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18PYB101J Module-III Lecture-1
DEPARTMENT OF PHYSICS AND NANOTECHNOLOGY
SRM INSTITUTE OF SCIENCE AND TECHNOLOGY
18PYB101J –Physics: Electromagnetic Theory, Quantum Mechanics, Waves
and Optics
1
DEPARTMENT OF PHYSICS AND NANOTECHNOLOGY
SRM INSTITUTE OF SCIENCE AND TECHNOLOGY
21PYB101J-Electromagnetic Theory, Quantum Mechanics, Waves
and Optics
Module 3- Lecture-I
Inadequacies of Classical Mechanics & Introduction to quantum mechanics,
Black body radiation and Concept of Photon
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18PYB101J Module-III Lecture-1
Topics to be Discussed:--
Inadequacies of Classical Mechanics & Introduction to quantum
mechanics
Particle nature of light
3
18PYB101J Module-III Lecture-1
Where classical mechanics(CM) fails and quantum
mechanics arises(QM)?
Experimental results could not be explained by classical
mechanics. It is taken as failures of CM
1.Black-Body radiation spectrum.
2.Photo-electric effect
3.Compton scattering.
4.Spectrum of hydrogen emissions
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18PYB101J Module-III Lecture-1
Black Body Radiations
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18PYB101J Module-III Lecture-1
Black Body Radiations
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18PYB101J Module-III Lecture-1
Any object with a temperature above absolute zero emits light at all wavelengths. If
the object is perfectly black (so it doesn't reflect any light), then the light that comes
from it is called blackbody radiation .
Some experimental facts about blackbody radiation:
a. The blackbody spectrum depends only on the temperature of the object, and not on
what it is made of. An iron horseshoe, a ceramic vase, and a piece of charcoal --- all
emit the same blackbody spectrum if their temperatures are the same.
b. As the temperature of an object increases, it emits more blackbody energy at all
wavelengths.
c. As the temperature of an object increases, the peak wavelength of the blackbody
spectrum becomes shorter (bluer). For example, blue stars are hotter than red stars.
d. The blackbody spectrum always becomes small at the left-hand side (the short
wavelength, high frequency side).
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18PYB101J Module-III Lecture-1
The explanation of classical physics: Light is an electromagnetic wave
that is produced when an electric charge vibrates. (Strictly speaking, "vibrates" means
any change in how the charge moves --- speeding up, slowing down, or changing
direction.) Now recall that heat is just the kinetic energy of random motion. In a hot
object, electrons vibrate in random directions and produce light as a result. A hotter
object means more energetic vibrations and so more light is emitted by a hotter object -
-- it glows brighter. So far, so good. But classical physics could not explain the shape of
the blackbody spectrum.
The electrons in a hot object can vibrate with a range of frequencies, ranging from very
few vibrations per second to a huge number of vibrations per second. In fact, there is
no limit to how great the frequency can be. Classical physics said that each frequency
of vibration should have the same energy. Since there is no limit to how great the
frequency can be, there is no limit to the energy of the vibrating electrons at high
frequencies. This means that, according to classical physics, there should be no limit to
the energy of the light produced by the electrons vibrating at high frequencies.
WRONG!! Experimentally, the blackbody spectrum always
becomes small at the left-hand side (short wavelength, high
frequency).
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18PYB101J Module-III Lecture-1
The Photoelectric Effect
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
When light shines on the surface of a metallic substance, electrons in the metal
absorb the energy of the light and they can escape from the metal's surface.
This is called the photoelectric effect, and it is used to produce the electric current
that runs many solar-powered devices. Using the idea that light is a wave with the
energy distributed evenly throughout the wave, classical physicists expected that
when using very dim light, it would take some time for enough light energy to build up
to eject an electron from a metallic surface. WRONG!! Experiments show that if light
of a certain frequency can eject electrons from a metal, it makes no difference how
dim the light is. There is never a time delay.
In 1905, Albert Einstein came up with the solution. If Max Planck's idea that energy
comes in clumps (quanta) is correct, then light must consist of a stream of clumps of
energy. Each clump of light energy is called a photon, said Einstein, and each photon
has an energy equal to hf (Planck's constant times the frequency of the light).
Therefore the energy of light is not evenly distributed along the wave, but is
concentrated in the photons. A dimmer light means fewer photons, but simply turning
down the light (without changing its frequency) does not alter the energy of an
individual photon. So for a specific frequency light, if a single photon has
enough energy to eject an electron from a metallic surface, then electrons will
always be ejected immediately after the light is turned on and the photons hit
the metal.
