RAY OPTICS - I
1. Refraction of Light
2. Laws of Refraction
3. Principle of Reversibility of Light
4. Refraction through a Parallel Slab
5. Refraction through a Compound Slab
6. Apparent Depth of a Liquid
7. Total Internal Reflection
8. Refraction at Spherical Surfaces - Introduction
9. Assumptions and Sign Conventions
10.Refraction at Convex and Concave Surfaces
11.Lens Maker’s Formula
12.First and Second Principal Focus
13.Thin Lens Equation (Gaussian Form)
14.Linear Magnification
Created by C. Mani, Principal, K V No.1, AFS, Jalahalli West, Bangalore
Refraction of Light:
Refraction is the phenomenon of change in the path of light as it travels
from one medium to another (when the ray of light is incident obliquely).
It can also be defined as the phenomenon of change in speed of light
from one medium to another.
Rarer
Rarer
Denser
N
N
r
i
r
i
Laws of Refraction:
I Law: The incident ray, the normal to
the refracting surface at the point of
incidence and the refracted ray all lie in
the same plane.
II Law: For a given pair of media and for
light of a given wavelength, the ratio of
the sine of the angle of incidence to the
sine of the angle of refraction is a
constant. (Snell’s Law)
μ =
sin i
sin r
(The constant μ is called refractive index of the medium,
i is the angle of incidence and r is the angle of
refraction.)
μ
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
TIPS:
1. μ of optically rarer medium is lower and that of a denser medium is higher.
2. μ of denser medium w.r.t. rarer medium is more than 1 and that of rarer
medium w.r.t. denser medium is less than 1. (μair = μvacuum = 1)
3. In refraction, the velocity and wavelength of light change.
4. In refraction, the frequency and phase of light do not change.
5. aμm = ca / cm and aμm = λa / λm
Principle of Reversibility of Light:
Rarer
(a)
N
r
i
Denser
(b)
sin i
aμb =
sin r
sin r
bμa =
sin i
aμb x bμa = 1 or aμb = 1 / bμa
If a ray of light, after suffering any number of
reflections and/or refractions has its path
reversed at any stage, it travels back to the
source along the same path in the opposite
direction.
A natural consequence of the principle of reversibility is that the image and object
positions can be interchanged. These positions are called conjugate positions.
μ
Refraction through a Parallel Slab:
Rarer (a)
Rarer (a)
Denser
(b)
N
N
r1
i1
i2
r2
M
t
δ
y
sin i1
aμb =
sin r1
sin i2
bμa =
sin r2
But aμb x bμa = 1
sin i1
sin r1
sin i2
sin r2
x = 1
It implies that i1 = r2 and i2 = r1
since i1 ≠ r1 and i2 ≠ r2.
μ
Lateral Shift:
t sin δ
y =
cos r1
t sin(i1- r1)
y =
cos r1
or
Ray optics 1 (1).ppt of physics class 12
Refraction through a Compound Slab:
Rarer (a)
Rarer (a)
Denser
(b)
N
N
μb
r1
i1
r1
r2
r2
i1
Denser
(c)
μc
N
sin i1
aμb =
sin r1
sin r1
bμc =
sin r2
aμb x bμc x cμa = 1
sin r2
cμa =
sin i1
aμb x bμc = aμc
or
bμc = aμc / aμb
or
μa
μc > μb
Apparent Depth of a Liquid:
Rarer (a)
Denser (b)
O
O’
N
μb
hr
ha
i
r
r
i
sin i
bμa =
sin r
sin r
aμb =
sin i
or
hr
aμb =
ha
=
Real depth
Apparent depth
Apparent Shift:
Apparent shift = hr - ha = hr – (hr / μ)
= hr [ 1 - 1/μ]
TIPS:
1. If the observer is in rarer medium and the object is in denser medium then
ha < hr. (To a bird, the fish appears to be nearer than actual depth.)
2. If the observer is in denser medium and the object is in rarer medium then
ha > hr. (To a fish, the bird appears to be farther than actual height.)
μa
Total Internal Reflection:
Total Internal Reflection (TIR) is the phenomenon of complete reflection of
light back into the same medium for angles of incidence greater than the
critical angle of that medium.
N N N N
O
r = 90°
ic i > ic
i
Rarer
(air)
Denser
(glass)
μg
μa
Conditions for TIR:
1. The incident ray must be in optically denser medium.
2. The angle of incidence in the denser medium must be greater than the
critical angle for the pair of media in contact.
