right. \\
&=\frac{q}{2 \pi \varepsilon_{0} R}\left(1-\frac{1}{\sqrt{1+(a / R)^{2}}}\right)
\end{aligned}
$$

Narayan Hari
Narayan Hari
Numerade Educator
01:01

Problem 31

We know from Gauss theorem that the electric field due to an infinietly long straight wire, at a perpendicular distance $r$ from it equals, $E_{r}=\frac{\lambda}{2 \pi \varepsilon_{0} r} .$ So, the work done is
$$
\int_{1}^{2} E_{r} d r=\int_{x}^{\eta x} \frac{\lambda}{2 \pi \varepsilon_{0} r} d r
$$
(where $x$ is perpendicular distance from the thread by which point 1 is removed from it.)
Hence
$$
\Delta \varphi_{12}=\frac{\lambda}{2 \pi \varepsilon_{0}} \ln \eta
$$

Narayan Hari
Narayan Hari
Numerade Educator
03:07

Problem 32

Let us consider a ring element as shown in the figure. Then the charge, carried by the element, $d q=(2 \pi R \sin \theta) R d \theta \sigma$
Hence, the potential due to the considered element at the centre of the hemisphere, $d \varphi=\frac{1}{4 \pi \varepsilon_{0}} \frac{d q}{R}=\frac{2 \pi \sigma R \sin \theta d \theta}{4 \pi \varepsilon_{0}}=\frac{\sigma R}{2 \varepsilon_{0}} \sin \theta d \theta$
So potential due to the whole hemisphere
Now from the symmetry of the problem, net electric field of the hemisphere is directed towards the negative $y$ -axis. We have $d E_{y}=\frac{1}{4 \pi \varepsilon_{0}} \frac{d q \cos \theta}{R^{2}}=\frac{\sigma}{2 \varepsilon_{0}} \sin \theta \cos \theta d \theta$
Thus $E=E_{y}^{\prime}=\frac{\sigma}{2 \varepsilon_{0}} \int_{0}^{\pi / 2} \sin \theta \cos \theta d \theta=\frac{\sigma}{4 \varepsilon_{0}} \int_{0}^{\pi / 2} \sin 2 \theta d \theta=\frac{\sigma}{4 \varepsilon_{0}}$, along $Y O$

Narayan Hari
Narayan Hari
Numerade Educator
02:49

Problem 33

Let us consider an elementary ring of thickness $d y$ and radius $y$ as shown in the figure. Then potential at a point $P$, at distance $l$ from the centre of the disc, is
$$
d \varphi=\frac{\sigma 2 \pi y d y}{4 \pi \varepsilon_{0}\left(y^{2}+l^{2}\right)^{1 / 2}}
$$
Hence potential due to the whole disc, $\varphi=\int_{0}^{R} \frac{\sigma 2 \pi y d y}{4 \pi \varepsilon_{0}\left(y^{2}+l^{2}\right)^{1 / 2}}=\frac{\sigma l}{2 \varepsilon_{0}}\left(\sqrt{1+(R / l)^{2}}-1\right)$
From symmetry
$$
\begin{gathered}
E=E_{l}=-\frac{d \varphi}{d l} \\
=-\frac{\sigma}{2 \varepsilon_{0}}\left[\frac{2 l}{2 \sqrt{R^{2}+l^{2}}}-1\right]=\frac{\sigma}{2 \varepsilon_{0}}\left[1-\frac{1}{\sqrt{1+(R / l)^{2}}}\right]
\end{gathered}
$$
when $l \rightarrow 0, \varphi=\frac{\sigma R}{2 \varepsilon_{0}}, E=\frac{\sigma}{2 \varepsilon_{0}}$ and when $l>>R$,
$$
\varphi=\frac{\sigma R^{2}}{4 \varepsilon_{0} l}, E=\frac{\sigma R^{2}}{4 \varepsilon_{0} l^{2}}
$$

