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In Young’s double slit experiment, the fringe width is \(\beta\). If the entire arrangement is placed in a liquid of refractive index \(n\), then the fringe width becomes
(c) We have, \(\beta=\frac{\lambda D}{d}\)
\(\because \quad\) The arrangement is placed in a liquid of refractive index \(n\).
\(
\therefore \quad \lambda^{\prime}=\frac{\lambda}{n}
\)
Therefore, fringe width, \(\beta^{\prime}=\frac{\lambda D}{d n}\)
\(
\beta^{\prime}=\frac{\beta}{n}
\)
In Young’s double slit experiment, the angular width of a fringe formed on a distant screen is \(1^{\circ}\), the wavelength of light used is \(6000 Å\). The spacing between the slits is
\(
\begin{array}{ll}
\text { (c) } \theta(\text { in radian }) & =\frac{\lambda}{d} \\
\therefore \quad d =\frac{\lambda}{\theta}=\frac{6 \times 10^{-7}}{\pi / 180^{\circ}}=3.4 \times 10^{-5} \mathrm{~m}
\end{array}
\)
Two waves of same frequency and same amplitude from two monochromatic sources are allowed to superpose at a certain point. If in one case, the phase difference is 0 and in other case it is \(\pi / 2\), then the ratio of the intensities in the two cases will be
(b) When phase difference is 0 , intensity is maximum, i.e. \(I_{\text {max }}\).
When \(\quad \phi=\frac{\pi}{2}\) or \(\frac{\phi}{2}=\frac{\pi}{4}\), the intensity will be
\(
I=I_{\max } \cos ^2 \frac{\phi}{2}=\frac{I_{\max }}{2}
\)
\(\therefore\) The desired ratio is \(2: 1\).
What is the minimum thickness of a soap film needed for constructive interference in reflected light, if the light incident on the film is 750 nm? Assume that the index for the film is \(n=1.33\).
(c) For constructive interference in case of soap film,
\(
2 \mu t=\left(n-\frac{1}{2}\right) \lambda
\)
For minimum thickness \(t, n=1\)
\(
\begin{aligned}
\Rightarrow & 2 \mu t =\frac{\lambda}{2} \\
\therefore & t =\frac{\lambda}{4 \mu}=\frac{750}{4 \times 1.33}=141 \mathrm{~nm}
\end{aligned}
\)
Monochromatic light from a narrow slit illuminates two parallel narrow slits producing an interference pattern on a screen. The separation between the two slits is now doubled and the distance between the screen and the slits is reduced to half. The fringe width
\(
\begin{aligned}
&\text { (c) Fringe width, } \beta=\frac{\lambda D}{d} \Rightarrow \beta \propto \frac{D}{d}\\
&\frac{\beta_2}{\beta_1}=\frac{D_2}{d_2} \times \frac{d_1}{D_1}=\frac{\frac{1}{2} D_1}{2 d_1} \times \frac{d_1}{D_1}=\frac{1}{4} \Rightarrow \beta_2=\frac{\beta_1}{4}
\end{aligned}
\)
Two slits separated by a distance of 1 mm, are illuminated with red light of wavelength \(6.5 \times 10^{-7} \mathrm{~m}\). The interference fringes are observed on a screen placed 1 m from the slits. The distance between the third dark fringe and the fifth bright fringe is equal to
(b)
\(
\begin{aligned}
\Delta y=\frac{5 \lambda D}{d} & -\frac{5 \lambda D}{2 d}=\frac{5 \lambda D}{2 d} \\
& =\frac{5 \times 6.5 \times 10^{-7} \times 1}{2 \times 10^{-3}} \mathrm{~m}=1.63 \mathrm{~mm}
\end{aligned}
\)
In Young’s double slit experiment, 12 fringes are observed to be formed in a certain segment of the screen, when light of wavelength 600 nm is used. If the wavelength of light is changed to 400 nm, number of fringes observed in the same segment of the screen is given by
\(
\text { (b) } n_1 \lambda_1=n_2 \lambda_2 \Rightarrow n_2=\frac{n_1 \lambda_1}{\lambda_2}=12 \times \frac{600}{400}=18
\)
A parallel beam of monochromatic light of wavelength \(5000 Å\) is incident normally on a single narrow slit of width 0.001 mm. The light is focused by a convex lens on a screen placed on the focal plane. The first minima will be formed for the angle of diffraction equal to
\(
\begin{aligned}
&\text { (c) In single narrow slit, for first minima, }\\
&\begin{aligned}
& d \sin \theta =\lambda \\
\Rightarrow & \sin \theta =\frac{\lambda}{d} \\
\therefore & \theta =\sin ^{-1}\left(\frac{5000 \times 10^{-10}}{0.001 \times 10^{-3}}\right)=30^{\circ}
\end{aligned}
\end{aligned}
\)
In Young’s double slit experiment, the 10 th maxima of wavelength \(\lambda_1\) is at a distance of \(y_1\) from the central maximum. When the wavelength of the source is changed to \(\lambda_2\), 5th maxima is at a distance of \(y_2\) from its central maximum. The ratio \(\left(\frac{y_1}{y_2}\right)\) is
\(
\begin{aligned}
&\text { (a) We have, } y_1=\frac{10 \lambda_1 D}{d}, y_2=\frac{5 \lambda_2 D}{d}\\
&\therefore \quad \frac{y_1}{y_2}=\frac{2 \lambda_1}{\lambda_2}
\end{aligned}
\)
It is found that when waves of same intensity from two coherent sources superpose at a certain point, then the resultant intensity is equal to the intensity of one wave only. This means that the phase difference between the two waves at that point is
\(
\begin{array}{ll}
\text { (c) Intensity, } I=4 I_0 \cos ^2 \frac{\phi}{2} \\
\because I=I_0 \Rightarrow \cos ^2 \frac{\phi}{2}=\frac{1}{4} \\
\therefore \phi=\frac{2 \pi}{3}
\end{array}
\)
Young’s double slit experiment is performed in a liquid. The 10th bright fringe in liquid lies on screen where 6th dark fringe lies in vacuum. The refractive index of the liquid is approximately
\(
\begin{aligned}
&\text { (a) We have, } \frac{2(6)-1}{2} \beta=10 \beta^{\prime}\\
&\therefore \quad \frac{\beta}{\beta^{\prime}}=\frac{10}{5.5}=1.8=\mu
\end{aligned}
\)
In a Young’s double slit experiment using red and blue lights of wavelengths 600 nm and 480 nm respectively, the value of \(n\) for which the \(n\)th red fringe coincides with \((n+1)\) th blue fringe is
(b) Let \(n\)th red fringe coincides with \(m\) th blue fringe, then
\(
\begin{aligned}
& \frac{n \lambda_R D}{d} & =\frac{m \lambda_B D}{d} \\
\therefore & \frac{n}{m} & =\frac{\lambda_B}{\lambda_R}=\frac{480}{600}=\frac{4}{5}
\end{aligned}
\)
i.e. 4th red fringe coincides with 5th blue fringe. Next 8th red fringe will coincide with 10th blue fringe and so on. Thus, \(n=4\)
and \(m=n+1=5\)
In Young’s double slit experiment, how many maximas can be obtained on a screen (including the central maximum) on both sides of the central fringes, if \(\lambda=2000 Å\) and \(d=7000 Å\)?
(b) For maximum (brightness) intensity on the screen, path difference should be integer multiple of wavelength, i.e.
\(
\begin{gathered}
d \sin \theta=n \lambda \\
\sin \theta=\frac{n \lambda}{d}=\frac{n(2000)}{7000}=\frac{n}{3.5}
\end{gathered}
\)
As, \(\quad(\sin \theta)_{\max }=1 \Rightarrow n=3.5\)
So, number of maximas \(=0, \pm 1, \pm 2, \pm 3\)
Thus, only seven maximas can be obtained on both sides of the screen.
A beam of light parallel to central line \(A B\) is incident on the plane of slits. The number of minima obtained on the large screen is \(n_1\). Now, if the beam is tilted by some angle ( \(\neq 90^{\circ}\) ) as shown in the figure, then the number of minima obtained is \(n_2\). Then,
(a) When a light beam is tilted, the number of minima observed on the screen remains the same. Therefore, \(\mathrm{n} 1=\mathrm{n} 2\). The fringe pattern shifts, but the total number of fringes (and thus minima) stays constant.