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
Compton scattering is DIRECT evidence of particle nature of light
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
The Hydrogen Atom
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18PYB101J Module-III Lecture-1
When a small tube of hydrogen gas is heated, it begins to glow and emit light.
Unlike the blackbody radiation that comes from a hot dense solid or gas, this light
consists of just a few colors (wavelengths): a red wavelength, a turquoise, and
several violets. Classical physicists at the beginning of the century thought they
should certainly be able to understand hydrogen, since it is the simplest atom.
Hydrogen consists of a positively charged proton at the center, with a negatively
charged electron orbiting around it. The electrical attraction between the positive
proton and the negative electron keeps the electron in orbit, just like the
gravitational attraction between the Sun and the Earth holds the Earth in orbit.
There was just one problem.
Classical physics said that because the orbiting electron is constantly
changing direction, it should emit electromagnetic radiation --- light. As a
result, the electron should be continually losing energy. In fact, physicists
calculated that the electron should lose all of its energy and spiral down
into the proton in only about 0.000000000001 second! In other words,
atoms should not exist longer than a mere 10-12 seconds. WRONG!!
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
Niels Bohr provided an explanation in 1913. In the Bohr model of
the hydrogen atom, the electron can't orbit the proton in any size
orbit it pleases. There are only certain allowed orbits, and each
allowed orbit has a certain radius and a certain energy. Bohr
invented a rule that allowed him to calculate the size and energy
of each orbit. If you are curious, Bohr's rule said that
2π x (electron mass) x (electron orbital speed) x (orbit radius) = (any integer) x h
which is not too obvious, to say the least! (The integer would be 1 for the
smallest orbit, 2 for the next orbit out, and so on.) Bohr also made up a
new rule to explain the stability of the hydrogen atom --- why it could last
longer than 0.000000000001 second. He said that when an electron is in
an allowed orbit, the electron will not produce electromagnetic radiation.
Bohr did not explain why, he just proposed a new law of nature. And
nature agreed with Niels Bohr. His new model of hydrogen gave
wavelengths for hydrogen gas that precisely agreed with what was
measured.
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18PYB101J Module-III Lecture-1
Young’s double-slit Experiment
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18PYB101J Module-III Lecture-1
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18PYB101J Module-III Lecture-1
Classical Physics could not explain phenomena such as interference
diffraction and polarization. It predicted that the velocity of light is more in
a denser medium than that in a rarer medium.
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18PYB101J Module-III Lecture-1
LIGHT---===WAVES OR PARTICLES? BOTH!
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18PYB101J Module-III Lecture-1
When light passes through a double-slit, an interference pattern consisting of bright
bands and dark bands is seen on a screen. This is produced when the wave from
one slit combines with the wave from the other slit. If two wave crests meet at the
screen, the waves add and you get a bright band. If a wave crest from one slit
meets a wave trough from the other slit, the waves cancel and you get a dark band.
This proves that light is a wave.
On the other hand, the photoelectric effect proves that light consists of massless
particles called photons.
So which is it? Is light a wave or a stream of particles? The answer is "Yes!"
Light acts like a wave if you want to know how it propagates, how it travels from
one place to another. To describe how light travels from the double slits to the
screen, you have to use the wave characteristics of light.
25
18PYB101J Module-III Lecture-1
Light acts like particles (photons) if you want to know how light interacts
with matter. To describer how light interacts with the electrons in a metal
and how it ejects them from the metal's surface, you have to use the
particle characteristics of light.
We say that light exhibits a wave-particle duality.
It can behave like either waves or particles (but
not both at the same time), depending on the
situation.[DUAL NATURE OF LIGHT]
Thinking about the photoelectric effect again, how can a photon (which
has no mass) knock an electron about? Einstein used his theory of
relativity to show that even massless photons have momentum. Newton
defined momentum = (mass) x (velocity) for a particle with mass, but
Einstein was able to show that the momentum of a massless photon
depends on its wavelength:
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
•A photon is an elementary particle. It is a quantum of light.
•Energy of a photon is given by E=hν. Its momentum is p=hν/c and speed is c, which is the
speed of light.
•Irrespective of the intensity of radiation, every photon of a frequency v has the same
momentum p=hν/c and energy E=hν.