Narayan Hari
Narayan Hari
Numerade Educator
01:54

Problem 34

By definition, the potential in the case of a surface charge distribution is defined by integral $\varphi=\frac{1}{4 \pi \varepsilon_{0}} \int \frac{\sigma d S}{r}$. In order to simplify integration, we shall choose the area element $d S$ in the form of a part of the ring of radius $r$ and width $d r$ in (Fig.). Then $d S=2 \theta r d r$, $r=2 R \cos \theta$ and $d r=-2 R \sin \theta d \theta .$ After substituting these expressions into integral $\varphi=\frac{1}{4 \pi \varepsilon_{0}} \int \frac{\sigma d S}{r}$, we obtain the expression for $\varphi$ at the point $O$ :
$\varphi=-\frac{\sigma R}{\pi \varepsilon_{0}} \int_{N / 2} \theta \sin \theta d \theta$
$d r$
We integrate by parts, denoting $\theta=u$ and $\sin \theta d \theta=d v:$
$$
\int \theta \sin \theta d \theta=-\theta \cos \theta
$$
$+\int \cos \theta d \theta=-\theta \cos \theta+\sin \theta$
which gives $-1$ after substituting the limits of integration. As a result, we obtain
$$
\varphi=\sigma R / \pi \varepsilon_{0^{\circ}}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
01:17

Problem 35

In accordance with the problem $\varphi=\vec{a} \cdot \vec{r}$ Thus from the equation $: \vec{E}=-\vec{\nabla} \varphi$ $\vec{E}=-\left[\frac{\partial}{\partial x}\left(a_{x} x\right) \vec{i}+\frac{\partial}{\partial_{y}}\left(a_{y} y\right) \vec{j}+\frac{\partial}{\partial_{z}}\left(a_{z} z\right) \vec{k}\right]=-\left[a_{x} \vec{i}+a_{y} \vec{j}+{ }_{z} \vec{k}\right]=-\vec{a}$

Narayan Hari
Narayan Hari
Numerade Educator
01:17

Problem 36

(a) Given, $\varphi=a\left(x^{2}-y^{2}\right) \overrightarrow{\vec{E}}=-\vec{\nabla} \varphi=-2 a(x \vec{i}-y \vec{j})$
The sought shape of field lines is as shown in the figure (a) of answersheet assuming $a>0:$
$\begin{aligned}&\text { (b) Since } \varphi=a x y \\&\text { So, }\end{aligned} \quad \vec{E}=-\vec{\nabla} \varphi=-a y \vec{i}-a x \vec{j}$
Plot as shown in the figure (b) of answersheet.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
07:54

Problem 37

Given, $\varphi=a\left(x^{2}+y^{2}\right)+b z^{2}$
So, $\vec{E}=-\vec{\nabla} \varphi=-[2 a x \overrightarrow{i+2} a y \overrightarrow{j+2} b z \vec{k}]$
Hence $|\vec{E}|=2 \sqrt{a^{2}\left(x^{2}+y^{2}\right)+b^{2} z^{2}}$
Shape of the equipotential surface :
Put $\vec{\rho}=x \overrightarrow{i+} y \vec{j}$ or $\rho^{2}=x^{2}+y^{2}$
Then the equipotential surface has the equation
$$
a \rho^{2}+b z^{2}=\text { constant }=\varphi
$$
If $a>0, b>0$ then $\varphi>0$ and the equation of the equipotential surface is
$$
\frac{\rho}{\varphi / a}+\frac{z^{2}}{\varphi / b}=1
$$
which is an ellipse in $\rho, z$ coordinates. In three dimensions the surface is an ellipsoid of revolution with semi- axis $\sqrt{\varphi / a}, \sqrt{\varphi / a}, \sqrt{\varphi / b}$
If $a>0, b<0$ then $\varphi$ can be $\geq 0$. If $\varphi>0$ then the equation is
$$
\frac{\rho^{2}}{\varphi / a}-\frac{z^{2}}{\varphi /|b|}=1
$$
This is a single cavity hyperboloid of revolution about $z$ axis. If $\varphi=0$ then
or
$$
\begin{aligned}
&a \rho^{2}-|b| z^{2}=0 \\
&z=\pm \sqrt{\frac{a}{|b|}} \rho
\end{aligned}
$$
is the equation of a right circular cone.
If $\varphi<0$ then the equation can be written as
or
$$
\begin{gathered}
|b| z^{2}-a \rho^{2}=|\varphi| \\
\frac{z^{2}}{|\varphi| /|b|}-\frac{\rho^{2}}{|\varphi| / a}=1
\end{gathered}
$$
This is a two cavity hyperboloid of revolution about $z$ -axis.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:04