Explanation:
In a double-slit experiment, the number of minima is determined by the wavelength of light and the separation of the slits, not the angle of incidence of the light beam as long as the beam remains parallel to the screen. Tilting the beam simply shifts the entire interference pattern, but the pattern’s width and the number of minima remain unchanged.
Therefore, the relationship between \(n_1\) and \(n_2\) is: \(n_1=n_2\)
A monochromatic beam of light falls on YDSE apparatus at some angle (say \(\theta\) ) as shown in the figure. A thin sheet of glass is inserted in front of the lower slit \(S_2\). The central bright fringe (path difference \(=0\) ) will be obtained
(d) If \(d \sin \theta=(\mu-1) t\), central fringe is obtained at \(O\).
If \(d \sin \theta>(\mu-1) t\), central fringe is obtained above \(O\).
If \(d \sin \theta<(\mu-1) t\), central fringe is obtained below \(O\).
Unpolarised light of intensity \(32 \mathrm{Wm}^{-2}\) passes through three polarisers such that the transmission axis of the last polariser is crossed with the first. If the intensity of the emerging light is \(3 \mathrm{Wm}^{-2}\). What is the angle between the transmission axes of the first two polarisers?
\(
\text { (a) } I_2=I_1 \cos ^2\left(90^{\circ}-\theta\right)=\frac{I^{\prime}}{2} \cos ^2 \theta \sin ^2 \theta=\frac{I^{\prime}}{8}(\sin 2 \theta)^2
\)
\(
\begin{aligned}
3 & =\frac{32}{8}(\sin 2 \theta)^2 \\
\sin 2 \theta=\frac{\sqrt{3}}{2} & =\sin 60^{\circ} \text { or } \sin 120^{\circ} \\
\theta & =30^{\circ} \text { or } 60^{\circ}
\end{aligned}
\)
In a Young’s double slit experiment, one of the slits is covered with a transparent sheet of thickness \(3.6 \times 10^{-3} \mathrm{~cm}\) due to which position of central fringe shifts to a position originally occupied by 30th bright fringe. The refractive index of the sheet, if \(\lambda=6000 Å\) is
(a) Number of fringes shifted, \(N=\frac{(\mu-1) t}{\lambda}\)
\(\therefore\) Refractive index of the sheet,
\(
\mu=\frac{N \lambda}{t}+1=\frac{30 \times 6000 \times 10^{-10}}{3.6 \times 10^{-5}}+1=1.5
\)
In Young’s double slit experiment, the \(y\)-coordinates of central maximum and 10th maxima are 2 cm and 5 cm, respectively. When the YDSE apparatus is immersed in a liquid of refractive index 1.5. The corresponding \(y\)-coordinates will be
(c) Fringe width, \(\beta=\frac{D \lambda}{d}\)
i.e. \(\beta \propto \lambda\)
So, wavelength \(\lambda\) and hence fringe width \(\beta[latex] decreases 1.5 or [latex]\frac{3}{2}\) times when immersed in liquid. The distance between central maximum and 10th maxima is 3 cm in vacuum. When immersed in liquid it will reduce to 2 cm. Position of central maximum will not change while 10 th maxima will be obtained at \(y=4 \mathrm{~cm}\).
In Young’s double slit experiment, wavelength \(\lambda=5000 Å\), the distance between the slits is 0.2 mm and the screen is at 200 cm from the slits. The central maximum is at \(x=0\). The third maxima (taking the central maximum as zeroth maxima) will be at \(x\) equal to
\(
\begin{aligned}
&\text { (b) Position of third maxima, }\\
&x_3=\frac{3 \lambda D}{d}=\frac{3\left(5 \times 10^{-5}\right)(200)}{0.02}=1.5 \mathrm{~cm}
\end{aligned}
\)
A parallel beam of light of intensity \(I\) is incident on a glass plate. 25% of light is reflected in any reflection by upper surface and \(50 \%\) of light is reflected by any reflection from lower surface. Rest is refracted. The ratio of maximum to minimum intensity in interference region of reflected rays is
\(
\begin{aligned}
& \text { (d) } I_1=\frac{I}{4} \text { and } I_2=\frac{9 I}{32} \\
& \therefore \quad \frac{I_1}{I_2}=\frac{8}{9} \\
& \text { or } \sqrt{\frac{I_1}{I_2}}=\frac{2 \sqrt{2}}{3}
\end{aligned}
\)
\(
\frac{I_{\max }}{I_{\min }}=\left(\frac{\sqrt{I_1 / I_2}+1}{\sqrt{I_1 / I_2}-1}\right)^2=\left(\frac{2 \sqrt{2}+3}{2 \sqrt{2}-3}\right)^2
\)
In the Young’s double slit experiment, the intensities at two points \(P_1\) and \(P_2\) on the screen are respectively \(I_1\) and \(I_2\). If \(P_1\) is located at the centre of a bright fringe and \(P_2\) is located at a distance equal to a quarter of fringe width from \(P_1\), then \(\frac{I_1}{I_2}\) is
\(
\begin{aligned}
&\text { (a) According to the question, }\\
&y=\frac{\omega}{4}=\frac{\lambda D}{4 d} \Rightarrow \Delta x=\frac{y d}{D}=\frac{\lambda}{4}
\end{aligned}
\)
Phase difference, \(\phi=\frac{2 \pi}{\lambda} \cdot \Delta x=\frac{\pi}{2}\)
\(
\therefore \quad \frac{\phi}{2}=\frac{\pi}{4}
\)
Now, intensity, \(I_2=I_1 \cos ^2 \frac{\phi}{2}\)
\(
\frac{I_1}{I_2}=\frac{1}{\cos ^2 \phi / 2}=2
\)
In Young’s double slit experiment, the two slits acts as coherent sources of equal amplitude \(A\) and wavelength \(\lambda\). In another experiment with the same set up the two slits are sources of equal amplitude \(A\) and wavelength \(\lambda\) but are incoherent. The ratio of the intensity of light at the mid-point of the screen in the first case to that in the second case is
(c) Intensity in the first case, \(I_1=\left(\sqrt{I_0}+\sqrt{I_0}\right)^2=4 I_0\) where, \(I_0=\) intensity due to each source.