•The increase in the intensity of light only increases the number of photons crossing an area
per unit time. It does not affect the energy of the radiation.
•A photon remains unaffected by electric and magnetic fields. It is electrically neutral.
•A photon has a zero mass, i.e. it is massless.
•It is a stable particle.
Concept of Photon:
31
18PYB101J Module-III Lecture-2
•Photons can be created or destroyed when radiation is emitted or absorbed.
•The total energy and momentum are conserved during a photon-electron collision.
•A photon cannot decay on its own.
•The energy of a photon can be transferred during an interaction with other particles.
•A photon is a spin-1 particle, unlike electrons which are ½ spin. It’s spin axis is parallel to the
direction of travel.
Concept of Photon:
32
18PYB101J Module-III Lecture-2
photoelectric effect
33
18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
Experimentally obtained RESULTS
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
photoelectric effect equation
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18PYB101J Module-III Lecture-2
Compton scattering
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-2
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18PYB101J Module-III Lecture-3
de-Broglie Concept of Dual Nature
The universe is made of Radiation (light) and matter (particles). The light exhibits the dual
nature (i.e.,) it can behaves both as a wave (Interference, diffraction phenomenon) and as a
particle (Compton effect, photo-electric effect etc).
Since the nature loves symmetry, in 1924 Louis de-Broglie suggested that an electron (or)
any other material particle must exhibit wave like properties in addition to particle nature.
The waves associated with a material particle are called as Matter waves.
48
18PYB101J Module-III Lecture-3
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18PYB101J Module-III Lecture-3
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18PYB101J Module-III Lecture-3
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18PYB101J Module-III Lecture-3
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18PYB101J Module-III Lecture-3
53
Heisenberg’s Uncertainty principle
54
55
56
57
18PYB101J Module-III Lecture-4
Work examplev 3.1 : A particle is dropped from height H, find
its de Broglie wavelength.
58
18PYB101J Module-III Lecture-4
Work example 3.2: Determine the de Broglie wavelength of an electron that
has been accelerate through a potential difference of 100 eV.
Solution:-
The energy gained by the electron = 100 eV
eV
m
p
100
2
2

Therefore,
  2
/
1
10
31
)
10
6
.
1
100
(
)
10
11
.
9
(
2 




 kg
p
Or,
= 5.399  10-24 kg ms
1
24
34
10
399
.
5
10
626
.
6








ms
kg
Js
p
h
=1.23  10-10 m = 1.23 A

59
18PYB101J Module-III Lecture-4
Please note that C1=8πhc
Please note that
C2=hc
Work example 3.3
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18PYB101J Module-III Lecture-4
Work example 3.4: In the Compton scattering the photon of wavelength 22 pm is
scattered at angle of 85 degree. Find the change wavelength and fractional loss of
energy of the photon.
61
18PYB101J Module-III Lecture-4
1. A particle of rest mass m0 has kinetic energy K which is not
negligible compared with moc2. Prove that the de-Broglie wavelength is
given by
 
2 2 2 4
0
E p c m c
 
2
( 2 )
o
hc
K m c



Hint: use
62
18PYB101J Module-III Lecture-4
2. A light with a frequency of 8.3 × 1014 Hz shines on calcium, which has a work
function of 2.9 eV. What is the maximum kinetic energy of an electron released due
to the photoelectric effect? Estimate h as 4.14 × 10-15 eVs.
We will use the equation KEmax = hf-ϕ. We plug in our known values and get
KEmax = (8.3 × 1014) (4.14 × 10-15) -2.9 = 0.54eV.
Hint:
63
18PYB101J Module-III Lecture-4
3. What is the de Broglie wavelength of a photon with a momentum 7.6 × 10-35
kg∙m/s? Estimate h as 6.63 × 10-34J s and keep 3 significant figures.
We can use the formula: λ = h/p.
In this case, we know that p = 7.6 × 10-35 kg∙m/s.