Problem 38

From Gauss' theorem intensity at a point, inside the sphere at a distance $r$ from the centre is given by, $E_{r}=\frac{\rho r}{3 \varepsilon_{0}}$ and outside it, is given by $E_{r}=\frac{1}{4 \pi \varepsilon_{0}} \frac{q}{r^{2}}$
(a) Potential at the centre of the sphere,
$$
\varphi_{0}=\int_{0}^{\infty} \vec{E} \cdot d \vec{r}=\int_{0}^{R} \frac{\rho r}{3 \varepsilon_{0}} d r+\int_{R}^{\infty} \frac{q}{4 \pi \varepsilon_{0} r^{2}} d r=\frac{\rho}{3 \varepsilon} \frac{R^{2}}{2}+\frac{q}{4 \pi \varepsilon_{0} R}
$$
as
$$
=\frac{q}{8 \pi \varepsilon_{0} R}+\frac{q}{4 \pi \varepsilon_{0} R}=\frac{3 q}{8 \pi \varepsilon_{0} R}\left(\text { as } \rho=\frac{3 q}{4 \pi R^{3}}\right)
$$
(b) Now, potential at any point, inside the sphere, at a distance $r$ from it s centre.
$$
\varphi(r)=\int_{r}^{R} \frac{\rho}{3 \varepsilon_{0}} r d r \int_{r}^{\infty} \frac{q}{4 \pi \varepsilon_{0}} \frac{d r}{r^{2}}
$$
On integration : $\varphi(r)=\frac{3 q}{8 \pi \varepsilon_{0} R}\left[1-\frac{r^{2}}{3 R^{2}}\right]=\varphi_{0}\left[1-\frac{r^{2}}{3 R^{2}}\right]$

Narayan Hari
Narayan Hari
Numerade Educator
03:18

Problem 39

Let two charges $+q$ and $-q$ be separated by a distance $l$. Then electric potential at a point at distance $r>>l$ from this dipole,
$$
\varphi(r)=\frac{+q}{4 \pi \varepsilon_{0} r_{+}}+\frac{-q}{4 \pi \varepsilon_{0} r_{-}}=\frac{q}{4 \pi \varepsilon_{0}}\left(\frac{r_{-}-r_{+}}{r_{+} r_{-}}\right)
$$
But
From
where
and Now,
So $\quad E=\sqrt{E_{r}^{2}+E_{0}^{2}}=\frac{p}{4 \pi \varepsilon_{0} r^{3}} \sqrt{4 \cos ^{2} \theta+\sin ^{2} \theta}$

Narayan Hari
Narayan Hari
Numerade Educator
03:25

Problem 40

From the results, obtained in the previous problem,
$$
E_{r}=\frac{2 p \cos \theta}{4 \pi \varepsilon_{0} r^{3}} \text { and } E_{\theta}=\frac{p \sin \theta}{4 \pi \varepsilon_{0} r^{3}}
$$
From the given figure, it is clear that,
$$
E_{z}=E_{r} \cos \theta-E_{\theta} \sin \theta=\frac{p}{4 \pi \varepsilon_{0} r^{3}}\left(3 \cos ^{2} \theta-1\right)
$$
and $\quad E_{\perp}=E_{r} \sin \theta+E_{0} \cos \theta=\frac{3 p \sin \theta \cos \theta}{4 \pi \varepsilon_{0} r^{3}}$
When
$$
\vec{E} \perp \vec{p}, \vec{E} \mid=E_{\perp} \text { and } E_{z}=0
$$
So
$$
3 \cos ^{2} \theta=1 \text { and } \cos \theta=\frac{1}{\sqrt{3}}
$$
Thus $\vec{E}_{\perp} \vec{p}$ at the points located on the lateral surface of the cone, having its axis, coinciding with the direction of $z$ -axis and semi vertex angle $\theta=\cos ^{-1} 1 / \sqrt{3}$.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
01:58