Intensity in second case, \(I_2=I_0+I_0=2 I_0\)
\(
\frac{I_1}{I_2}=\frac{4 I_0}{2 I_0}=\frac{2}{1}
\)
In the ideal double slit experiment, when a glass-plate (refractive index 1.5) of thickness \(t\) is introduced in the path of one of the interfering beams (wavelength \(\lambda\) ), the intensity at the position where the central maximum occurred previously remains unchanged. The minimum thickness of the glass-plate is
\(
\begin{aligned}
& \text { (a) Shift }=\frac{(\mu-1) t D}{d}=\omega=\frac{\lambda D}{d} \\
& \therefore \quad t=2 \lambda \text { (as } \mu=1.5)
\end{aligned}
\)
In the standard Young’s double slit experiment, the intensity on the screen at a point distant 1.25 fringe widths from the central maximum is (assuming slits to be identical)
\(
\begin{aligned}
&\text { (a) Path difference, }\\
&\begin{aligned}
\Delta x=\frac{y d}{D} & =\left(\frac{1.25 \lambda D}{d}\right)\left(\frac{d}{D}\right) \\
& =1.25 \lambda=\frac{5}{4} \lambda
\end{aligned}
\end{aligned}
\)
\(
\begin{array}{ll}
\text { Phase difference, } \phi & =\frac{2 \pi}{\lambda} \cdot \Delta x \\
& =\frac{2 \pi}{\lambda} \times \frac{5}{4} \lambda=\frac{5}{2} \pi \\
\therefore \quad & \frac{\phi}{2}=\frac{5}{4} \pi=225^{\circ} \\
\therefore \quad & \text { Intensity, } I=I_{\max } \cos ^2 \frac{\phi}{2}=\frac{1}{2} I_{\max }
\end{array}
\)
In a Young’s double slit experiment, \(D\) equals the distance of screen and \(d\) is the separation between the slits. The distance of the nearest point to the central maximum where the intensity is same as that due to a single slit, is equal to
\(
\text { (c) Intensity, } I=4 I_0 \cos ^2 \frac{\phi}{2}
\)
\(
\begin{aligned}
& I=I_0 \\
& \phi=\frac{2 \pi}{3}=\frac{2 \pi}{\lambda} \cdot \Delta x=\frac{2 \pi}{\lambda}\left(\frac{y d}{D}\right) \\
& y=\frac{\lambda D}{3 d}
\end{aligned}
\)
The intensity of each of the two slits in Young’s double slit experiment is \(I_0\). Calculate the minimum separation between the two points on the screen where intensities are \(2 I_0\) and \(I_0\). (Given, fringe width \(=\alpha\) )
\(
\text { (c) } 2 I_0=4 I_0 \cos ^2 \frac{\phi}{2}
\)
\(
\begin{aligned}
& \phi=\frac{\pi}{2}=\frac{2 \pi}{\lambda} \cdot \Delta x=\frac{2 \pi}{\lambda} \cdot\left(\frac{y d}{D}\right) \\
& y_1=\frac{\lambda D}{4 d}
\end{aligned}
\)
Further, \(I_0=4 I_0 \cos ^2 \frac{\phi}{2}\)
\(
\begin{array}{ll}
\Rightarrow & \phi=\frac{2 \pi}{3}=\frac{2 \pi}{\lambda} \Delta x=\frac{2 \pi}{\lambda}\left(\frac{y_2 d}{D}\right) \\
\therefore & y_2=\frac{\lambda D}{3 d}
\end{array}
\)
Minimum separation, \(\Delta y=y_2-y_1=\frac{1}{12}\left(\frac{\lambda D}{d}\right)=\frac{\alpha}{12}\)
One slit of a double slit experiment is covered by a thin glass plate of refractive index 1.4, and the other by a thin glass plate of the refractive index 1.7. The point on the screen where the central maximum fall before the glass plate was inserted, is now occupied by what had been the fifth bright fringe was seen before. Assume the plate have the same thickness \(t\) and wavelength of light 480 nm . Then, the value of \(t\) is
\(
\begin{aligned}
&\text { (c) Five fringes have to be shifted. }\\
&\begin{aligned}
& \therefore \quad 5=\frac{\left(\mu_1-1\right) t-\left(\mu_2-1\right) t}{\lambda}=\frac{\left(\mu_1-\mu_2\right) t}{\lambda} \\
& \begin{aligned}
\therefore \text { Thickness, } t=\frac{5 \lambda}{\left(\mu_1-\mu_2\right)} & =\frac{5 \times 480 \times 10^{-9}}{1.7-1.4} \\
& =8 \times 10^{-6} \mathrm{~m} \text { or } 8 \mu \mathrm{~m}
\end{aligned}
\end{aligned}
\end{aligned}
\)
An interference is observed due to two coherent sources separated by a distance \(5 \lambda\) along \(Y\)-axis, where \(\lambda\) is the wavelength of light. A detector \(D\) is moved along the positive \(X\)-axis. The number of point on the \(X\)-axis excluding the points \(x=0\) and \(x=\infty\) at which resultant intensity will be maximum, are
(a) At \(x=0, \Delta x=5 \lambda\)
which corresponds to a maximum.
At \(x=\infty, \Delta x=0\), this also corresponds to a maximum.
\(\therefore\) Other possible maxima between \(x=0\) and \(x=\infty\) are \(\Delta x=\lambda, 2 \lambda, 3 \lambda, 4 \lambda\).
In a Young’s double slit experiment, using unequal slit widths, the intensity at a point midway between a bright and dark fringes is \(4 I\). If one slit is covered by an opaque film, intensity at that point becomes \(2 I\). If the other is covered instead, then the intensity at that point is
(a) Location of the point, \(y=\frac{\omega}{4}=\frac{\lambda D}{4 d}\)
\(
\begin{aligned}
\Delta x & =\frac{y d}{D}=\frac{\lambda}{4} \\
\phi & =\frac{2 \pi}{\lambda} \cdot \Delta x=\frac{\pi}{2} \\
I_R & =I_1+I_2+2 \sqrt{I_1 I_2} \cos \phi \\
4 I & =2 I+I_2+0 \\
I_2 & =2 I
\end{aligned}
\)
Two coherent light sources \(A\) and \(B\) are at a distance \(3 \lambda\) from each other \((\lambda=\) wavelength \()\). The distance from \(A\) on the \(X\)-axis at which the interference is constructive, is
(c) Say \(P\) be the point on \(X\)-axis, where constructive interference is obtained.
\(
\begin{aligned}
B P-A P & =2 \lambda \text { or } \lambda \\
\sqrt{9 \lambda^2+x^2}-x & =2 \lambda \\
9 \lambda^2+x^2 & =x^2+4 \lambda^2+4 x \lambda \\
x & =\frac{5 \lambda}{4}
\end{aligned}
\)
Further, \(\sqrt{9 \lambda^2+x^2}-x=\lambda\)
\(
\begin{aligned}
& \therefore 9 \lambda^2+x^2 & =x^2+\lambda^2+2 x \lambda \\
& \therefore x & =4 \lambda
\end{aligned}
\)
Hence, the distance from \(A\) on the \(X\)-axis at which the interference is constructive is \(5 \lambda / 4\).
Two coherent sources separated by distance \(d\) are radiating in phase having wavelength \(\lambda\). A detector moves in a big circle around the two sources in the plane of the two sources. The angular position of \(n=4\) interference maxima is given as
(b) Path difference at a point \(Q\) on the circle is
\(
\Delta y=d \cos \theta \dots(i)
\)
For maxima at \(Q\), path difference should be integer multiple of wavelength
\(
\Delta y=n \lambda \dots(ii)
\)
\(
\begin{aligned}
&\text { From Eqs. (i) and (ii), we get }\\
&\begin{array}{ll}
& n \lambda=d \cos \theta \\
\therefore & \theta=\cos ^{-1}\left(\frac{n \lambda}{d}\right) \\
\text { For } & n=4 \\
\text { Angular position, } & \theta=\cos ^{-1}\left(\frac{4 \lambda}{d}\right)
\end{array}
\end{aligned}
\)
Two ideal slits \(S_1\) and \(S_2\) are at a distance \(d\) apart and illuminated by light of wavelength \(\lambda\) passing through an ideal source slit \(S\) placed on the line through \(S_2\) as shown below. The distance between the plane of slits and the source slit is \(D\).
A screen is held at a distance \(D\) from the plane of the slits. The minimum value of \(d\) for which there is darkness at \(O\) is
(c) Path difference between the waves reaching at \(O\),
\(
\Delta=\Delta_1+\Delta_2
\)
where, \(\Delta_1=\) initial path difference and \(\Delta_2=\) path difference between the waves after emerging from slits.
\(
\text { Now, } \quad \Delta_1=S S_1-S S_2=\sqrt{\left(D^2+d^2\right)}-D
\)
and \(\quad \Delta_2=S_1 O-S_2 O=\sqrt{\left(D^2+d^2\right)}-D\)
\(
\begin{aligned}
\Delta & =2\left|\sqrt{\left(D^2+d^2\right)}-D\right|=2\left\{\left(D^2+d^2\right)^{1 / 2}-D\right\} \\
& =2\left\{\left(D+\frac{d^2}{2 D}\right)-D\right\} \text { (from binomial expansion) } \\
& =\frac{d^2}{D}
\end{aligned}
\)
For obtaining dark at \(O, \Delta\) must be equals to \((2 n-1) \frac{\lambda}{2}\).
