Refraction Through Plane Surfaces
Optics of Class 12
Refraction Through Plane Surfaces
Glass Slab
The refracting surfaces of a glass slab are parallel to each other. When a light ray passes through a glass slab it is refracted twice at the two parallel faces and finally emerges out parallel to its incident direction. i.e. the ray undergoes no deviation, δ = 0. The angle of emergence (e) is equal to the angle of incidence (i). e = i |
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The lateral displacement (d) of the ray is the perpendicular distance between the incident and the emergent ray as shown in the fig.(15.27). It is given by
d = (15.10)
Apparent shift A point source S placed in a medium of refractive index μ is observed from air at a small angle α to the normal to the interface between the medium and air. If the source is at a distance h from the interface, find its apparent position h′ from the interface, as shown in the fig. (15.28). Applying geometry,
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Since alpha; and beta; are small, therefore, tan α ≈ sin α and tan β ≈ sin β
Thus,
Using Snell’s law
μ sin β = sin α
∴ sin α/sin β = μ
Now μ = h/h'
or h′ = h/μ
The apparent shift in the position of the source is
s = h – h′ = h(1-1/μ)(15.11)
If there are n number of slabs with different refractive indices are placed between the observer and the object, then the total apparent shift is equal to the summation of all the individual shifts.
s = s1 + s2 + ………..+sn
ors = h1 (15.12)
If the shift comes out to be positive, the image of the object shifts toward the observer, and vice-versa.
Example 15.7
A 2 cm thick layer of water covers a 3cm thick glass slab. A coin is placed at the bottom of the slab and is being observed from the air side along the normal to the surface. Find the apparent position of the coin from the surface. |
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Solution
Using equation , the total apparent shift is
s =
ors = = 1.5 cm Thus, h = h1 + h2 – s = 2 + 3 – 1.5 = 3.5 cm |
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Example 15.8
For the arrangement shown in the figure, a light ray is incident at an angle of 60o on the layer of water. Find the angle between this ray and the normal in the glass. |
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Solution
Using Snell’s law
μsinθ = constant
∴1 sin 60o =
Thus,sin r2 = or r2 = sin-1(1/√3) ≈ 35o
Important
1.When the glass slab of thickness t and refractive index μ is placed in the path of a convergent beam as shown in the figure(15.31 a), then the point of convergence is shifted by
s = t(1 - 1/μ)
2.When the same glass slab is placed in the path of a divergent beam as shown in fig.(15.31b), then the path of divergence also gets shifted by
s = t(1 - 1/μ)
Example 15.9
If a point object is placed at distance 20 cm in front of a concave mirror of focal length 10 cm, then the final image coincides with the object itself. But, if we place a glass slab (μ = 1.5) of thickness 3 cm between the mirror and the object. Then find the new position of the object so that the final image again coincides with the object. Also, draw the ray diagram.
Solution
As it is clear from the figure the position of the object is shifted by s away from the mirror. s = t(1 - 1/μ) = 3(1 - 1/3/2) = 1 cm Distance of object from the mirror is (20 + 1) = 21 cm |
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Total Internal Reflection
Fig.(15.32) shows a boundary between two media with refractive indices μ1 and μ2 where μ2 > μ1. A ray approaching the boundary from the medium of higher refractive index is refracted away from the normal. For small angle of incidence, there is both a reflected and a refracted ray. But, at a particular angle of incidence (called critical angle θc) the refracted ray emerges parallel to the surface. For any angle of incidence greater than θc the light is totally reflected back into the medium of higher refractive index. The phenomenon is called total internal reflection and was first noted by Kepler in 1604.
Applying Snell’s law at the critical angle μ2sinθc = μ1
or θc = If the rarer medium is air, μ1 = 1. Then, the values of critical angle for glass and water are given below. |
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Example 15.10
In the fig.(15.33) shown, for an angle of incidence i at the top surface, what is the minimum refractive index needed for total internal reflection at the vertical face?
Solution
Applying Snell’s law at the top surface
μ sin r = sin i (i)
For total internal reflection at the vertical face
μ sin θc = 1
Using geometry, θc = 90o – r
∴μ sin (90 – r) = 1
orμ cos r = 1 (ii)
On squaring and adding equation (i) and (ii), we get
μ2sin2r + μ2cos2r = 1 + sin2i
or μ = √1 + sin2i
Example 15.11
A point source of light is placed at the bottom of a tank containing a liquid (refractive index = μ) upto a depth h. A bright circular spot is seen on the surface of the liquid. Find the radius of this bright spot. |
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Solution
Rays coming out of the source and incidenting at an angle greater than θc will be reflected back into the liquid, therefore, the corresponding region on the surface will appear dark.
As obvious from the figure, the radius of the bright spot is given by
R = h tan θc =
orR =
Sincesinθc = 1/μ
∴R =
Example 15.12
The cross-section of the glass prism has the form of an isosceles triangle. One of the equal faces is silvered. A ray of light incident normally on the other equal face and after being reflected twice, emerges through the base of prism along the normal. Find the angle of the prism. |
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Solution
From the figure,
α = 90o – A
i = 90o - α = A (i)
Alsoβ = 90o – 2i = 90o – 2A
andr = 90o - β = 2A
Thus,γ = r = 2A
From geometry,
A + γ + γ = 180o
A + 4A = 180o
orA = 180/5 = 36o
PRISM
Prism is a transparent medium bounded by any number of surfaces in such a way that the surface on which light is incident and the surface from which light emerges are plane and non-parallel.