Problem 41

Let us assume that the dipole is at the centre of the one equipotential surface which is spherical (Fig.). On an equipotential surface the net electric field strength along the tangent of it becomes zero. Thus $-E_{0} \sin \theta+E_{\theta}=0 \quad$ or $-E_{0} \sin \theta+\frac{p \sin \theta}{4 \pi \varepsilon_{0} r^{3}}=0$
Hence $\quad r=\left(\frac{p}{4 \pi \varepsilon_{0} E_{0}}\right)^{1 / 3}$
Alternate : Potential at the point, near the dipole is given by, $\varphi=\frac{\vec{p} \cdot \vec{r}}{4 \pi \varepsilon_{0} r^{3}}-\vec{E}_{0} \cdot \vec{r}+$ constant,
$=\left(\frac{p}{4 \pi \varepsilon_{0} r^{3}}-E_{0}\right) \cos \theta+$ Const
For $\varphi$ to be constant,
$\frac{p}{4 \pi \varepsilon_{0} r^{3}}-E_{0}=0$ or, $\frac{p}{4 \pi \varepsilon_{0} r^{3}}=E_{0}$
Thus $r=\left(\frac{p}{4 \pi \varepsilon_{0} E_{0}}\right)^{1 / 3}$

Narayan Hari
Narayan Hari
Numerade Educator
03:41

Problem 42

$$
\begin{aligned}
&\text { Let } P \text { be a point, at distace } r>>l \text { and at an angle to } \theta \text { the vector } l \text { (Fig.). }\\
&\text { Thus } \vec{E} \text { at } P=\frac{\lambda}{2 \pi \varepsilon_{0}} \frac{\vec{r}+\frac{\vec{l}}{2}}{\left|\vec{r}+\frac{\vec{l}}{2}\right|^{2}}-\frac{\lambda}{2 \pi \varepsilon_{0}} \frac{\vec{r}-\frac{\vec{l}}{2}}{\left|\vec{r}-\frac{\vec{l}}{2}\right|^{2}}
\end{aligned}
$$
$$
\text { Also, } \quad \begin{aligned}
&\left.\varphi=\frac{\lambda}{2 \pi \varepsilon_{0}} \ln |\vec{r}+\vec{l} / 2|-\frac{\lambda}{2 \pi \varepsilon_{0}} \ln \mid \vec{r}-\vec{l} / 2\right] \\
=& \frac{\lambda}{4 \pi \varepsilon_{0}} \ln \frac{r^{2}+r l \cos \theta+l^{2} / 4}{r^{2}-r l \cos \theta+l^{2} / 4}=\frac{\lambda l \cos \theta}{2 \pi \varepsilon_{0} r}, r>>l
\end{aligned}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
04:17

Problem 43

The potential can be calculated by superposition. Choose the plane of the upper ring as $x=l / 2$ and that of the lower ring as $x=-l / 2$
For $\quad|x|>>R, \varphi \sim \frac{q l}{4 \pi x^{2}}$
The electric field is $E=-\frac{\partial \varphi}{\partial x}$
$$
=-\frac{q l}{4 \pi \varepsilon_{0}\left(R^{2}+x^{2}\right)^{3 / 2}}+\frac{3}{2} \frac{q l}{\left(R^{2}+x^{2}\right)^{5 / 2} 4 \pi \varepsilon_{0}} \times 2 x=\frac{q l\left(2 x^{2}-R^{2}\right)}{4 \pi \varepsilon_{0}\left(R^{2}+x^{2}\right)^{5 / 2}}
$$
For $\quad|x|>>R, E \sim \frac{q l}{2 \pi \varepsilon-r^{3}} . \quad$ The plot is as given in the book.