\(
\begin{array}{ll}
\text { i.e. } & \frac{d^2}{D}=(2 n-1) \frac{\lambda}{2} \\
\therefore & d^2=\frac{(2 n-1) \lambda D}{2} \text { or } d=\sqrt{\frac{(2 n-1) \lambda D}{2}}
\end{array}
\)
For minimum distance ( \(n=1\) ),
So,\(d=\sqrt{\frac{\lambda D}{2}}\)
In the diagram below, \(C P\) represents a wavefront and \(A O\) and \(B P\), the corresponding incident rays. Find the condition of \(\theta\) for constructive interference at point \(P\) between the rays \(B P\) and reflected ray \(O P\)
(b) Path difference between the two rays is given by
\(
\begin{aligned}
\Delta & =C O+P O \\
P R & =d \\
P O & =d \sec \theta \\
C O & =P O \cos 2 \theta=d \sec \theta \cos 2 \theta \\
\Delta & =(d \sec \theta+d \sec \theta \cos 2 \theta)
\end{aligned}
\)
Phase difference between two rays is \(\phi=\pi\) (as one ray is reflected one and another is direct).
Now, for constructive interference, path difference should be even multiple of half-wavelength.
i.e. \(\Delta=\lambda / 2,3 \lambda / 2, \ldots\)
\(
\text { So, } d \sec \theta+d \sec \theta \cos 2 \theta=\frac{\lambda}{2}
\)
\(
\begin{aligned}
d \sec \theta(1+\cos 2 \theta) & =\frac{\lambda}{2} \\
d \sec \theta\left(2 \cos ^2 \theta\right) & =\frac{\lambda}{2} \\
\cos \theta & =\lambda / 4 d
\end{aligned}
\)
Distance of 5th dark fringe from centre is 4 mm . If \(D=2 \mathrm{~m}, \lambda=600 \mathrm{~nm}\), then distance between slits is [AIIMS 2019]
(a) Given, distance between source and observer,
\(
D=2 \mathrm{~m}
\)
Distance of 5th dark fringe from centre
\(
=4 \times 10^{-3} \mathrm{~m}
\)
Wavelength, \(\lambda=600 \mathrm{~nm}=6 \times 10^{-7} \mathrm{~m}\)
Distance of 5th dark fringe from centre
\(
=\beta+\beta+\beta+\beta+\frac{\beta}{2}=\frac{9 \beta}{2}
\)
where, \(\beta\) = fringe width.
According to question, \(\frac{9 \beta}{2}=4 \times 10^{-3}\)
\(
\begin{gathered}
\frac{9}{2} \times \frac{D \lambda}{d}=4 \times 10^{-3} \\
\frac{9}{2} \times \frac{2 \times 6 \times 10^{-7}}{d}=4 \times 10^{-3} \\
\Rightarrow \quad \begin{aligned}
d & =1.35 \times 10^{-3} \mathrm{~m} \\
& =1.35 \mathrm{~mm}
\end{aligned}
\end{gathered}
\)
A light of wavelength 500 nm is incident on a Young’s double slit experiment. The distance between slit and screen is \(D=1.8 \mathrm{~m}\) and distance between slits is \(d=0.4 \mathrm{~mm}\). If screen moves with a speed of \(4 \mathrm{~ms}^{-1}\), then with what speed first maxima will move? [AIIMS 2019]
(a) Given, wavelength of light,
\(
\lambda=500 \mathrm{~nm}=5 \times 10^{-7} \mathrm{~m}
\)
Distance between slit and screen,
\(
D=1.8 \mathrm{~m}
\)
Distance between two slits,
\(
d=0.4 \mathrm{~mm}=4 \times 10^{-4} \mathrm{~m}
\)
Velocity of screen \(=\frac{d D}{d t}=4 \mathrm{~ms}^{-1}\)
Speed of first maxima \(=\frac{d \beta}{d t}=\) ?
In Young’s double slit experiment, fringe width,
\(
\beta=\frac{D \lambda}{d}
\)
Differentiating with respect to \(t[latex], we get
[latex]
\begin{aligned}
\frac{d \beta}{d t}=\frac{\lambda}{d} \cdot \frac{d D}{d t} & =\frac{5 \times 10^{-7}}{4 \times 10^{-4}} \times 4 \\
& =5 \times 10^{-3} \mathrm{~ms}^{-1} \\
& =5 \mathrm{mms}^{-1}
\end{aligned}
\)
Assertion: Distance between position of bright and dark fringes remain same in Young’s double slit experiment.
Reason: Fringe width, \(\beta=\frac{\lambda D}{d}\) [AIIMS 2019]
(a) Distance between position of bright and dark fringes is called fringe width in Young’s double slit experiment, which is given by \(\beta=\frac{D \lambda}{d}\).
where, \(\beta=\) fringe width,
\(D=\) distance between source and screen,
\(d=\) distance between two slits
and \(\lambda=\) wavelength of monochromatic light wave.
Therefore, in Young’s double slit experiment, fringes are of equal width, i.e. width of bright and dark fringes are same. Hence, both Assertion and Reason are correct and Reason is the correct explanation of Assertion.
Assertion: Incoming light reflected by earth is partially polarised.
Reason: Atmospheric particle polarise the light. [AIIMS 2019]
(b) When unpolarised light coming from sun, enters the atmosphere of earth, then it scatters due to presence of atmospheric particles. The scattered light seen in a direction perpendicular to the direction of incidence is found to be plane polarised.
When the light from the sun incident on reflecting surface of earth at an angle of polarisation, then reflecting light is polarised. Little amount of light is incident on polarising direction, hence reflected light is partially polarised.
Hence, Assertion and Reason both are correct but Reason is not the correct explanation of Assertion.
Huygens’ principle does not use [JIPMER 2019]
(d) Huygens’ principle use the phenomenon of light as reflection, refraction and diffraction but does not use point of spectra origin.
The Young’s double slit experiment is performed with blue and green light of wavelengths \(4360 Å\) and \(5460 Å\), respectively. If \(x\) is the distance of 4 th maxima from the central one, then [AIIMS 2017]
(c) In Young’s double slit experiment, position of bright fringes on the screen are given by
\(
x=\frac{n D \lambda}{d}
\)
Hence, distance of \(n\)th maxima will be \(x=n \lambda \frac{D}{d} \propto \lambda\)
\(
\lambda_{\text {blue }}=4360 Å, \lambda_{\text {green }}=5480 Å
\)
where, \(x=\) distance of 4th maxima from the central one.
\(
\begin{array}{ll}
\text { As, } & \lambda_{\text {blue }}<\lambda_{\text {green }} \\
\therefore & x_{\text {blue }}<x_{\text {green }}
\end{array}
\)
White light is used to illuminate two slits in Young’s double slit experiment. The separation between the slits is \(b\) and the screen is at a distance \(d(\gg b)\) from the slits. At a point on the screen directly in front of one of the slits, which wavelengths are missing? [JIPMER 2017]
(c) The situation is shown in the figure
The path difference between the waves reaching the point \(P\) is
\(
\begin{aligned}
\Delta p & =B P-A P \\
& =\left(d^2+b^2\right)^{1 / 2}-d \\
& =d\left(1+\frac{b^2}{d^2}\right)^{1 / 2}-d \\
& \approx d\left[1+\frac{1}{2} \cdot \frac{b^2}{d^2}\right]-d=\frac{b^2}{2 d}
\end{aligned}
\)
For a dark band, \(\Delta p=\frac{b^2}{2 d}=(2 n-1) \frac{\lambda}{2}\) where, \(n=1,2,3\) or \(\lambda=\frac{1}{(2 n-1)} \cdot \frac{b^2}{d}\)
Hence, the missing wavelengths are \(\frac{b^2}{d}, \frac{b^2}{3 d}, \frac{b^2}{5 d}, \ldots\).
The maximum numbers of possible interference maxima for slit separation equal to twice the wavelength in Young’s double slit experiment, is [JIPMER 2017]
(b) The condition of interference maxima is \(d \sin \theta=n \lambda, \quad \sin \theta=\frac{n \lambda}{d}\)
Given, \(d=2 \lambda\) and \(\sin \theta=\frac{n \lambda}{2 \lambda}=\frac{n}{2}\)
The magnitude of \(\sin \theta\) lies between 0 and 1.
When \(n=0, \sin \theta=0 \Rightarrow \theta=0^{\circ}\)
When \(n=1, \sin \theta=1 / 2 \Rightarrow \theta=30^{\circ}\)
When \(n=2, \sin \theta=1 \Rightarrow \theta=90^{\circ}\)
Thus, there is central maximum at \(\theta=0^{\circ}\), on either side of it maxima lie at \(\theta=30^{\circ}\) and \(\theta=90^{\circ}\), so maximum number of possible interference maxima is five.