Relation between Critical Angle and Refractive Index:
Critical angle is the angle of incidence in the denser medium for which the
angle of refraction in the rarer medium is 90°.
sin i
gμa =
sin r
sin ic
=
sin 90°
= sin ic
or
1
aμg =
gμa
1
aμg =
sin ic
or
1
sin ic =
aμg
λg
sin ic =
λa
Also
Red colour has maximum value of critical angle and Violet colour has
minimum value of critical angle since,
1
sin ic =
aμg
=
1
a + (b/ λ2
)
Applications of T I R:
1. Mirage formation
2. Totally reflecting Prisms
3. Optical Fibres
4.Sparkling of Diamonds
TOTALLY REFLECTING PRISMS
Spherical Refracting Surfaces:
A spherical refracting surface is a part of a sphere of refracting material.
A refracting surface which is convex towards the rarer medium is called
convex refracting surface.
A refracting surface which is concave towards the rarer medium is
called concave refracting surface.
•
•
C C
P P
R R
A B A
B
APCB – Principal Axis
C – Centre of Curvature
P – Pole
R – Radius of Curvature
•
•
Denser Medium
Denser Medium Rarer Medium
Rarer Medium
Assumptions:
1. Object is the point object lying on the principal axis.
2. The incident and the refracted rays make small angles with the principal
axis.
3. The aperture (diameter of the curved surface) is small.
New Cartesian Sign Conventions:
1. The incident ray is taken from left to right.
2. All the distances are measured from the pole of the refracting surface.
3. The distances measured along the direction of the incident ray are
taken positive and against the incident ray are taken negative.
4. The vertical distances measured from principal axis in the upward
direction are taken positive and in the downward direction are taken
negative.
Refraction at Convex Surface:
(From Rarer Medium to Denser Medium - Real Image)
•
C
P
R
O
•
Denser Medium
Rarer Medium
• •
I
M
μ2
μ1
α β
γ
i
r
i = α + γ
γ = r + β or r = γ - β
A
tan α =
MA
MO
tan β =
MA
MI
tan γ =
MA
MC
or α =
MA
MO
or β =
MA
MI
or γ =
MA
MC
According to Snell’s law,
μ2
sin i
sin r μ1
= or
i
r μ1
=
μ2
or μ1 i = μ2 r
Substituting for i, r, α, β and γ, replacing M by P and rearranging,
μ1
PO
μ2
PI
μ2 - μ1
PC
+ =
Applying sign conventions with values,
PO = - u, PI = + v and PC = + R
v
u
μ1
- u
μ2
v
μ2 - μ1
R
+ =
N
Refraction at Convex Surface:
(From Rarer Medium to Denser Medium - Virtual
Image)
μ1
- u
μ2
v
μ2 - μ1
R
+ =
Refraction at Concave Surface:
(From Rarer Medium to Denser Medium - Virtual
Image)
μ1
- u
μ2
v
μ2 - μ1
R
+ =
•
C
P R
•
Denser Medium
Rarer Medium
• •
I M
μ2
μ1
α
β γ
i r
A
v
u
O
N
O
•
C P
R
•
Denser Medium
Rarer Medium
•
I M
μ2
μ1
α β γ
r
A
v
u
•
i
N
Refraction at Convex Surface:
(From Denser Medium to Rarer Medium -
Real Image)
•
C P
R
O
•
Denser Medium Rarer Medium
• •
I
M
μ2 μ1
α β
γ
r
A
v
u
N
i
μ2
- u
μ1
v
μ1 - μ2
R
+ =
Refraction at Convex Surface:
(From Denser Medium to Rarer Medium - Virtual
Image)
μ2
- u
μ1
v
μ1 - μ2
R
+ =
Refraction at Concave Surface:
(From Denser Medium to Rarer Medium -
Virtual Image)
μ2
- u
μ1
v
μ1 - μ2
R
+ =
Note:
1. Expression for ‘object in rarer medium’ is same for whether it is real or
virtual image or convex or concave surface.
2. Expression for ‘object in denser medium’ is same for whether it is real or
virtual image or convex or concave surface.
3. However the values of u, v, R, etc. must be taken with proper sign
conventions while solving the numerical problems.