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
03:35

Problem 44

The field of a pair of oppositely charged sheets with holes can by superposition be reduced to that of a pair of uniform opposite charged sheets and discs with opposite charges. Now the charged sheets do not contribute any field outside them. Thus using the result of the previous problem
$$
\begin{aligned}
&\varphi=\int_{0} \frac{(-\sigma) l 2 \pi r d r x}{4 \pi \varepsilon_{0}\left(r^{2}+x^{2}\right)^{3 / 2}}\\
&R^{2}+x^{2}\\
&=-\frac{\sigma x l}{4 \varepsilon_{0}} \int_{x^{2}} \frac{d y}{y^{3 / 2}}=\frac{\sigma x l}{2 \varepsilon_{0} \sqrt{R^{2}+x^{2}}} \quad+6\\
&E_{x}=-\frac{\partial \varphi}{\partial x}=-\frac{\sigma l}{2 \varepsilon_{0}}\left[\frac{i}{\sqrt{R^{2}+x^{2}}}-\frac{x^{2}}{\left(R^{2}+x^{2}\right)^{3 / 2}}\right]=-\frac{\sigma l R^{2}}{2 \varepsilon_{0}\left(R^{2}+x^{2}\right)^{3 / 2}}\\
&\text { The plot is as shown in the answersheet. }
\end{aligned}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
01:44

Problem 45

For $x>0$ we can use the result as given above and write
$$
\varphi \sim \pm \frac{\sigma l}{2 \varepsilon_{0}}\left(1-\frac{|x|}{\left(R^{2}+x^{2}\right)^{1 / 2}}\right)
$$
for the solution that vanishes at $\alpha$. There is a discontinuity in potential for $|x|=0$. The solution for negative $x$ is obtained by $\sigma \rightarrow-\sigma$. Thus
$$
\varphi=-\frac{\sigma l x}{2 \varepsilon_{0}\left(R+x^{2}\right)^{1 / 2}}+\text { constant }
$$
Hence ignoring the jump
$$
E=-\frac{\partial \varphi}{\partial x}=\frac{\sigma l R^{2}}{2 \varepsilon_{0}\left(R^{2}+x^{2}\right)^{3 / 2}}
$$
for large $|x| \quad \varphi \sim \pm \frac{p}{4 \pi \varepsilon_{0} x^{2}}$ and $E=\frac{p}{2 \pi \varepsilon_{0}|x|^{3}}$ (where $p=\pi R^{2} \sigma l$ )

Narayan Hari
Narayan Hari
Numerade Educator
02:32

Problem 46

Here $E_{r}=\frac{\lambda}{2 \pi \varepsilon_{0} r}, E_{\theta}=E_{\varphi}=0$ and $\vec{F}=p \frac{\partial \vec{E}}{\partial l}$
(a) $\vec{p}$ along the thread.
$E$ does not change as the point of observation is moved along the thread.
$$
\vec{F}=0
$$
(b) $\vec{p}$ along $\vec{r}$
$$
\vec{F}=F_{r} \overrightarrow{e_{r}}=\frac{\lambda p}{2 \pi \varepsilon_{0} r^{2}} \overrightarrow{e_{r}}=-\frac{\lambda \vec{p}}{2 \pi \varepsilon_{0} r^{2}}\left(\text { On using } \frac{\partial}{\partial r} \overrightarrow{e_{r}}=0\right)
$$
(c) $\vec{p}$ along $\overrightarrow{e_{\theta}}$
$$
\begin{gathered}
\vec{F}=p \frac{\partial}{r \partial \theta} \frac{\lambda}{2 \pi \varepsilon_{0} r} e_{r} \\
=\frac{p \lambda}{2 \pi \varepsilon_{0} r^{2}} \frac{\partial \vec{e}_{r}}{\partial \theta}=\frac{p \lambda}{2 \pi \varepsilon_{0} r^{2}} \vec{e}_{\theta}=\frac{\vec{p} \lambda}{2 \pi \varepsilon_{0} r^{2}} .
\end{gathered}
$$

Narayan Hari
Narayan Hari
Numerade Educator
01:10

Problem 47

Force on a dipole of moment $p$ is given by,
$$
F=\left|\varphi \frac{\partial \vec{E}}{\partial l}\right|
$$
In our problem, field, due to a dipole at a distance $l$, where a dipole is placed,
$$
|\vec{E}|=\frac{p}{2 \pi \varepsilon_{0} l^{3}}
$$
Hence, the force of interaction,
$$
F=\frac{3 p^{2}}{2 \pi \varepsilon_{0} l^{4}}=2 \cdot 1 \times 10^{-16} \mathrm{~N}
$$