Light of wavelength \(\lambda\) is incident on slit of width \(d\). The resulting diffraction pattern is observed on a screen placed at distance \(D\). The linear width of central maximum is equal to width of the slit, then \(D=\ldots\) [Guj. CET 2015]
(b) In diffraction, fringe width, \(\beta=\frac{\lambda D}{d}\)
When \(\frac{d}{2}=\beta\), then \(\frac{d}{2}=\frac{\lambda D}{d} \Rightarrow D=\frac{d^2}{2 \lambda}\)
A beam of light contains two wavelengths \(6500 Å\) and \(5200 Å\). They form interference fringes in Young’s double slit experiment. What is the least distance (approx) from central maximum, where the bright fringes due to both wavelength coincide? The distance between the slits is 2 mm and distance between the screen and slit is 120 cm. [CG PMT 2015]
(a) To find the point of coincidence of bright fringes, we can equate the distance of bright fringes from the central maximum, made by both the wavelengths of light.
Given, distance between the screen and slit,
\(
D=120 \mathrm{~cm}=120 \times 10^{-2} \mathrm{~m}
\)
Slit width,
\(
\begin{aligned}
d & =2 \mathrm{~mm}=2 \times 10^{-3} \mathrm{~m} \\
\lambda_1 & =6500 Å \text { and } \lambda_2=5200 Å
\end{aligned}
\)
Let \(n\)th fringe due to \(\lambda_2=5200 Å\) coincide with \((n-1)\) th bright fringe due to \(\lambda_1=6500 Å\).
\(
\begin{array}{rlrl}
& \therefore & \frac{D n \lambda_2}{d} & =\frac{D(n-1) \lambda_1}{d} \\
\text { or } & n \times 5200 & =(n-1) 6500 \\
\text { or } & 4 n & =5 n-5
\end{array}
\)
\(
\begin{aligned}
&\Rightarrow \quad n=5\\
&\text { So, the least distance required, } y_n=\frac{n \lambda_2 D}{d}\\
&\begin{aligned}
& =\frac{5 \times 5200 \times 10^{-10} \times 120 \times 10^{-2}}{2 \times 10^{-3}} \\
& =0.16 \times 10^{-2} \mathrm{~m}=0.16 \mathrm{~cm}
\end{aligned}
\end{aligned}
\)
Find the right condition for Fraunhofer diffraction due to a single slit. [WB JEE 2015]
(c) The correct condition for Fraunhofer diffraction due to a single slit is: Source is at infinity and the incident beam is parallel.
Explanation: Fraunhofer diffraction requires a plane wavefront incident on the slit, which is achieved when the light source is infinitely far away and the beam is parallel.
The parallel beams of monochromatic light of wavelength \(4.5 \times 10^{-7} \mathrm{~m}\) passes through a long slit with width \(0.2 \times 10^{-3} \mathrm{~m}\). The angular divergence in which most of the light is [UP CPMT 2015]
(a) Most of the light is diffracted between the two first order minima.
These minima occur at angles given by \(b \sin \theta= \pm \lambda\).
\(\Rightarrow \quad \sin \theta= \pm \frac{\lambda}{b}= \pm \frac{4.5 \times 10^{-7}}{0.2 \times 10^{-3}}= \pm 2.25 \times 10^{-3}\)
\(\Rightarrow \quad \theta \simeq 2.25 \times 10^{-3} \mathrm{rad} \quad\) (angle is very small)
The angular divergence, \(2 \theta=4.5 \times 10^{-3} \mathrm{rad}\)
The condition for obtaining secondary maxima in the diffraction pattern due to single slit is [Manipal 2015]
(b) The correct condition for obtaining secondary maxima in the diffraction pattern due to a single slit is given by option (b) \(a \sin \theta=(2 n-1) \lambda / 2\).
Explanation:
In single-slit diffraction, secondary maxima are observed as less intense bright fringes located between the dark fringes (minima). The condition for these secondary maxima to occur is that the path difference between wavelets from different parts of the slit is an odd multiple of half the wavelength.
For secondary maxima, we need to consider the odd multiples of the wavelength. The correct condition for secondary maxima can be derived from the equation for minima, which occurs at:
\(
a \sin \theta=\left(n+\frac{1}{2}\right) \lambda
\)
where \(n\) is a positive integer \((1,2,3, \ldots)\)
In Young’s double slit experiment, when wavelength used is \(6000 Å\) and the screen is 40 cm from the slits, the fringes are 0.012 cm wide. What is the distance between the slits? [Manipal 2015]
\(
\begin{aligned}
&\text { (b) Fringe width, } \beta=\frac{D \lambda}{d}\\
&\Rightarrow \quad d=\frac{D \lambda}{\beta}=\frac{6000 \times 10^{-10} \times 40 \times 10^{-2}}{0.012 \times 10^{-2}}=0.2 \mathrm{~cm}
\end{aligned}
\)
The polarising angle of glass is \(57^{\circ}\). A ray of light which is incident at this angle will have an angle of refraction as [KCET 2015]
(d) Given, \(\theta_P=57^{\circ}\)
According to Brewster’s law, we have
\(
\theta_P+\theta_r=90^{\circ} \Rightarrow \theta_r=90^{\circ}-\theta_P=90^{\circ}-57^{\circ}
\)
Angle of refraction, \(\theta_r=33^{\circ}\)
To observe diffraction, the size of the obstacle [KCET 2015]
(c) To observe diffraction, the size of the obstacle should be of the order of wavelength, i.e. \(\lambda \approx d\).
A plane wave of wavelength \(6250 Å\) is incident normally on a slit of width \(2 \times 10^{-2} \mathrm{~cm}\). The width of the principal maximum of diffraction pattern on a screen at a distance of 50 cm will be [EAMCET 2015]
(a) According to the question,
\(
\lambda=6250 \AA=6250 \times 10^{-10} \times 10^2 \mathrm{~cm}=6250 \times 10^{-8} \mathrm{~cm}
\)
Width of the slit, \(a=2 \times 10^{-2} \mathrm{~cm}\)
The angular width of central maximum, \(\beta=2 \theta=2 \frac{\lambda}{a}\)
Thus, linear width is
\(
\begin{aligned}
L & =\beta \times D=\frac{2 \lambda}{a} \times D=\frac{2 \times 6250 \times 10^{-8}}{2 \times 10^{-2}} \times 50 \\
& =6250 \times 10^{-6} \times 50=3125 \times 10^{-4} \\
& =312.5 \times 10^{-3} \mathrm{~cm}
\end{aligned}
\)
A beam of light of wavelength 590 nm is focussed by a converging lens of diameter 10 cm at a distance of 20 cm from it. Find the diameter of the disc image formed [UK PMT 2015]
(a) Given, wavelength, \(\lambda=590 \mathrm{~nm}=590 \times 10^{-9} \mathrm{~m}\)
Diameter of lens \(=10 \times 10^{-2} \mathrm{~m}\)
Radius of lens \(=5 \times 10^{-2} \mathrm{~m}\)
Focal length of lens \(=20 \times 10^{-2} \mathrm{~m}\)
Now, the diameter of image disc
\(
\begin{aligned}
D=2 R=2\left(1.22 \frac{\lambda D}{b}\right) & =\left(\frac{1.22 \times 590 \times 10^{-9} \times 20 \times 10^{-2}}{5 \times 10^{-2}}\right) \times 2 \\
& \simeq 5.76 \times 10^{-4} \mathrm{~cm}
\end{aligned}
\)
A plane polarised light is incident normally on a tourmaline plate. Its \(\mathbf{E}\) vector make an angle of \(60^{\circ}\) with the optic axis of the plate. Find the percentage difference between initial and final intensities. [Guj.CET 2015]
(c) According to law of Malus, when a beam of completely plane polarised light is incident on an analyser, the resultant intensity of light \(I\) transmitted from an analyser varies directly as the square of cosine angle between plane of analyser and polariser.
