2. 1. Two-slit interference
Optical path L = nr (n: index of refraction, r: distance between two points)
Notes
d < 1 mm and i ~ sereval mm.
Sign () implies the symmetry of interference fringes at two sides of central line.
Interference max: L2 – L1 = dsin = m position of bright fringe:
d
R
mλ
yb
m
Interference min: position of dark fringe:
2
1
2
1
2
λ
m
θ
sin
d
L
L
d
R
λ
m
yd
m
2
1
2
Width of fringe:
d
R
λ
y
y
i m
m
1
Most important equations
S1
S2
P
(normally, is considered very small)
R
r1 = L1
r2 = L2
= L2 – L1 = dsin
d
y = Rtg
H
O
r
Notes: d = distance; R = Range, L = optical path length
S1
S2
S
y, Intensity
Observation
screen
m = 2, 2nd order max.
m = 0, central max.
m = 1, 1st order max.
m = 2, 2nd order max.
m = 1, 1st order max.
m = 0, 1nd min.
m = 1, 2nd min.
m = 0, 1nd min.
m = 1, 2nd min.
m = 0, 1, 2, 3, …
Model
4. 4
2. Thin film interference
n
m
tb
m
4
1
2
Bright fringe: (one phase shift ray) or (both phase shift rays)
n
m
td
m
4
1
2
Dark fringe: (one phase shift ray) or both phase shift rays)
n
m
td
m
2
n
m
tb
m
2
Film thickness should be < 1 m (corresponding to light’s wavelength)
Observed position corresponding to the film thickness (t)
Phase shift at the interface of two media, index of refraction n1 & n2
if n1 > n2 no phase shift;
if n1 < n2 phase shift of reflected ray;
1
2
1
2
2 t
Incidence
n2
A C
B
D
n1
2
Phase
shift
No phase shift
Constructive condition:
2
1
2
1
2
m
L
L
one of two reflected rays has phase-shift
Destructive condition:
m
L
L
1
2
Incidence light to film surface is nearly
normal 2 0 & cos2 1 path
difference L2 – L1 = 2n2tcos2 = 2nt
= n
Constructive condition:
2
1
2
1
2
m
L
L
Both reflected rays has phase-shift
Destructive condition:
m
L
L
1
2
5. 5
Light
source
Reflection
mirror
Glass
plates
Optical
Microscope
Air film between either two glass plates or one upper convex glass len with
large curvature radius (~ m) and one lower glass plate (usually n > nair).
Thickness t gradually increased from 0 to 1 m with very small inclined
angle ( ~ several percentage of degree)
Light
source
Reflection
mirror
Wegde-like air gap Convex
glass len
Glass
plate
Optical Microscope
Newton fringes
Air wedge
2. Thin film interference
6. Incident
ray
nG
R
O
R - t
1
2
nG
t
rm
Reflection
rays
Bright fringe:
2
1
2
2
1
2
m
t
L
L
Dark fringe: L2 – L1 = 2t = m
4
1
2
m
tb
m
Wedge’s thickness at bright fringes:
Wedge’s thickness at dark fringes:
2
m
td
m
Fringe’s width:
α
λ
α
sin
t
t
i m
m
2
1
Dark Newton fringe’s radius: mRλ
Rt
r m
m
2
Bright Newton fringe’s radius:
1st bright fringe m = 0
Central dark fringe,
m = 0
1st dark fringe m = 1
Dark
Bright
Contact edge
of G1 & G2
tm
tm+1
G1
G2
l
If index of refraction is
gradually increased
no any phase shift for
both reflected rays
interference conditions
are reversed.
5th dark fringe, m = 4
G1 & G2
tm
air
2. Thin film interference
Air wedge
2
1
2
2
Rλ
m
Rt
r m
m