A jar of height $h$ is filled with a transparent liquid of refractive index $\propto$ figure. At the centre of the jar on the bottom surface is a dot. Find the minimum diameter of a disc, such that when placed on the top surface symmetrically about the centre, the dot is invisible.
Let $d$ be the diameter of the disc. The spot shall be invisible if the incident rays from the dot at $O$ to the surface at $d / 2$ at the critical angle.
Let $i$ be the angle of incidence.
Using relationship between refractive index and critical angle, then,
$$\sin t=\frac{1}{\propto}$$
Using geometry and trigonometry.
Now,
$$\begin{aligned} \frac{d / 2}{h} & =\tan i \\ \Rightarrow\quad\frac{d}{2} & =h \tan i=h\left[\sqrt{\alpha^2-1}\right]^{-1} \\ \therefore\quad d & =\frac{2 h}{\sqrt{\alpha^2-1}} \end{aligned}$$
This is the required expression of $d$.
A myopic adult has a far point at 0.1 m . His power of accomodation is 4 D.
(i) What power lenses are required to see distant objects?
(ii) What is his near point without glasses?
(iii) What is his near point with glasses? (Take the image distance from the lens of the eye to the retina to be 2 cm .)
(i) Let the power at the far point be $P_f$ for the normal relaxed eye of an average person. The required power
$$P_f=\frac{1}{f}=\frac{1}{0.1}+\frac{1}{0.02}=60 \mathrm{D}$$
By the corrective lens the object distance at the far point is $\infty$.
The power required is
$$P_f^{\prime}=\frac{1}{f^{\prime}}=\frac{1}{\infty}+\frac{1}{0.02}=50 \mathrm{D}$$
So for eye + lens system,
we have the sum of the eye and that of the glasses $P_g$
$$\begin{array}{lr} \therefore & P_f^{\prime}=P_f+P_g \\ \therefore & P_g=-10 \mathrm{D} \end{array}$$
(ii) His power of accomodatlon is 4 D for the normal eye. Let the power of the normal eye for near vision be $P_n$.
Then,
$$4=P_n-P_f \text { or } P_n=64 \mathrm{D}$$
Let his near point be $x_n$, then
$$\begin{aligned} \frac{1}{x_n}+\frac{1}{0.02} & =64 \text { or } \frac{1}{x_n}+50=64 \\ \frac{1}{x_n} & =14 \end{aligned}$$
$$\therefore \quad x_n=\frac{1}{14} ; 0.07 \mathrm{~m}$$
(iii) With glasses $P_n^{\prime}=P_f^{\prime}+4=54$
$$\begin{aligned} & 54=\frac{1}{x_n^{\prime}}+\frac{1}{0.02}=\frac{1}{x_n^{\prime}}+50 \\ & \frac{1}{x_n^{\prime}}=4 \\ \therefore\quad & x_n^{\prime}=\frac{1}{4}=0.25 \mathrm{~m} \end{aligned}$$
Show that for a material with refractive index $\propto \geq \sqrt{2}$, light incident at any angle shall be guided along a length perpendicular to the incident face.
Any ray entering at an angle $i$ shall be guided along $A C$ if the angle ray makes with the face $A C(\phi)$ is greater than the critical angle as per the principle of total internal reflection $\phi+r=902$, therefore $\sin \phi=\cos r$
$$\begin{array}{lc} \Rightarrow & \sin \phi \geq \frac{1}{\alpha} \\ \Rightarrow & \cos r \geq \frac{1}{\alpha} \\ \text { or } & 1-\cos ^2 r \leq 1-\frac{1}{\alpha^2} \\ \text { i.e., } & \sin ^2 r \leq \frac{1}{\alpha^2} \\ \text { i.e., } & \sin ^2 r \leq 1-\frac{1}{\alpha^2} \end{array}$$
$$\begin{aligned} \text{since,}\quad\sin i & =\alpha \sin r \\ \frac{1}{\alpha_2} \sin ^2 i & \leq 1-\frac{1}{\alpha^2} \text { or } \sin ^2 i \leq \alpha^2-1 \end{aligned}$$
when $$i=\frac{\pi}{2}$$
Then, we have smallest angle $\phi$.
If that is greater than the critical angle, then all other angles of incidence shall be more than the critical angle.
Thus,
$$\begin{aligned} 1 & \leq \alpha^2-1 \\ \text{or}\quad\alpha^2 & \geq 2 \\ \Rightarrow\quad\alpha & \geq \sqrt{2} \end{aligned}$$
This is the required result.