Let initial intensity is \(I\) and final intensity is \(I^{\prime}\), then
\(
I^{\prime}=I \cos ^2 60^{\circ}=I\left(\frac{1}{2}\right)^2=\frac{I}{4}
\)
Now, % difference between initial and final intensities,
\(
\begin{aligned}
& =\frac{I-(I / 4)}{I} \times 100=\frac{3 I}{4} \times \frac{1}{I} \times 100 \\
& =\frac{3}{4} \times 100=75 \%
\end{aligned}
\)
In Young’s double slit experiment, the locus of the point \(P\) lying in a plane with a constant path difference between two interfering waves is [Kerala CEE 2015]
(a) A hyperbola.
Explanation:
In Young’s double-slit experiment, a point \(P\) on the screen will experience constructive interference (bright fringe) when the path difference between the light waves traveling from the two slits to \(P\) is a multiple of the wavelength. This condition can be mathematically represented as:
\(
d \sin (\theta)=n \lambda
\)
where \(d\) is the distance between the slits, \(\theta\) is the angle between the line connecting \(P\) to the center of the slits and the normal to the slits, \(n\) is an integer representing the order of the fringe ( 0 for the central maximum, 1 for the first bright fringe, etc.), and \(\lambda\) is the wavelength of the light.
If we rearrange this equation to solve for \(d \sin (\theta)\) :
\(
d \sin (\theta)=n \lambda
\)
The equation of a hyperbola in standard form is:
\(
\frac{x^2}{a^2}-\frac{y^2}{b^2}=1
\)
If we make the substitutions \(x=d \sin (\theta)\) and \(y=n \lambda\), we can see that the equation for a hyperbola describes the locus of points \(P\) with a constant path difference.
Wavefront is the locus of all points, where the particles of the medium vibrate with the same [KCET 2014]
(a) Phase.
Explanation: A wavefront is defined as the locus of all points in a medium that are vibrating in the same phase. This means that all particles on a wavefront are at the same point in their oscillation cycle (e.g., all at crests or all at troughs).
In the Young’s double slit experiment, the intensity of light at a point on the screen (where the path difference is \(\lambda\) ) is \(K\), ( \(\lambda\) being the wavelength of light used). The intensity at a point where the path difference is \(\lambda / 4\), will be [J & K CET 2014]
\(
\text { (c) For net intensity, } I^{\prime}=4 I_0 \cos ^2 \frac{\phi}{2}
\)
\(
\text { Case I: } K=4 I_0 \cos ^2\left(\frac{2 \pi}{2}\right) \quad\left(\because \phi=\frac{2 \pi}{\lambda} \times \lambda\right)
\)
\(
K=4 I_0 \cos ^2(\pi) \Rightarrow K=4 I_0 \dots(i)
\)
\(
\text { Case II: } \quad K^{\prime}=4 I_0 \cos ^2\left(\frac{\pi / 2}{2}\right) \quad\left(\because \phi=\frac{2 \pi}{\lambda} \times \frac{\lambda}{4}\right)
\)
\(
K^{\prime}=4 I_0 \cos ^2(\pi / 4) \Rightarrow K^{\prime}=2 I_0 \dots(ii)
\)
\(
\begin{aligned}
&\text { Comparing Eqs. (i) and (ii), we get }\\
&K^{\prime}=K / 2
\end{aligned}
\)
Two coherent monochromatic beams of intensities \(I\) and \(4 I\) respectively, are superposed. Then, the maximum and minimum intensities in the resulting pattern are [WB JEE 2014]
(d) We know that,
The maximum intensity, \(I_{\max }=\left(\sqrt{I_1}+\sqrt{I_2}\right)^2 \dots(i)\)
The minimum intensity, \(I_{\min }=\left(\sqrt{I_1}-\sqrt{I_2}\right)^2 \dots(ii)\)
So, the ratio of the maximum and minimum intensities is
\(
\begin{aligned}
& \frac{I_{\max }}{I_{\min }}=\frac{\left(\sqrt{I_1}+\sqrt{I_2}\right)^2}{\left(\sqrt{I_1}-\sqrt{I_2}\right)^2}=\frac{(\sqrt{4 I}+\sqrt{I})^2}{(\sqrt{4 I}-\sqrt{I})^2} \\
\Rightarrow \quad & \frac{I_{\max }}{I_{\min }}=\left(\frac{3 \sqrt{I}}{\sqrt{I}}\right)^2=\frac{9}{1}=9: 1
\end{aligned}
\)
Hence, the maximum and minimum intensities in the resulting pattern are \(9 I\) and \(I\).
Colours appear on a thin soap film and soap bubbles due to the phenomenon of [UK PMT 2014]
(a) The diagram below shows a thin soap film and soap bubbles.
The rays 1 and 2 produce the phenomenon of interference when they meet. The path difference between the rays are proportional to thickness of film, i.e. path difference \((\Delta x) \propto t\). As, thickness \(t\) varies, so \(\Delta x\) varies. Maximas and minimas appear for different wavelengths in incident white light. When white light is used, the path difference (phase difference) will satisfy the condition of maxima for certain wavelengths and condition of minima for other wavelengths. This gives coloured appearance of the film.
In Young’s double slit experiment, the ratio of maximum and minimum intensities in the fringe system is \(9: 1\). The ratio of amplitudes of coherent sources is [UK PMT 2014]
(c) \(\frac{I_{\max }}{I_{\min }}=\left(\frac{a_{\max }}{a_{\min }}\right)^2=\left(\frac{a_1+a_2}{a_1-a_2}\right)^2\)
According to given question, \(\frac{I_{\max }}{I_{\min }}=\frac{9}{1}\)
\(
\begin{aligned}
9 & =\left(\frac{a_1 / a_2+1}{a_1 / a_2-1}\right)^2 \Rightarrow(3)^2=\left(\frac{a_1 / a_2+1}{a_1 / a_2-1}\right)^2 \\
3 & =\frac{a_1 / a_2+1}{a_1 / a_2-1} \Rightarrow 3\left(\frac{a_1}{a_2}\right)-3=\frac{a_1}{a_2}+1 \\
2\left(\frac{a_1}{a_2}\right) & =4 \Rightarrow \frac{a_1}{a_2}=\frac{4}{2}=\frac{2}{1} \Rightarrow a_1: a_2=2: 1
\end{aligned}
\)
In Young’s double slit interference experiment, using two coherent waves of different amplitudes, the intensities ratio between bright and dark fringes is 3. Then, the value of the wave amplitudes ratio that arrive there is [EAMCET 2014]
(c) According to given question,
\(
I_1: I_2=3: 1, a_1: a_2=?
\)
The intensity of light due to an illuminated slit is directly proportional to the width of the slit, if \(w_1\) and \(w_2\) be the width of two silts and \(I_1\) and \(I_2\) are the intensities of light on the screen due to the respective slits, then
\(
\frac{w_1}{w_2}=\frac{I_1}{I_2}=\left(\frac{a_1}{a_2}\right)^2
\)
where, \(a_1\) and \(a_2\) are the amplitudes of the corresponding light wave.
Here, \(\frac{w_1}{w_2}=\frac{3}{1}\)
\(
\Rightarrow \quad\left(\frac{a_1}{a_2}\right)^2=\frac{3}{1} \quad \text { or } a_1: a_2=\sqrt{3}: 1
\)
The angle of incidence at which reflected light is totally polarised for refraction from air to glass (refractive index \(\mu\) ) is [UK PMT 2014]
(d) Suppose, \(i_p\) is the Brewster’s angle, when unpolarised light is incident at an polarising angle, the reflected component along \(O B\) and refracted component along \(O C\) in the following figure.
Now, \(\quad \angle B O Y+\angle Y O C=90^{\circ}\)
\(
\left(90^{\circ}-i_p\right)+\left(90^{\circ}-r\right)=90^{\circ}
\)
Here, \(r\) is the angle of refraction.