Thus, λ = (6.63 × 10-34) / (7.6 × 10-35) = 8.72 eV
Hint:
64
65
66
67
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18PYB101J Module-III Lecture-13
BORN INTERPRETATION OF WAVE FUNCTION:
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18PYB101J Module-III Lecture-13
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18PYB101J Module-III Lecture-13
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18PYB101J Module-III Lecture-13
Normalisation Condition

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  • 1. 18PYB101J Module-III Lecture-1 DEPARTMENT OF PHYSICS AND NANOTECHNOLOGY SRM INSTITUTE OF SCIENCE AND TECHNOLOGY 18PYB101J –Physics: Electromagnetic Theory, Quantum Mechanics, Waves and Optics 1 DEPARTMENT OF PHYSICS AND NANOTECHNOLOGY SRM INSTITUTE OF SCIENCE AND TECHNOLOGY 21PYB101J-Electromagnetic Theory, Quantum Mechanics, Waves and Optics Module 3- Lecture-I Inadequacies of Classical Mechanics & Introduction to quantum mechanics, Black body radiation and Concept of Photon
  • 2. 2 18PYB101J Module-III Lecture-1 Topics to be Discussed:-- Inadequacies of Classical Mechanics & Introduction to quantum mechanics Particle nature of light
  • 3. 3 18PYB101J Module-III Lecture-1 Where classical mechanics(CM) fails and quantum mechanics arises(QM)? Experimental results could not be explained by classical mechanics. It is taken as failures of CM 1.Black-Body radiation spectrum. 2.Photo-electric effect 3.Compton scattering. 4.Spectrum of hydrogen emissions
  • 6. 6 18PYB101J Module-III Lecture-1 Any object with a temperature above absolute zero emits light at all wavelengths. If the object is perfectly black (so it doesn't reflect any light), then the light that comes from it is called blackbody radiation . Some experimental facts about blackbody radiation: a. The blackbody spectrum depends only on the temperature of the object, and not on what it is made of. An iron horseshoe, a ceramic vase, and a piece of charcoal --- all emit the same blackbody spectrum if their temperatures are the same. b. As the temperature of an object increases, it emits more blackbody energy at all wavelengths. c. As the temperature of an object increases, the peak wavelength of the blackbody spectrum becomes shorter (bluer). For example, blue stars are hotter than red stars. d. The blackbody spectrum always becomes small at the left-hand side (the short wavelength, high frequency side).
  • 7. 7 18PYB101J Module-III Lecture-1 The explanation of classical physics: Light is an electromagnetic wave that is produced when an electric charge vibrates. (Strictly speaking, "vibrates" means any change in how the charge moves --- speeding up, slowing down, or changing direction.) Now recall that heat is just the kinetic energy of random motion. In a hot object, electrons vibrate in random directions and produce light as a result. A hotter object means more energetic vibrations and so more light is emitted by a hotter object - -- it glows brighter. So far, so good. But classical physics could not explain the shape of the blackbody spectrum. The electrons in a hot object can vibrate with a range of frequencies, ranging from very few vibrations per second to a huge number of vibrations per second. In fact, there is no limit to how great the frequency can be. Classical physics said that each frequency of vibration should have the same energy. Since there is no limit to how great the frequency can be, there is no limit to the energy of the vibrating electrons at high frequencies. This means that, according to classical physics, there should be no limit to the energy of the light produced by the electrons vibrating at high frequencies. WRONG!! Experimentally, the blackbody spectrum always becomes small at the left-hand side (short wavelength, high frequency).
  • 10. 10 18PYB101J Module-III Lecture-1 When light shines on the surface of a metallic substance, electrons in the metal absorb the energy of the light and they can escape from the metal's surface. This is called the photoelectric effect, and it is used to produce the electric current that runs many solar-powered devices. Using the idea that light is a wave with the energy distributed evenly throughout the wave, classical physicists expected that when using very dim light, it would take some time for enough light energy to build up to eject an electron from a metallic surface. WRONG!! Experiments show that if light of a certain frequency can eject electrons from a metal, it makes no difference how dim the light is. There is never a time delay. In 1905, Albert Einstein came up with the solution. If Max Planck's idea that energy comes in clumps (quanta) is correct, then light must consist of a stream of clumps of energy. Each clump of light energy is called a photon, said Einstein, and each photon has an energy equal to hf (Planck's constant times the frequency of the light). Therefore the energy of light is not evenly distributed along the wave, but is concentrated in the photons. A dimmer light means fewer photons, but simply turning down the light (without changing its frequency) does not alter the energy of an individual photon. So for a specific frequency light, if a single photon has enough energy to eject an electron from a metallic surface, then electrons will always be ejected immediately after the light is turned on and the photons hit the metal.