4. The refractive indices μ1 and μ2 get interchanged in the expressions.
μ1
- u
μ2
v
μ2 - μ1
R
+ =
μ2
- u
μ1
v
μ1 - μ2
R
+ =
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Lens Maker’s Formula:
R1
P1
•
O
•
μ2
μ1
i
A
v
u
N1
R2
C1
• •
I1
N2
L
C
N
P2
•
C2
•
I
•
μ1
For refraction at
LP1N,
μ1
CO
μ2
CI1
μ2 - μ1
CC1
+ =
(as if the image is
formed in the denser
medium)
For refraction at
LP2N,
(as if the object is in the denser medium and the image is formed in the rarer
medium)
μ2
-CI1
μ1
CI
-(μ1 - μ2)
CC2
+ =
Combining the refractions at both the surfaces,
μ1
CO
(μ2 - μ1)(
CC1
+ =
1
μ1
CI CC2
+ )
1
Substituting the values
with sign conventions,
1
- u
(μ2 - μ1)
R1
+ =
1
1
v R2
- )
1
(
μ1
Since μ2 / μ1 = μ
1
- u
μ2
R1
+ =
1
1
v R2
- )
1
(
μ1
- 1)
(
or
1
- u
(μ – 1)
R1
+ =
1
1
v R2
- )
1
(
When the object is kept at infinity, the image is formed at the principal focus.
i.e. u = - ∞, v = + f.
So, (μ – 1)
R1
=
1
1
f R2
- )
1
(
This equation is called ‘Lens Maker’s Formula’.
Also, from the above equations we get,
1
- u f
+ =
1
1
v
First Principal Focus:
First Principal Focus is the point on the principal axis of the lens at which if
an object is placed, the image would be formed at infinity.
F1
f1
F2
f2
Second Principal Focus:
Second Principal Focus is the point on the principal axis of the lens at
which the image is formed when the object is kept at infinity.
F2
f2
F1
f1
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Thin Lens Formula: For Convex Lens:
f
•
R
u
C
A
B
A’
B’
M
Triangles ABC and A’B’C are similar.
A’B’
AB
=
CB’
CB
Triangles MCF2 and A’B’F2 are similar.
A’B’
MC
=
B’F2
CF2
v
A’B’
AB
=
B’F2
CF2
or
•
2F2
•
F2
•
F1
•
2F1
CB’
CB
=
B’F2
CF2
CB’
CB
=
CB’ - CF2
CF2
According to new Cartesian sign
conventions,
CB = - u, CB’ = + v and CF2 = + f.
1
v f
- =
1
1
u
Linear Magnification:
Linear magnification produced by a lens is defined as the ratio of the size of
the image to the size of the object.
m =
I
O
A’B’
AB
=
CB’
CB
+ I
- O
=
+ v
- u
According to new Cartesian sign
conventions,
A’B’ = + I, AB = - O, CB’ = + v and
CB = - u.
m
I
O
=
v
u
=
or
Magnification in terms of v and f:
m =
f - v
f
Magnification in terms of u and f:
m =
f
f - u
Power of a Lens:
Power of a lens is its ability to bend a ray of light falling on it and is reciprocal
of its focal length. When f is in metre, power is measured in Dioptre (D).
P =
1
f
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12
Ray optics 1 (1).ppt of physics class 12

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Ray optics 1 (1).ppt of physics class 12

  • 1. RAY OPTICS - I 1. Refraction of Light 2. Laws of Refraction 3. Principle of Reversibility of Light 4. Refraction through a Parallel Slab 5. Refraction through a Compound Slab 6. Apparent Depth of a Liquid 7. Total Internal Reflection 8. Refraction at Spherical Surfaces - Introduction 9. Assumptions and Sign Conventions 10.Refraction at Convex and Concave Surfaces 11.Lens Maker’s Formula 12.First and Second Principal Focus 13.Thin Lens Equation (Gaussian Form) 14.Linear Magnification Created by C. Mani, Principal, K V No.1, AFS, Jalahalli West, Bangalore
  • 2. Refraction of Light: Refraction is the phenomenon of change in the path of light as it travels from one medium to another (when the ray of light is incident obliquely). It can also be defined as the phenomenon of change in speed of light from one medium to another. Rarer Rarer Denser N N r i r i Laws of Refraction: I Law: The incident ray, the normal to the refracting surface at the point of incidence and the refracted ray all lie in the same plane. II Law: For a given pair of media and for light of a given wavelength, the ratio of the sine of the angle of incidence to the sine of the angle of refraction is a constant. (Snell’s Law) μ = sin i sin r (The constant μ is called refractive index of the medium, i is the angle of incidence and r is the angle of refraction.) μ
