Angle of Deviation for Light Ray Refracting and Reflecting Inside Sphere
A light ray is incident on the surface of a sphere of refractive index n at an angle of incidence θ0. The ray partially refracts into the sphere with angle of refraction ϕ0 and then partly reflects from the back surface. The reflected ray then emerges out of the sphere after a partial refraction. The total angle of deviation of the emergent ray with respect to the incident ray is α. Match the quantities mentioned in List-I with their values in List-II and choose the correct option.
List-I(P) If n=2 and α=180∘, then all the possible values of θ0 will be(Q) If n=3 and α=180∘, then all the possible values of θ0 will be(R) If n=3 and α=180∘, then all the possible values of ϕ0 will be(S) If n=2 and θ0=45∘, then all the possible values of α will beList-II(1) 30∘ and 0∘(2) 60∘ and 0∘(3) 45∘ and 0∘(4) 150∘(5) 0∘
To determine the correct matching between List-I and List-II, we first establish the expression for the total deviation α of a light ray undergoing two refractions and one internal reflection inside a sphere of refractive index n.
1. General Derivation for Total Deviation
Let:
θ0 be the angle of incidence at the first surface.
ϕ0 be the angle of refraction inside the sphere.
By Snell's law at the first surface (air to sphere):
sinθ0=nsinϕ0
Due to the spherical symmetry of the sphere, the chord representing the ray inside the sphere forms an isosceles triangle with the center of the sphere. Thus:
The deviation at the first refraction (entry) is:
δ1=θ0−ϕ0
The angle of incidence at the back surface inside the sphere is also ϕ0. The deviation at internal reflection is:
δ2=180∘−2ϕ0
The angle of incidence at the exit surface inside the sphere is ϕ0, and the angle of refraction into air is θ0. The deviation at the second refraction (exit) is:
δ3=θ0−ϕ0
The total angle of deviation α of the emergent ray with respect to the incident ray is the sum of these three deviations:
α=δ1+δ2+δ3α=(θ0−ϕ0)+(180∘−2ϕ0)+(θ0−ϕ0)=180∘+2θ0−4ϕ0
2. Analysis of List-I Items
(P) For n=2 and α=180∘:
Substitute α=180∘ into the total deviation formula:
180∘=180∘+2θ0−4ϕ0⟹θ0=2ϕ0
Using Snell's law with n=2:
sinθ0=2sinϕ0sin(2ϕ0)=2sinϕ02sinϕ0cosϕ0=2sinϕ02sinϕ0(cosϕ0−1)=0
This yields two possibilities:
sinϕ0=0⟹ϕ0=0∘⟹θ0=0∘
cosϕ0=1⟹ϕ0=0∘⟹θ0=0∘
Thus, the only possible value of θ0 is 0∘.
P→(5)
(Q) For n=3 and α=180∘:
From α=180∘, we have θ0=2ϕ0.
Using Snell's law with n=3:
sinθ0=3sinϕ0sin(2ϕ0)=3sinϕ02sinϕ0cosϕ0=3sinϕ0sinϕ0(2cosϕ0−3)=0
This yields two solutions:
sinϕ0=0⟹ϕ0=0∘⟹θ0=0∘
2cosϕ0−3=0⟹cosϕ0=23⟹ϕ0=30∘⟹θ0=2(30∘)=60∘
Thus, the possible values of θ0 are 60∘ and 0∘.
Q→(2)
(R) For n=3 and α=180∘:
From the derivation in part (Q), the corresponding possible values for the angle of refraction ϕ0 are:
ϕ0=30∘ and 0∘
R→(1)
(S) For n=2 and θ0=45∘:
By Snell's law:
sin(45∘)=2sinϕ021=2sinϕ0⟹sinϕ0=21⟹ϕ0=30∘
Now, calculate the total deviation α:
α=180∘+2θ0−4ϕ0=180∘+2(45∘)−4(30∘)=180∘+90∘−120∘=150∘
S→(4)
Conclusion
The correct matching is:
P→5;Q→2;R→1;S→4
This corresponds to Option A.
Angle of Deviation for Light Ray Refracting and Reflecting Inside Sphere | Physics PYQ Solution - JEE Challenger