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Question: Derive the following expression for the refraction at concave spherical surface: \( \dfrac{\mu }{...

Derive the following expression for the refraction at concave spherical surface:
μv1u=μ1R.\dfrac{\mu }{v} - \dfrac{1}{u} = \dfrac{{\mu - 1}}{R}.

Explanation

Solution

Hint
A spherical mirror is a part of a sphere with a reflecting surface. If the inner surface is the reflective surface then the mirror is called a concave mirror and if the outer surface is the reflecting surface then the mirror is called a convex mirror. Here we have a concave reflecting surface for which we have to derive the given expression.

Complete step by step answer
Let us consider a concave mirror as shown in the diagram below,

The concave mirror is represented by MPNMPN . The refractive index of the medium of the spherical surface is given by μ\mu . We consider PP as the pole of the mirror, OO as the centre of curvature, and PCPC represents the principal axis of the refractive spherical surface. We consider a point object at OO . An incident ray travels through CC and it is normal to the spherical surface. It will not undergo any refraction hence it will travel in a straight line along PXPX . Another ray that we consider is OAOA . It will refract at the point AA bending towards the normal. At a point ii we will get a virtual image.
Let us consider the ray angles with the principal axis to be α,β\alpha,\beta , and γ\gamma respectively.
According to Snell’s law, we can write the refractive index as
μ=sinisinr\Rightarrow \mu = \dfrac{{\sin i}}{{\sin r}}
Where ii is the angle of incidence and rr is the angle of refraction.
Here we have very small ii and rr , hence we can write,
sini=i\Rightarrow \sin i = i And sinr=r\sin r = r in equation
We get,
μ=ir\Rightarrow \mu = \dfrac{i}{r}
From this we get,
i=μr\Rightarrow i = \mu r
By using the exterior angle theorem, from ΔAOC\Delta AOC we get,
γ=i+α\Rightarrow \gamma = i + \alpha
From this we get
i=γα\Rightarrow i = \gamma - \alpha
Now, by using exterior angle theorem in ΔIAC\Delta IAC , we get
γ=β+r\Rightarrow \gamma = \beta + r
From this we get,
r=γβ\Rightarrow r = \gamma - \beta
Substituting these values of ii and rr in equation we get,
(γα)=μ(γβ)\Rightarrow \left( {\gamma - \alpha } \right) = \mu \left( {\gamma - \beta } \right)
For a spherical surface, we can write the angle as
angle=arcradius\Rightarrow angle = \dfrac{{arc}}{{radius}}
We can write
α=PAOP\Rightarrow \alpha = \dfrac{{PA}}{{OP}}
And
β=PAIP\Rightarrow \beta = \dfrac{{PA}}{{IP}}
Also
γ=PACP\Rightarrow \gamma = \dfrac{{PA}}{{CP}}
Substituting these values of α,β\alpha ,\beta and γ\gamma in , we get
PAPCPAPO=μ(PAPCPAPI)\Rightarrow \dfrac{{PA}}{{PC}} - \dfrac{{PA}}{{PO}} = \mu \left( {\dfrac{{PA}}{{PC}} - \dfrac{{PA}}{{PI}}} \right)
Taking the common terms outside we get,
PA(1PC1PO)=μPA(1PC1PO)\Rightarrow PA\left( {\dfrac{1}{{PC}} - \dfrac{1}{{PO}}} \right) = \mu PA\left( {\dfrac{1}{{PC}} - \dfrac{1}{{PO}}} \right)
PA\Rightarrow PA gets cancelled as it is common on both sides. Now we have
1PC1PO=μ(1PC1PI)\Rightarrow \dfrac{1}{{PC}} - \dfrac{1}{{PO}} = \mu \left( {\dfrac{1}{{PC}} - \dfrac{1}{{PI}}} \right)
Now we have to apply the sign convention.
PC=R\Rightarrow PC = - R (where RR is the radius of curvature)
PI=v\Rightarrow PI = - v (Where vv is the distance of the image from the pole of the mirror)
PO=u\Rightarrow PO = - u (Where uu is the distance of the object from the pole of the mirror)
Putting these values in equation
We get,
(1R)(1u)=μ(1R+1v)\Rightarrow \left( {\dfrac{1}{{ - R}}} \right) - \left( {\dfrac{1}{{ - u}}} \right) = \mu \left( {\dfrac{1}{{ - R}} + \dfrac{1}{v}} \right)
Opening the brackets on LHS
1R+1u=μ(1R+1v)\Rightarrow\dfrac{{ - 1}}{R} + \dfrac{1}{u} = \mu \left( {\dfrac{{ - 1}}{R} + \dfrac{1}{v}} \right)
Opening the brackets on RHS
1R+1u=μR+μv\Rightarrow \dfrac{{ - 1}}{R} + \dfrac{1}{u} = \dfrac{\mu }{R} + \dfrac{\mu }{v}
Rearranging, we get
1R+μR=μv1u\Rightarrow \dfrac{{ - 1}}{R} + \dfrac{\mu }{R} = \dfrac{\mu }{v} - \dfrac{1}{u}
We can write this expression as,
μ1R=μv1u\Rightarrow \dfrac{{\mu - 1}}{R} = \dfrac{\mu }{v} - \dfrac{1}{u}
Hence we got the required expression for the concave refractive surface.

Note
According to the Cartesian sign convention,
-All distances as measured from the pole of the mirror.
-The distances that are measured in the direction of the incident light are taken as positive.
-The distances that are measured opposite to the direction of incident light is considered as negative.
-The height measured upward the principal axis is measured as positive and the height measured downward is measured negative.