  • 8. TIPS: 1. μ of optically rarer medium is lower and that of a denser medium is higher. 2. μ of denser medium w.r.t. rarer medium is more than 1 and that of rarer medium w.r.t. denser medium is less than 1. (μair = μvacuum = 1) 3. In refraction, the velocity and wavelength of light change. 4. In refraction, the frequency and phase of light do not change. 5. aμm = ca / cm and aμm = λa / λm Principle of Reversibility of Light: Rarer (a) N r i Denser (b) sin i aμb = sin r sin r bμa = sin i aμb x bμa = 1 or aμb = 1 / bμa If a ray of light, after suffering any number of reflections and/or refractions has its path reversed at any stage, it travels back to the source along the same path in the opposite direction. A natural consequence of the principle of reversibility is that the image and object positions can be interchanged. These positions are called conjugate positions. μ
  • 9. Refraction through a Parallel Slab: Rarer (a) Rarer (a) Denser (b) N N r1 i1 i2 r2 M t δ y sin i1 aμb = sin r1 sin i2 bμa = sin r2 But aμb x bμa = 1 sin i1 sin r1 sin i2 sin r2 x = 1 It implies that i1 = r2 and i2 = r1 since i1 ≠ r1 and i2 ≠ r2. μ
  • 10. Lateral Shift: t sin δ y = cos r1 t sin(i1- r1) y = cos r1 or
  • 12. Refraction through a Compound Slab: Rarer (a) Rarer (a) Denser (b) N N μb r1 i1 r1 r2 r2 i1 Denser (c) μc N sin i1 aμb = sin r1 sin r1 bμc = sin r2 aμb x bμc x cμa = 1 sin r2 cμa = sin i1 aμb x bμc = aμc or bμc = aμc / aμb or μa μc > μb
  • 13. Apparent Depth of a Liquid: Rarer (a) Denser (b) O O’ N μb hr ha i r r i sin i bμa = sin r sin r aμb = sin i or hr aμb = ha = Real depth Apparent depth Apparent Shift: Apparent shift = hr - ha = hr – (hr / μ) = hr [ 1 - 1/μ] TIPS: 1. If the observer is in rarer medium and the object is in denser medium then ha < hr. (To a bird, the fish appears to be nearer than actual depth.) 2. If the observer is in denser medium and the object is in rarer medium then ha > hr. (To a fish, the bird appears to be farther than actual height.) μa
  • 14. Total Internal Reflection: Total Internal Reflection (TIR) is the phenomenon of complete reflection of light back into the same medium for angles of incidence greater than the critical angle of that medium. N N N N O r = 90° ic i > ic i Rarer (air) Denser (glass) μg μa Conditions for TIR: 1. The incident ray must be in optically denser medium. 2. The angle of incidence in the denser medium must be greater than the critical angle for the pair of media in contact.
  • 15. Relation between Critical Angle and Refractive Index: Critical angle is the angle of incidence in the denser medium for which the angle of refraction in the rarer medium is 90°. sin i gμa = sin r sin ic = sin 90° = sin ic or 1 aμg = gμa 1 aμg = sin ic or 1 sin ic = aμg λg sin ic = λa Also Red colour has maximum value of critical angle and Violet colour has minimum value of critical angle since, 1 sin ic = aμg = 1 a + (b/ λ2 )
  • 16. Applications of T I R: 1. Mirage formation 2. Totally reflecting Prisms 3. Optical Fibres 4.Sparkling of Diamonds
  • 18. Spherical Refracting Surfaces: A spherical refracting surface is a part of a sphere of refracting material. A refracting surface which is convex towards the rarer medium is called convex refracting surface. A refracting surface which is concave towards the rarer medium is called concave refracting surface. • • C C P P R R A B A B APCB – Principal Axis C – Centre of Curvature P – Pole R – Radius of Curvature • • Denser Medium Denser Medium Rarer Medium Rarer Medium
  • 19. Assumptions: 1. Object is the point object lying on the principal axis. 2. The incident and the refracted rays make small angles with the principal axis. 3. The aperture (diameter of the curved surface) is small. New Cartesian Sign Conventions: 1. The incident ray is taken from left to right. 2. All the distances are measured from the pole of the refracting surface. 3. The distances measured along the direction of the incident ray are taken positive and against the incident ray are taken negative. 4. The vertical distances measured from principal axis in the upward direction are taken positive and in the downward direction are taken negative.