Narayan Hari
Narayan Hari
Numerade Educator
01:02

Problem 48

$$
\begin{aligned}
&-d \varphi=\vec{E} \cdot d \vec{r}=a(y d x+x d y)=a d(x y)\\
&\text { On integrating, }\\
&\varphi=-a x y+C
\end{aligned}
$$

Narayan Hari
Narayan Hari
Numerade Educator
01:40

Problem 49

$$
\begin{aligned}
&-d \varphi=\vec{E} \cdot d r=\left[2 a x y \vec{i}+2\left(x^{2}-y^{2}\right) \vec{j}\right] \cdot[d x \vec{i}+d y \vec{j}] \\
&\text { or, } \quad d \varphi=2 a x y d x+a\left(x^{2}-y^{2}\right) d y=a d\left(x^{2} y\right)-a y^{2} d y
\end{aligned}
$$On integrating, we get,
$$
\varphi=a y\left(\frac{y^{2}}{3}-x^{2}\right)+C
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
01:50

Problem 50

Given, again
$$
\begin{aligned}
-d \varphi &=\vec{E} \cdot d \vec{r}=(a y \vec{i}+(a x+b z) \vec{j}+b y \vec{k}) \cdot(d x \vec{i}+d y \vec{j}+d x \vec{k}) \\
&=a(y d x+a x d y)+b(z d y+y d z)=a d(x y)+b d(y z)
\end{aligned}
$$
On integrating,
$$
\varphi=-(a x y+b y z)+C
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
00:54

Problem 51

Field intensity along $x$ -axis.
$$
E_{x}=-\frac{\partial \varphi}{\partial x}=3 a x^{2}
$$
Then using Gauss's theorem in differential from
$$
\frac{\partial E_{x}}{\partial x}=\frac{\rho(x)}{\varepsilon_{0}} \text { so, } \rho(x)=6 a \varepsilon_{0} x .
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:53

Problem 52

In the space between the plates we have the Poisson equation
or,
$$
\begin{array}{r}
\frac{\partial^{2} \varphi}{\partial x^{2}}=-\frac{\rho_{0}}{\varepsilon_{0}} \\
\varphi=-\frac{\rho_{0}}{2 \varepsilon_{0}} x^{2}+A x+B
\end{array}
$$
where $\rho_{0}$ is the constant space charge density between the plates. We can choose $\quad \varphi(0)=0$ so $B=0$
Then $\varphi(d)=\Delta \varphi=A d-\frac{\rho_{0} d^{2}}{2 \varepsilon_{0}}$
or, $A=\frac{\Delta \varphi}{d}+\frac{\rho_{0} d}{2 \varepsilon_{0}}$
Now $\quad E=-\frac{\partial \varphi}{\partial x}=\frac{\rho_{0}}{\varepsilon_{0}} x-A=0$ for $x=0$
if $\quad A=\frac{\Delta \varphi}{d}+\frac{\rho_{0} d}{2 \varepsilon_{0}}=0$
then
$$
\rho_{0}=-\frac{2 \varepsilon_{0} \Delta \varphi}{d^{2}}
$$
Also
$$
E(d)=\frac{\rho_{0} d}{\varepsilon_{0}}
$$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator
02:15

Problem 53

Field intensity is along radial line and is
$$
E_{r}=-\frac{\partial \varphi}{\partial r}=-2 a r
$$
From the Gauss' theorem,
$$
4 \pi r^{2} E_{r}=\int \frac{d q}{\varepsilon_{0,}}
$$
where $d q$ is the charge contained between the sphere of radii $r$ and $r+d r$.
Hence
$$
4 \pi r^{2} E_{r}=4 \pi r^{2} \times(-2 a r)=\frac{4 \pi}{\varepsilon_{0}} \int_{0}^{r} r^{\prime 2} \rho\left(r^{\prime}\right) d r^{\prime}
$$
Differentiating $(2) \rho=-6 \varepsilon_{0} a$

Khoobchandra Agrawal
Khoobchandra Agrawal
Numerade Educator