The mixture a pure liquid and a solution in a long vertical column (i.e., horizontal dimensions $\ll<$ vertical dimensions) produces diffusion of solute particles and hence a refractive index gradient along the vertical dimension. A ray of light entering the column at right angles to the vertical is deviated from its original path. Find the deviation in travelling a horizontal distance $d \ll h$, the height of the column.
Let us consider a portion of a ray between $x$ and $x+d x$ inside the liquid. Let the angle of incidence at $x$ be $\theta$ and let it enter the thin column at height $y$. Because of the bending it shall emerge at $x+d x$ with an angle $\theta+d \theta$ and at a height $y+d y$. From Snell's law,
$\alpha(y) \sin \theta=\alpha(y+d y) \sin (\theta+d \theta)$
$$\begin{gathered} \text{or}\quad\alpha(y) \sin \theta ;\left(\alpha(y)+\frac{d \alpha}{d y} d y\right)(\sin \theta \cos d \theta+\cos \theta \sin d \theta) \\ \text{or}\quad\alpha(y) \sin \theta+\alpha(y) \cos \theta d \theta+\frac{d \alpha}{d y} d y \sin \theta \\ \text{or}\quad\alpha(y) \cos \theta d \theta ; \frac{-d \alpha}{d y} d y \sin \theta \end{gathered}$$
$$\begin{gathered} d \theta ; \frac{-d \propto}{\alpha d y} d y \tan \theta \\ \text{But}\quad\tan \theta=\frac{d x}{d y}\text{(from the figure)} \end{gathered}$$
On solving, we have
$$\therefore \quad d \theta=\frac{-1 d \alpha}{\alpha d y} d x$$
Solving this variable separable form of differential equation.
$$\therefore \quad \theta=\frac{-1 d \alpha}{\alpha d y} \int_0^d d x=\frac{-1 d \propto}{\alpha d y} d$$
If light passes near a massive object, the gravitational interaction causes a bending of the ray. This can be thought of as happening due to a change in the effective refractive index of the medium given by
$$n(r)=1+2 G M / r c^2$$
where $r$ is the distance of the point of consideration from the centre of the mass of the massive body, $G$ is the universal gravitational constant, $M$ the mass of the body and $c$ the speed of light in vacuum. Considering a spherical object find the deviation of the ray from the original path as it grazes the object.
Let us consider two planes at $r$ and $r+d r$. Let the light be incident at an angle $\theta$ at the plane at $r$ and leave $r+d r$ at an angle $\theta+d \theta$. Then from Snell's law,
$$\begin{gathered} n(r) \sin \theta=n(r+d r) \sin (\theta+d \theta) \\ \Rightarrow \quad n(r) \sin \theta ;\left(n(r)+\frac{d n}{d r} d r\right)(\sin \theta \cos d \theta+\cos \theta \sin d \theta) \\ ;\left(n(r)+\frac{d n}{d r} d r\right)(\sin \theta+\cos \theta d \theta) \end{gathered}$$
Ignoring the product of differentials or we have,
$$\begin{aligned} n(r) \sin \theta ; n(r) \sin \theta & +\frac{d n}{d r} d r \sin \theta+n(r) \cos \theta d \theta \\ -\frac{d n}{d r} \tan \theta & =n(r) \frac{d \theta}{d r} \\ \frac{2 G M}{r^2 c^2} \tan \theta & =\left(1+\frac{2 G M}{r c^2}\right) \frac{d \theta}{d r} \approx \frac{d \theta}{d r} \\ \int_0^{\theta_0} d \theta & =\frac{2 G M}{c^2} \int_{-\infty}^{\infty} \frac{\tan \theta d r}{r^2} \end{aligned}$$
Now substitution for integrals, we have
Now, $r^2=x^2+R^2$ and $\tan \theta=\frac{R}{x}$
$$\begin{aligned} 2 r d r & =2 x d x \\ \int_0^{\theta_0} d \theta & =\frac{2 G M}{c^2} \int_{-\infty}^{\infty} \frac{R}{x} \frac{x d x}{\left(x^2+R^2\right)^{\frac{3}{2}}} \end{aligned}$$
$$\begin{aligned} \text{Put}\quad x & =R \tan \phi \\ d x & =R \sec ^2 \phi d \phi \\ \therefore\quad\theta_0 & =\frac{2 G M R}{c^2} \int_{-\pi / 2}^{\pi / 2} \frac{R \sec ^2 \phi d \phi}{R^3 \sec ^3 \phi} \\ & =\frac{2 G M}{R c^2} \int_{-\pi / 2}^{\pi / 2} \cos \phi d \phi=\frac{4 G M}{R c^2} \end{aligned}$$
This is the required proof.