  • 20. Refraction at Convex Surface: (From Rarer Medium to Denser Medium - Real Image) • C P R O • Denser Medium Rarer Medium • • I M μ2 μ1 α β γ i r i = α + γ γ = r + β or r = γ - β A tan α = MA MO tan β = MA MI tan γ = MA MC or α = MA MO or β = MA MI or γ = MA MC According to Snell’s law, μ2 sin i sin r μ1 = or i r μ1 = μ2 or μ1 i = μ2 r Substituting for i, r, α, β and γ, replacing M by P and rearranging, μ1 PO μ2 PI μ2 - μ1 PC + = Applying sign conventions with values, PO = - u, PI = + v and PC = + R v u μ1 - u μ2 v μ2 - μ1 R + = N
  • 21. Refraction at Convex Surface: (From Rarer Medium to Denser Medium - Virtual Image) μ1 - u μ2 v μ2 - μ1 R + = Refraction at Concave Surface: (From Rarer Medium to Denser Medium - Virtual Image) μ1 - u μ2 v μ2 - μ1 R + = • C P R • Denser Medium Rarer Medium • • I M μ2 μ1 α β γ i r A v u O N O • C P R • Denser Medium Rarer Medium • I M μ2 μ1 α β γ r A v u • i N
  • 22. Refraction at Convex Surface: (From Denser Medium to Rarer Medium - Real Image) • C P R O • Denser Medium Rarer Medium • • I M μ2 μ1 α β γ r A v u N i μ2 - u μ1 v μ1 - μ2 R + = Refraction at Convex Surface: (From Denser Medium to Rarer Medium - Virtual Image) μ2 - u μ1 v μ1 - μ2 R + = Refraction at Concave Surface: (From Denser Medium to Rarer Medium - Virtual Image) μ2 - u μ1 v μ1 - μ2 R + =
  • 23. Note: 1. Expression for ‘object in rarer medium’ is same for whether it is real or virtual image or convex or concave surface. 2. Expression for ‘object in denser medium’ is same for whether it is real or virtual image or convex or concave surface. 3. However the values of u, v, R, etc. must be taken with proper sign conventions while solving the numerical problems. 4. The refractive indices μ1 and μ2 get interchanged in the expressions. μ1 - u μ2 v μ2 - μ1 R + = μ2 - u μ1 v μ1 - μ2 R + =
  • 26. Lens Maker’s Formula: R1 P1 • O • μ2 μ1 i A v u N1 R2 C1 • • I1 N2 L C N P2 • C2 • I • μ1 For refraction at LP1N, μ1 CO μ2 CI1 μ2 - μ1 CC1 + = (as if the image is formed in the denser medium) For refraction at LP2N, (as if the object is in the denser medium and the image is formed in the rarer medium) μ2 -CI1 μ1 CI -(μ1 - μ2) CC2 + = Combining the refractions at both the surfaces, μ1 CO (μ2 - μ1)( CC1 + = 1 μ1 CI CC2 + ) 1 Substituting the values with sign conventions, 1 - u (μ2 - μ1) R1 + = 1 1 v R2 - ) 1 ( μ1
  • 27. Since μ2 / μ1 = μ 1 - u μ2 R1 + = 1 1 v R2 - ) 1 ( μ1 - 1) ( or 1 - u (μ – 1) R1 + = 1 1 v R2 - ) 1 ( When the object is kept at infinity, the image is formed at the principal focus. i.e. u = - ∞, v = + f. So, (μ – 1) R1 = 1 1 f R2 - ) 1 ( This equation is called ‘Lens Maker’s Formula’. Also, from the above equations we get, 1 - u f + = 1 1 v
  • 28. First Principal Focus: First Principal Focus is the point on the principal axis of the lens at which if an object is placed, the image would be formed at infinity. F1 f1 F2 f2 Second Principal Focus: Second Principal Focus is the point on the principal axis of the lens at which the image is formed when the object is kept at infinity. F2 f2 F1 f1
  • 32. Thin Lens Formula: For Convex Lens: f • R u C A B A’ B’ M Triangles ABC and A’B’C are similar. A’B’ AB = CB’ CB Triangles MCF2 and A’B’F2 are similar. A’B’ MC = B’F2 CF2 v A’B’ AB = B’F2 CF2 or • 2F2 • F2 • F1 • 2F1 CB’ CB = B’F2 CF2 CB’ CB = CB’ - CF2 CF2 According to new Cartesian sign conventions, CB = - u, CB’ = + v and CF2 = + f. 1 v f - = 1 1 u
  • 33. Linear Magnification: Linear magnification produced by a lens is defined as the ratio of the size of the image to the size of the object. m = I O A’B’ AB = CB’ CB + I - O = + v - u According to new Cartesian sign conventions, A’B’ = + I, AB = - O, CB’ = + v and CB = - u. m I O = v u = or Magnification in terms of v and f: m = f - v f Magnification in terms of u and f: m = f f - u Power of a Lens: Power of a lens is its ability to bend a ray of light falling on it and is reciprocal of its focal length. When f is in metre, power is measured in Dioptre (D). P = 1 f