Option 1: Lens maker's (focal length) formula
Step 1: Setup.
Consider a thin lens of material refractive index \( n \) (with respect to the surrounding medium) bounded by two spherical surfaces of radii of curvature \( R_1 \) and \( R_2 \). Let an object O lie on the principal axis. We use the refraction-at-a-single-spherical-surface formula twice.
Step 2: Refraction at the first surface.
For refraction from medium 1 (\( n_1=1 \)) into the lens (\( n_2=n \)) at a surface of radius \( R_1 \), the image would form at \( v_1 \):
\[ \frac{n}{v_1} - \frac{1}{u} = \frac{n-1}{R_1} \quad\text{...(1)} \]
Step 3: Refraction at the second surface.
The image \( I_1 \) at \( v_1 \) acts as the object for the second surface (radius \( R_2 \)), where light goes from the lens (\( n \)) back to the outside medium (\( 1 \)). For a thin lens the thickness is neglected, so the object distance is \( v_1 \):
\[ \frac{1}{v} - \frac{n}{v_1} = \frac{1-n}{R_2} \quad\text{...(2)} \]
Step 4: Add equations (1) and (2).
The \( n/v_1 \) terms cancel:
\[ \frac{1}{v} - \frac{1}{u} = (n-1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) \]
Step 5: Introduce focal length.
By definition, when the object is at infinity (\( u\to\infty \)) the image forms at the focus, \( v=f \). Also for any object \( \dfrac{1}{v}-\dfrac{1}{u}=\dfrac{1}{f} \). Hence:
\[ \frac{1}{f} = (n-1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) \]
This is the lens maker's formula giving the focal length of a thin lens.
\[\boxed{\dfrac{1}{f} = (n-1)\left(\dfrac{1}{R_1} - \dfrac{1}{R_2}\right)}\]
Option 2: Diffraction vs interference and fringe width
Step 1: Difference between interference and diffraction.
(i) Interference is the superposition of light from two (or more) separate coherent sources; diffraction is the superposition of the secondary wavelets coming from different parts of the same wavefront (a single slit/obstacle).
(ii) In interference all bright fringes are of equal width and equal intensity; in diffraction the central maximum is the brightest and widest, and the intensity of side maxima falls off rapidly.
(iii) In interference the dark fringes are almost perfectly dark; in diffraction the minima are not perfectly dark.
Step 2: Fringe width formula (YDSE).
\[ \beta = \frac{\lambda D}{d} \]
where \( \lambda \) is the wavelength, \( D \) the slit-to-screen distance and \( d \) the separation between the slits.
Step 3: Change the geometry.
New separation \( d' = \dfrac{d}{3} \) and new distance \( D' = 2D \). New fringe width:
\[ \beta' = \frac{\lambda D'}{d'} = \frac{\lambda (2D)}{d/3} = 6\,\frac{\lambda D}{d} = 6\beta \]
So the fringe width becomes six times the original.
Step 4: Immerse the apparatus in water.
In a medium of refractive index \( n_w \) the wavelength becomes \( \lambda' = \lambda/n_w \), so:
\[ \beta'' = \frac{\lambda' D}{d} = \frac{\beta}{n_w} \]
With \( n_w = 1.33 \), the fringe width reduces to about \( \beta/1.33 \approx 0.75\beta \), i.e. the fringes come closer together.
\[\boxed{\beta'=6\beta;\qquad \beta_{water}=\beta/n_w\approx 0.75\beta}\]