\(
\Rightarrow \quad 90^{\circ}-i_p=r
\)
According to Snell’s law, \(\mu=\frac{\sin i}{\sin r}\)
When \(i=i_p, r=90^{\circ}-i_p\), then
\(
\begin{aligned}
&\begin{aligned}
& \mu=\frac{\sin i_p}{\sin \left(90^{\circ}-i_p\right)}=\frac{\sin i_p}{\cos i_p}=\tan i_p \\
\therefore \quad & i_p=\tan ^{-1}(\mu)
\end{aligned}\\
&\text { where, } i_p \text { is polarised angle. }
\end{aligned}
\)
A polarised light of intensity \(I_0\) is passed through another polariser whose pass axis makes an angle of \(60^{\circ}\) with the pass axis of the former. What is the intensity of emergent polarised light from second polariser? [KCET 2014]
(d) By Malus’s law, \(\quad I=I_0 \cos ^2 \theta\)
(where, \(I=\) intensity of emergent polarised light, \(I_0=\) intensity passed through polariser)
Given, \(\theta=60^{\circ}, I=\) ?
\(
\Rightarrow \quad I=I_0 \times \cos ^2 60^{\circ}=I_0 \times\left(\frac{1}{2}\right)^2=\frac{I_0}{4}
\)
A fringe width of a certain interference pattern is \(\beta=0.002 \mathrm{~cm}\). What is the distance of 5th dark fringe from centre? [MHT CET 2014]
(c) The distance of dark fringe from centre is given by
\(
x_n=(2 n+1) \frac{\lambda D}{2 d}
\)
As, \(n=5\) for 5 th dark fringe.
As, \(n=5\) for 5 th dark fringe.
So, \(x_5=\frac{11}{2} \frac{\lambda D}{d}=\frac{11}{2} \beta \left(\because \frac{\lambda D}{d}=\beta\right)\)
\(
=11 / 2 \times 0.002=0.011 \mathrm{~cm}=1.1 \times 10^{-2} \mathrm{~cm}
\)
If two slits in Young’s experiment are 0.4 mm apart and fringe width on a screen 200 cm away is 2 mm , the wavelength of light illuminating the slits is [J & K CET 2013]
\(
\begin{aligned}
& \text { (c) Fringe width, } \beta=\frac{D \lambda}{d} \\
& \text { Given, } d=0.4 \mathrm{~mm}, D=200 \mathrm{~cm}=2000 \mathrm{~mm} \\
& \qquad \begin{array}{l}
\beta=2 \mathrm{~mm} \\
\therefore \quad 2=\frac{2000 \times \lambda}{0.4} \Rightarrow \lambda=400 \mathrm{~nm}
\end{array}
\end{aligned}
\)
Light of wavelength \(\lambda\) from a point source falls on a small circular obstacle of diameter \(d\). Dark and bright circular rings around a central bright spot are formed on a screen beyond the obstacle. The distance between the screen and obstacle is \(D\). Then, the condition for the formation of rings is [EAMCET 2013]
\(
\text { (b) Here, the condition for the formation of rings is } \lambda \approx \frac{d^2}{4 D} \text {. }
\)
Which of the following phenomena support the wave theory of light?
1. Scattering
2. Interference
3. Diffraction
4. Velocity of light in a denser medium is less than the velocity of light in the rarer medium. [Karnataka CET 2013]
(c) Wave theory of light explains the phenomenon of interference, diffraction and velocity of light in a denser medium or rarer medium, but this theory fails to explain the scattering of light.
\(\lambda_1\) and \(\lambda_2\) are used to illuminate the slits. \(\beta_1\) and \(\beta_2\) are the corresponding fringe widths. The wavelength \(\lambda_1\) can produce photoelectric effect when incident on a metal. But the wavelength \(\lambda_2\) cannot produce photoelectric effect. The correct relation between \(\beta_1\) and \(\beta_2\) is [Karnataka CET 2013]
(a) Fringe width \(\beta \propto \lambda\). As given that \(\lambda_1\) produces photoelectric effect, so \(\lambda_1<\lambda_2\).
Hence,\(\beta_1<\beta_2\)
When we close one slit in the Young’s double slit experiment, then [Kerala CET 2013]
(d) When one slit in a Young’s double-slit experiment is closed, the interference pattern disappears, and a single-slit diffraction pattern is observed. Therefore, the correct answer is (d) the diffraction pattern is observed.
Explanation:
Interference pattern:
In a typical Young’s double-slit experiment, light waves from two slits interfere, creating a series of bright and dark fringes on a screen.
Single-slit diffraction:
When only one slit is open, the light diffracts through that single slit, creating a central bright maximum and dimmer secondary maxima on either side.
A beam of light is incident on a glass slab \((\mu=1.54)\) in a direction as shown in the figure. The reflected light is analysed by a polaroid prism. On rotating the polaroid (take, \(\tan 57^{\circ}=1.54\) ) [Kerala CET 2013]
(c) Given, \(\mu=1.54\)
We know that, \(\theta=\tan ^{-1}(\mu) \Rightarrow \theta=\tan ^{-1}(1.54) \Rightarrow \theta=57^{\circ}\)
On rotating the polaroid, the reflected light is fully polarised. Hence, the intensity gradually reduced to zero and then again increases.
In Young’s double slit experiment, the phase difference between the two waves reaching at the location of the third dark fringe is [MP PMT 2013]
(c) In Young’s double-slit experiment, dark fringes occur at positions where the phase difference between the two waves is an odd multiple of \(\pi\). The formula for destructive interference (dark fringes) is given as:
\(
\Delta \phi=(2 n-1) \pi
\)
where \(\boldsymbol{\Delta} \boldsymbol{\phi}\) is the phase difference and \(\boldsymbol{n}\) is the order of the dark fringe, with \(n=1,2,3, \ldots\).
For the third dark fringe, \(\boldsymbol{n}=\mathbf{3}\).
\(
\begin{aligned}
& \Delta \phi=(2 \times 3-1) \pi \\
& \Delta \phi=(6-1) \pi \\
& \Delta \phi=5 \pi
\end{aligned}
\)
The phase difference between the two waves at the location of the third dark fringe is \(5 \pi\).
In Young’s double slit experiment, the fringe width is \(1 \times 10^{-4} \mathrm{~m}\). If the distance between the slit and screen is doubled and the distance between two slits is reduced to half and the wavelength is changed from \(6.4 \times 10^{-7} \mathrm{~m}\) to \(4.0 \times 10^{-7} \mathrm{~m}\), then the value of new fringe width will be [BCECE (Mains) 2012]
(a) Fringe width, \(\beta=\frac{D \lambda}{d}\) According to question, \(\frac{\beta_2}{\beta_1}=\frac{\lambda_2 D_2 d_1}{\lambda_1 D_1 d_2}\) Here, \(D_2=2 D_1\) and \(d_2=\frac{d_1}{2}\)
\(
\begin{aligned}
& \Rightarrow \quad \frac{\beta_2}{\beta_1}=\frac{\lambda_2\left(2 D_1\right) \times d_1}{\lambda_1\left(D_1\right) \times\left(\frac{d_1}{2}\right)}=4 \frac{\lambda_2}{\lambda_1}=\frac{4 \times 4 \times 10^{-7}}{6.4 \times 10^{-7}} \\
& \Rightarrow \quad \beta_2=\frac{4 \times 4 \times 10^{-7} \times 1 \times 10^{-4}}{6.4 \times 10^{-7}}=2.5 \times 10^{-4} \mathrm{~m}
\end{aligned}
\)
Assertion: The clouds in sky generally appear to be whitish.
Reason: Diffraction due to clouds is efficient in equal measure at all wavelengths. [AIIMS 2011]
(c) Let us first discuss the terms diffraction and scattering of light. The phenomenon in which the bending of light waves around the edges or corners of an obstacle or aperture happens is known as diffraction of light. When light passes through a medium in which the size of the particles present in it is of the order of wavelength of light, then light striking these particles deviates in different directions. This phenomena is known as scattering of light.
The size of the particles in the clouds is very large as compared to the wavelength of the incident light from the sun. Due to which diffraction/scattering of light hardly happens. Therefore, all the rays reflected are seen white. Hence, clouds normally appear to be whitish in colour.
Therefore, the assertion is true but reason is false.
