Wave front
During the propagation of the wave, all the particles of the medium which are located at the same distance from the source receive the disturbance simultaneously and vibrate in the same phase. Thus, a wave front of light at any instance is the locus of all particles of the medium vibrating in the same phase at that time. The shape of wave front depends on the nature of source and the disturbance of the wave front from the source. That is wave front. Wave front is the disturbance of the point source. Wave front formed by the locus of the real source. Wave fronts are of three types:
a. Spherical wave front
b. Cylindrical wave front
c. Plane wave front.
Huygens principle
Huygens’s principle states that:
a. Each point on the primary wave front acts as a source of secondary wave lets, sending out disturbance in all direction in a similar manner as the original source of the light does.
b. The new position of the wave front at any instant is given by the forward envelope of the secondary wavelets at that instant.
Consider a point source of light. Let XY be the section of the spherical wave front at any time t. supposed we are interested in finding the new position of the wave front at time t+∆t. to do so, a number of points a,b,c,d are the point taken on the primary wave front. These point acts as the source of secondary wavelets. In time ∆t light will travel a distance c∆t. taking the point a,b,c,d,…as the centre of sphere each of radius c∆t are drawn. The forward enveloped X’Y’ of these spheres give the position of wave front at ∆t +t and called secondary wave front.
Figure.
Laws of reflection on the basis of wave theory
Let us consider a plane wave front PQ incident on the reflecting surface AB at an angle of incidence i as shown in figure.
The I1, I2, I3 incident ray on the wave front PQ which are also perpendicular to the wave the wave front PQ. NP is normal to the reflecting surface AB. Point P of the wave front reaches the reflecting surface at time t=0. By the time , point Q, of the wave front reaches at point P’(t=t), the secondary wavelets from P spread out in the form of sphere having radius PQ’=QP’=ct, where c is the velocity of the light .now draw the tangent to the sphere from P’ point then P’Q’ become reflected wave front. Similarly, the wavelets from R reach point S and from S reach to the point T of the reflected wave front in the time t. reflected rays after strike the reflecting surface must be at right angle to the wave front P’Q’. in figure reflected rays are represented by I’1, I’2, I’3.
Now draw P’N’ normal to the reflecting surfaceAB. Then∠Q’P’P=r, where r is the angle of reflection. From figure we have right angle triangle PQP’ and PQ’P’, we have
PQ’=PA’
∠PQ’P’= ∠PQP’ = 90° and
PP’ is the common. Therefore the two triangles are congruent.
So, ∠QPP’=∠Q’P’P therefore i=r
This shows that the angle of incident is equal to the angle of reflection which is the first law of reflection.
Laws of refraction on the basis of wave theory
The laws of refraction are:
The ratio of the sine of the angle of the incidence to the sine angle of the refraction is constant for any two medium.
Sini/sinr=μ
which is the refractive index of medium in a air
The incident rays, refracted rays and the normal at the point of incident on the refracting surface lie on the same plane. These laws can be verified as:
Here each point of the wave front AB acts as secondary wavelets.
Figure
If t is time taken by the secondary wavelets to reach at time point C from B then BC=ct. In the same, time wave front originating from A has traveled a distance of vt =AD in denser medium
Similarly wave front from P reaches at Q. if we draw the sphere of radius AD=vt with tangent to the sphere CD emanating from points A and C then CD is the new wave front in denser medium.
Let us draw NA normal to the surface XY
Then ACD = r
In rt angled triangle ABC
Sini=BC/AC=ct/AC …………..1
Sinr = AD/CD =vt/AC ……….2
From 1 and 2
sini/sinr = c/v =μ which proves the Snell’s law
Further the incident ray refracted ray and the normal to the surface of incident all lie on the same plane. This verifies the laws of refraction.
Foucault’s method for the determination of speed of light
The experimental arrangement of Foucault’s method are given below
Experimental arrangement:
The rays of light from a bright source S are allowed to fall on convex lens L, which will bring them to focus at point I in the absence of plane mirror XY, which is capable of rotation about an axis through the point Q. The plane mirror make the ray to meet at point P, the pole of the concave mirror M such that PQ=IQ=d say. When the plane mirror is stationary, the rays of the light after reflection from concave mirror retrace their path and finally image coincident with S if the glass plate is placed at 450to the optical axis of the lens, then the returning light is reflected from it so as to produce the image I’( instead the image coincident with S)
Theory
When the plane mirror is rotated about its axis though the point Q,the intermittent image of the source is seen through the eyepiece. It is because the light falls on the concave mirror for a small fraction of revolution. As the speed of revolution is increased slowly, a stage comes, when image is seen continuously due to persistence of vision. It happens when mirror is rotated at the speed of more than 10r.p.s. as the distance between the plane mirror and the concave mirror is very small, negligible is compared to the velocity of light therefore , the light returning to the plane mirror ( after the reflection from the concave mirror)will find it practically in the same position . As a result, when plane mirror is rotating at low speed, the image will be seen still at I’
Now, suppose the speed of rotation of the plane mirror is increased. The light reflected from the plane mirror in the position XY, on returning from the concave mirror will find it in position X’Y’ i.e. displaced through, say angle ɵ the reflected ray will turn through angle 2ɵ . To the eye, the rays will appear to diverge from I and the image will be seen to shift to position I”. The displacement II’’ can be measure with the micrometer attached to the eyepiece.