Important
1.Angle of prism or refracting angle (A) of prism means the angle between the faces on which light is incident and from which it emerges, as shown in the fig.(15.36).
2.Angle of deviation (δ) means the angle between emergent and incident rays i.e., the angle through which incident ray turns in passing through a prism. It is represented by δ and is shown in fig.(15.36).
3.If the faces of a prism on which light is incident and from which it emerges becomes parallel (as in fig.(15.37)), angle of prism will be zero and as incident ray will emerge parallel to itself, deviation will also be zero i.e., the prism will act as a slab.
4.If μ of the material of the prism becomes equal to that of surroundings, no refraction at its faces will take place and light will pass through it undeviated.
i.e., δ = 0
Condition of No Emergence
The light will not emerge out of a prism for all values of angle of incidence, ifr2 > θc for i = 90o(1)
Applying Snell’s law,
1 (sin 90) = μ sin r1
orr1 = sin-1(1/μ)i.e.r1 = θc (2)
From equations (1) and (2), r1 + r2 > 2θc (3) However, in a prism r1 + r2 = A (4) Therefore, from (3) and (4) A > 2 θc (5) orsin(A/2) > sin θc i.e.μ > cosec(A/2)(15.14) |
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Thus, a ray of light will not emerge out of a prism (whatever be the angle of incidence) if A > 2theta;c, that is, if mu; > cosec(A/2)
Condition of Grazing Emergence
If a ray can emerge out of a prism, the value of angle of incidence i for which angle of emergence e = 90o is called the condition of grazing emergence.
As it is obvious from figure, r2 = θc(1) Sincer1 + r2 = A ∴r1 = A – θc(2) From Snell’s law, we have 1 sin i = μ sin r1 By using equation (2), sin i = μsin(A - θc) orsin i = μ[sin A cos θc – cos A sin θc]
orsin i = μ[(sin A) |
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Sincesin θc = 1/μ
∴sini =
ori = (15.15)
Note that light will emerge out of a prism only if angle of incidence is greater than the angle of incidence i given by equation (15.15).
Deviation Produced by a Prism
As shown in the Fig.(15.40), the angle of deviation δ is given by
δ = (i – r1) + (e – r2) i.e.δ = (i + e) – (r1 + r2)(1) Since r1 + r2 = A δ = [i + e – A] If the angle of prism A is small, then i and e are also small, because, A = r1 + r2 Applying Snell’s law at the first and the second surface. |
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sin i = μ sin r1 ⇒i = μ r1
and sine = μ sin r2 ⇒e = μ r2
Thusδ = i + e – A = μ(r1 + r2) – A
orδ = A(μ - 1)
Maximum deviation
Deviation will be maximum when angle of incidence i is maximum (imax = 90o)
Thus,δmax = 90 + e – A (6)
However when i = 90o, 1 sin 90o = μ sin r1
orr1 = sin-1(1/μ)⇒r1 = θc
Thus, at the second surface,
μ sin r2 = 1 sine orsin e = μ sin(A - θc)
ore = sin-1[μsin(A - θc)] (7)
So equation (6) gives maximum deviation while (7) angle of emergence in condition of maximum deviation i.e. i = 90o.
Minimum deviation
Theory and experiment show that δ will be minimum when the angle of incidence is equal to the angle of emergence.
i = e
Thus,
δmin = (i + e) – A = 2i – A
Applying Snell’s law at each interface, we get
sin i = μ sin r1
andμ sin r2 = sin e = sin i
Thussin r1 = sin r2
orr1 = r2 = r (say)
Since r1 + r2 = A, therefore r = A/2
The refractive index of the prism is given by
μ = (15.16)
Note that if the prism is equilateral or isosceles then the ray inside the prism is parallel to its base.
Dispersion of Light by a Prism
When a beam of composite light (consisting of several wavelengths) passes though a prism, it splits into its constituent colours. This phenomenon is called dispersion. The band of colours thus obtained on a screen is called the spectrum. If white light is used, seven colours are obtained as shown in the figure. The sequence of colours is VIBGYOR, from bottom to top.
The dispersion of light takes place because the refractive index μ of the medium depends on the wavelength of light. An approximate empirical relation is given by Cauchy’s formula,
where A and B are constants. The smaller the value of λ, the larger is the value of μ. Thus, μ is maximum for violet colour and minimum for red. The deviation of a ray depends on μ, it is larger for higher μ. Hence, violet suffers the maximum deviation and red the minimum.
Total angular dispersion is
θ = δv – δr.
where δv and δr are the deviations for violet and red light respectively.
Dispersive Power of a Prism
The ratio of dispersion to mean deviation is called dispersive power,
where δy is the deviation of yellow light (whose wavelength is considered as mean of all the wavelengths present)
For a prism, δ = (μ – 1)A
∴(15.17)
The dispersive power has no units and no dimensions. Its value depends on the material of the prism.
From a single prism, it is not possible to get deviation without dispersion, or to get dispersion without deviation.
Deviation Without Dispersion (Achromatic Prism)
It is possible to combine two prisms of different materials in such a way that each cancels the dispersion due to the other. Thus, the net dispersion is zero but a deviation is produced. The required condition is (μv – μr) A = (μv' – μr') A' which is equivalent to ωδ = ω′δ′(15.18) |
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where δ is the deviation for the mean ray.
Dispersion without Deviation
Two prisms can be combined in such a way that the deviation of the mean ray produced by one is equal and opposite to that produced by the other. Such a combination is called a direct vision prism. The required condition is (μ – 1) A = (μ′ – 1) A′(15.19) |
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