In a Young’s double slit interference experiment, the fringe width obtained with a light of wavelength \(5900 Å\) was 1.2 mm for parallel narrow slits placed 2 mm apart. In this arrangement, if the slit separation is increased by one-and-half times the previous value, then the fringe width is [EAMCET 2011]
\(
\begin{aligned}
&\text { (b) By Young’s double slit interference experiment, } \beta=\frac{\lambda D}{d}\\
&\begin{array}{ll}
\text { Given, } & \beta_1=1.2 \mathrm{~mm}, \frac{d_2}{d_1}=1 \frac{1}{2}=1.5 \\
\text { So, } & \beta \propto \frac{1}{d} \Rightarrow \frac{\beta_1}{\beta_2}=\frac{1 / d_1}{1 / d_2} \\
\Rightarrow & \frac{\beta_1}{\beta_2}=\frac{d_2}{d_1}=1.5 \Rightarrow \frac{1.2}{\beta_2}=1.5 \\
\Rightarrow & \beta_2=\frac{1.2}{1.5}=\frac{4}{5}=0.8 \mathrm{~mm}
\end{array}
\end{aligned}
\)
In Young’s double slit experiment, the angular width of the fringes is \(0.20^{\circ}\) for the sodium light \((\lambda=5890 Å)\). In order to increase the angular width of the fringes by \(10 \%\), the necessary change in wavelength is [Manipal 2011]
(d) Let \(\lambda\) be the wavelength of monochromatic light incident on slit \(S\), then the angular distance between two consecutive fringes, i.e. the angular fringe width is
\(
\theta=\lambda / d \dots(i)
\)
where, \(d=\) distance between coherent sources.
Given, \(\frac{\Delta \theta}{\theta}=\frac{10}{100}\)
So, from Eq. (i),
\(
\begin{aligned}
& \frac{\Delta \lambda}{\lambda}=\frac{\Delta \theta}{\theta}=\frac{10}{100}=0.1 \\
\Rightarrow \quad \Delta \lambda & =0.1 \lambda=0.1 \times 5890 Å=589 Å(\text { increases })
\end{aligned}
\)
In Young’s double slit experiment, the intensity of light coming from one of the slits is doubled the intensity from the other slit. The ratio of the maximum intensity to the minimum intensity in the interference fringe pattern observed is [Punjab PMET, Manipal 2011]
(a) \(\frac{I_{\max }}{I_{\min }}=\frac{(\sqrt{2 I}+\sqrt{I})^2}{(\sqrt{2 I}-\sqrt{I})^2}=\left(\frac{\sqrt{2}+1}{\sqrt{2}-1}\right)^2 \text { (given) }\)
\(
\begin{aligned}
\frac{I_{\max }}{I_{\min }} & =\left[\frac{(\sqrt{2}+1)(\sqrt{2}+1)}{(\sqrt{2}-1)(\sqrt{2}+1)}\right]^2 \\
& =\left(\frac{2+1+2 \sqrt{2}}{2-1}\right)^2=\frac{9+8+12 \sqrt{2}}{1}=34
\end{aligned}
\)
In Young’s double slit experiment, if \(d, D\) and \(\lambda\) represents, the distance between the slits, the distance of the screen from the slits and wavelength of light used respectively, then the bandwidth is inversely proportional to [Kerala CEE 2011]
(b) The bandwidth is inversely proportional to the distance between the slits \(d\).
\(
\text { As, } \beta=\frac{\lambda D}{d} \Rightarrow \beta \propto \frac{1}{d}
\)
A Young’s double slit set up for interference is shifted from air to within water, then the fringe width [J & K CET 2011]
(b) If a Young’s double slit set up is shifted from air to water, the fringe width decreases.
Explanation: When submerged in water, the wavelength of light decreases compared to air, which results in a smaller fringe width.
Key points:
Fringe width formula: The fringe width is directly proportional to the wavelength of light.
Refractive index: Water has a higher refractive index than air, meaning light travels slower in water, resulting in a shorter wavelength.
Therefore, options (a), (c), and (d) are incorrect: because the fringe width does not become infinite, increase, or remain unchanged when the experiment is moved to water.
In the case of light waves from two coherent sources \(S_1\) and \(S_2\), there will be constructive interference at an arbitrary point \(P\), if the path difference, \(S_1 P-S_2 P\) is [J & K CET 2011]
(b) The path difference \(S_1 P-S_2 P\) is a whole number of wavelength, for the interference at an arbitrary point \(P\).
So, \(S_1 P-S_2 P=n \lambda \text { (for maximum intensity) }\)
In Young’s double slit experiment, fringes of width \(\beta\) are produced on a screen kept at a distance of 1 m from the slit. When the screen is moved away by \(5 \times 10^{-2} \mathrm{~m}\), fringe width changes by \(3 \times 10^{-5} \mathrm{~m}\). The separation between the slits is \(1 \times 10^{-3} \mathrm{~m}\). The wavelength of the light used is …nm. [KCET 2011]
\(
\begin{aligned}
&\text { (c) In Young’s double slit experiment, we have }\\
&\begin{aligned}
\beta & =\frac{\lambda D}{d} \\
\Delta \beta & =\frac{\lambda \Delta D}{d} \\
\lambda & =\frac{\Delta \beta d}{\Delta D} \\
\lambda & =\frac{3 \times 10^{-5} \times 1 \times 10^{-3}}{5 \times 10^{-2}}=6 \times 10^{-7} \mathrm{~m}=600 \mathrm{~nm}
\end{aligned}
\end{aligned}
\)
In a single slit diffraction of light of wavelengths by a slit of width \(e\), the size of the central maximum on a screen at a distance \(b\) is [MP PMT 2011]
(c) The direction in which the first minima occurs is \(\theta\) (say), then \(e \sin \theta=\lambda\)
or \(\quad e \theta=\lambda\) or \(\theta=\frac{\lambda}{e}(\because \theta \simeq \sin \theta\), when \(\theta\) is small \()\) Width of the central maximum \(=2 b \theta+e=\frac{2 b \lambda}{e}+e\)
A grating which would be most suitable for constructing a spectrometer for the visible and ultraviolet region, should have [Haryana PMT, CG PMT 2011]
(d) Grating with \(10^6\) lines \(/ \mathrm{cm}\) is suitable for constructing spectrometer for visible and ultraviolet region because this corresponds to the wavelength, equivalent to the wavelengths of visible and ultraviolet region.
In a single slit diffraction experiment, the width of the slit is made double its original width. Then, the central maximum on the diffraction pattern will become [BCECE, J & K CET 2011]
(a) Width of central maximum,
\(
\beta=\frac{2 D \lambda}{d}
\)
As, we increase \(d\) to \(2 d, \beta\) becomes \(\frac{\beta}{2}\).
So, it becomes narrower and fainter.
The slit width, when a light of wavelength \(6500 Å\) is incident on a slit, if first minima for red light is at \(30^{\circ}\), is [DUMET 2011]
(c) When rays of monochromatic light of wavelength \(\lambda\) are incident on a diffraction grating in which slit separation is \(d\), then for angle of diffraction \(\theta\), the following relation holds true.
\(
d \sin \theta=n \lambda
\)
where, \(n\) is called the spectrum order.
Given, \(n=1, \lambda=6500 Å=6500 \times 10^{-10} \mathrm{~m}\)
and \(\quad \sin 30^{\circ}=\frac{1}{2}\)
\(
\begin{array}{ll}
\Rightarrow & d=\frac{n \lambda}{\sin 30^{\circ}}=\frac{6500 \times 10^{-10}}{(1 / 2)} \\
\Rightarrow & d=1.3 \times 10^{-6} \mathrm{~m}
\end{array}
\)
The critical angle of a certain medium is \(\sin ^{-1}\left(\frac{3}{5}\right)\). The polarising angle of the medium is [KCET 2011]
(b) For polarising angle, \(\mu=\tan i_p\)
\(
\begin{aligned}
\mu & =\frac{1}{\sin C} \\
\tan i_p & =\frac{1}{\sin C}
\end{aligned}
\)
where, \(C=\) critical angle.
\(
\begin{array}{rlrl}
& \therefore \cot i_p =\sin \left(\sin ^{-1}\left(\frac{3}{5}\right)\right) \\
\Rightarrow & \cot i_p =\frac{3}{5} \text { or } \tan i=\frac{5}{3} \\
& \text { or } i_p =\tan ^{-1}\left(\frac{5}{3}\right)
\end{array}
\)
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