Assume 'small aperture' ⇒ Paraxial is valid.
i.e. M is close to P
⇒α,β,γ,i and r are small
⇒tanα≈sinα≈α.
tanβ≈sinβ≈β, etc.
Refracted light can ba minimized by using Anti-reflection coatings.
Angles
i=α+β
r=β−γ
α≈tanα=ODMD≈OPMD
β≈tanβ−CDMD≈CPMD
γ≈tanγ=IDMD≈IPMP
∴i=OPMD+CPMD-----(3)
r=CPMDIPMD-----(4)
Using Snell's Law
sinrsini=n1n2⇒n1sini=n2sinr
For small i,r : sini≈i,sinr≈r⇒n1i=n2r-----(5)
∴n1(OPMD+CPMD=n2(CPMDIPMD)-----(6)
Refraction at a spherical surface :
n1(OPMD+CPMD=n2(CPMDIPMD)→(eqn−6)
OPn1+IPn2=CP(n2−n1)→(eqn−7)
Applying 'sign convention',
OP = -u, CP = R, IP = v
−un1+vn2=Rn2−n1
vn2−un1=Rn2−n1→(eqn−8)
Gives a relation between object distance and image distance in terms of r.i and R.O.C of the spherical surface.
Determine the position of the image when the point object is at a distance of (i) 100cm,
(ii) 50cm (iii) 25cm
in front of the spherical surface.
Solution: vn2−un1=R(n2−n1)---(1)
u1=−100cm,R=25cm
n1=1.0,n2=1.5
v1.5−(−100)1.0=2.51.5−1.0=501
gives v=150cm
i.e Real image in glass medium.
(2) u=−25cm
v1.5−(−25)1.0=501
v1.5=501−251=−501
v=−75cm, virtual image
"Thin Lens" OA≈OP≈OB
IA≈IP≈IB
't' is small
AB = thickness of the lens.
medium.1 → Air n1=1
medium.2 → Glass material of r.i n2
v1n2−un1=R1n2−n1→(1)
vn1−un=R2n1−n2→(2)
Adding eq(1) and eq(2)
vn1−un1=(n2−n1)(R11−R21)
v1−u1=(n1n2−1)(R11−R21)→(4) constant for a given lens
For large object distances, u1→0∴v1=constant.
⇒ Image point is fixed, independent of u, and is called principal focus F. The corresponding image distance is called the focal length, f.
∴v1=f1=(n1n2−1)(R11−R21)
From (4) & (5).
v1−u1=f1→(6)
Lens formula
v1−u1=f1 (Lens formula)
with f1=(n1n2−1)(R11−R21)
for u→∞, rays from object are almost parallel to the axis, and v=f, the focal length.
For a lens immersed in a liquid
of r.i⋅nl,fl1=(nln2−1)(R11−R21)
Since nl>nair(=1),
fe>fair
For common applications of
a lens, n1=nair=1 n2=n, r.i. of the material of lens
∴f1=(n−1)(R11−R21)→ (Lens-maker's formula.)
The formula indicates to the choice of R1 & R2 to obtain a desired focal length.
For a symmetric biconvex lens, R1=−R2=R
⇒f1 = (n−1)(R1 - (−R)1) = R2(n−2)
n>1 ⇒ f>0 ⇒ "converying lens"
For a symmetric biconvex lens,
f1=R2(n−1)
f=2R(n−1)1→(1)
For a symmetric biconcave lens,
R1=−R,R2=R gives
f=−2R(n−1)1→(2)
since n>1, f< 0 in Equation(2)
⇒ Diverging lens
for n=1.5 , f=R and for n=2, f=2R
Normally n2>n1. if n1>n2?
for n2<n1
Is |f2| = |f|?
f1=(n1n2−1)(R11−R21)
f21=(n1n2−1)(R21=−R11)
-f1
n1 is the same (medium) on both sides of the lens, even through R1=R2.
Thus, a lens has two principal focus.
F1 is the first principal focus, f1→ first focal length
F2 is the second principal focus,
f2→ second focal length
F1 and F2 are equidistant from the lens.
Normally, when we refer to the. "focus of a lens", wa refer to the point F2, and the focal length f2 Then, what is the importance of F1 ?
△ABP and △A′B′P are similar.
BPAB=P′B′A′B′ or ABA′B′=BPB′P:
Applying sign convention :
−hh′=−uv or m=hh′=uv
△ABP and △A′B′P are similar;
∴ABA′B′=BPB′P
i.e hh′=−u−v=uv
or m=uv as before.
Rays 1,2 and 3 appear to come from point A
∴ A'B' is a virtual image.