Let C be the velocity of the light d be the distance between the plane mirror and concave mirror and n be the no. of revolutions made per second by the rotating mirror.
The time taken by the light to cover distance 2d i.e. from Q to P and back to Q is given by
T=2d/c…………………….1
As the plane mirror make n rotation per second. It covers an angle 2∏n in one second. Therefore, time taken by the mirror to rotate thought angle ɵ is given by
T=ɵ/2∏n………………2
From 1 and 2 we get
C=4∏nd/ɵ…………………3
To find ɵ
Let a and b be the distance of the plane mirror and the source of the light from the optical centre of the convex lens.
Now angle between two reflected rays QI and QI’ is 2ɵ therefore
2ɵ=II’/d
Or, II’=2ɵd……………….4
The image S and S’ formed by the lens are the images of I and I’
From the relation
Size of image/size of object=distance of image/ distance of object
Then we have, SS’/II’=OS/OI…………5
Where OS=b and OI=a+d
Now SS’=I’I”
Let the displacement I’I” in the image be x then, SS’=x
Then from equation 5 we have
x/II’=
b/a+d
or, II’=
(a+d)x/b.........6
From 4 and6 we have
ɵ=(a+d)x/(2bd)........7
on putting the value of ɵ in equation in 3 we get
C = 8Ï€nbd2/(a+d)x
This equation gives the speed of light in term of speed rotation. According to the Newton’s corpuscular, the velocity of the light in water should be greater than air. By using the Foucault method, It was found that s’/s is greater i.e. the velocity of light in water is smaller than velocity of light in air. Also the ratio of c/c’ c’ being speed of light in water, equal to the refractive index supporting the wave theory of light.
The advantages of Foucault’s method are:
a. It can be performed in laboratory as it covers the small area.
b. Speed of the light in any optical medium can be determined.
c. It justified the validity of wave theory of light as velocity of light in water found to be less than velocity of light in air.
The disadvantages of Foucault’s method are:
a. The image obtained is very faint due to reflection and refraction of light at various surfaces thus makes the observation difficult.
b. Due to small displacement of the image accurate measurement cannot be obtained.
Velocity of Light: Michelsons's Method
Michelsons's Method is a precise method for measuring the speed of light. An octagonal mirror M1 is mounted on the shaft of a variable speed motor. Light from a bright source S is focused at an angle of 45o on one of the faces of mirror M1 after passing through a slit S1. The reflected light falls on a distant concave mirror M2. In figure, M3 is a plane mirror and with the help of this mirror M3 placed at the center of curvature of mirror M2 the beam of light is returned back and falls on face 3 of the octagonal mirror M1 again at an angle of 45o. The light reflected by this face is then collected by a telescope T and the eye of the telescope.
If the mirror M1 is rotated, the light returning to it from the mirror M2 will not be incident at an angle of 45o, and hence will not enter the telescope. When the speed of rotation of the mirror M1 is so adjusted that the face 2 of mirror occupies exactly the same position as was occupied by face 3 earlier (in 1/8th revolution, of mirror M1) during hte time light travels from M1 to M2 and back to M1, then the image of source will reappear.
Fig - Michealson's method for the determination of velocity of light
If d be the distance between the mirror M1 and M2 and c be the speed of light, then the time taken by the light to travel from M1 to M2 and back to M1 is
t=2d/c
If f is the number of revolutions per seconds of mirror M1 and m is the number of faces of this mirror, then the angle rotated by the mirror during the time t is
Now,
The speed of rotation of mirror M1 can be measured by using stroboscope. In Michelson's original experiment, the speed of the motor was about 500 rev/s and d was about 35 km. he obtained a value of 2.99775 x 108 ms-1 for speed of light in vacuum.
The modern methods of measuring speed of light use coherent laser beams and radar signals and give results with high degree of accuracy. The most probable value for the speed of light in free space is c = 2.99792458 x 108 ms-1 .
The advantages of Michelson’s method are:
The distance between the two stations is very large.
Images obtained are very bright so that position can be determined accurately.
There is no measurement of the displacement of image.
The disadvantages are:
It is very difficult to maintain the high speed rotation of mirror.
High speed of the rotation of the mirror can break the mirror.
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