  • 12. 12 18PYB101J Module-III Lecture-1 Compton scattering is DIRECT evidence of particle nature of light
  • 17. 17 18PYB101J Module-III Lecture-1 When a small tube of hydrogen gas is heated, it begins to glow and emit light. Unlike the blackbody radiation that comes from a hot dense solid or gas, this light consists of just a few colors (wavelengths): a red wavelength, a turquoise, and several violets. Classical physicists at the beginning of the century thought they should certainly be able to understand hydrogen, since it is the simplest atom. Hydrogen consists of a positively charged proton at the center, with a negatively charged electron orbiting around it. The electrical attraction between the positive proton and the negative electron keeps the electron in orbit, just like the gravitational attraction between the Sun and the Earth holds the Earth in orbit. There was just one problem. Classical physics said that because the orbiting electron is constantly changing direction, it should emit electromagnetic radiation --- light. As a result, the electron should be continually losing energy. In fact, physicists calculated that the electron should lose all of its energy and spiral down into the proton in only about 0.000000000001 second! In other words, atoms should not exist longer than a mere 10-12 seconds. WRONG!!
  • 19. 19 18PYB101J Module-III Lecture-1 Niels Bohr provided an explanation in 1913. In the Bohr model of the hydrogen atom, the electron can't orbit the proton in any size orbit it pleases. There are only certain allowed orbits, and each allowed orbit has a certain radius and a certain energy. Bohr invented a rule that allowed him to calculate the size and energy of each orbit. If you are curious, Bohr's rule said that 2π x (electron mass) x (electron orbital speed) x (orbit radius) = (any integer) x h which is not too obvious, to say the least! (The integer would be 1 for the smallest orbit, 2 for the next orbit out, and so on.) Bohr also made up a new rule to explain the stability of the hydrogen atom --- why it could last longer than 0.000000000001 second. He said that when an electron is in an allowed orbit, the electron will not produce electromagnetic radiation. Bohr did not explain why, he just proposed a new law of nature. And nature agreed with Niels Bohr. His new model of hydrogen gave wavelengths for hydrogen gas that precisely agreed with what was measured.
  • 22. 22 18PYB101J Module-III Lecture-1 Classical Physics could not explain phenomena such as interference diffraction and polarization. It predicted that the velocity of light is more in a denser medium than that in a rarer medium.
  • 24. 24 18PYB101J Module-III Lecture-1 When light passes through a double-slit, an interference pattern consisting of bright bands and dark bands is seen on a screen. This is produced when the wave from one slit combines with the wave from the other slit. If two wave crests meet at the screen, the waves add and you get a bright band. If a wave crest from one slit meets a wave trough from the other slit, the waves cancel and you get a dark band. This proves that light is a wave. On the other hand, the photoelectric effect proves that light consists of massless particles called photons. So which is it? Is light a wave or a stream of particles? The answer is "Yes!" Light acts like a wave if you want to know how it propagates, how it travels from one place to another. To describe how light travels from the double slits to the screen, you have to use the wave characteristics of light.
  • 25. 25 18PYB101J Module-III Lecture-1 Light acts like particles (photons) if you want to know how light interacts with matter. To describer how light interacts with the electrons in a metal and how it ejects them from the metal's surface, you have to use the particle characteristics of light. We say that light exhibits a wave-particle duality. It can behave like either waves or particles (but not both at the same time), depending on the situation.[DUAL NATURE OF LIGHT] Thinking about the photoelectric effect again, how can a photon (which has no mass) knock an electron about? Einstein used his theory of relativity to show that even massless photons have momentum. Newton defined momentum = (mass) x (velocity) for a particle with mass, but Einstein was able to show that the momentum of a massless photon depends on its wavelength:
  • 30. 30 18PYB101J Module-III Lecture-2 •A photon is an elementary particle. It is a quantum of light. •Energy of a photon is given by E=hν. Its momentum is p=hν/c and speed is c, which is the speed of light. •Irrespective of the intensity of radiation, every photon of a frequency v has the same momentum p=hν/c and energy E=hν. •The increase in the intensity of light only increases the number of photons crossing an area per unit time. It does not affect the energy of the radiation. •A photon remains unaffected by electric and magnetic fields. It is electrically neutral. •A photon has a zero mass, i.e. it is massless. •It is a stable particle. Concept of Photon:
  • 31. 31 18PYB101J Module-III Lecture-2 •Photons can be created or destroyed when radiation is emitted or absorbed. •The total energy and momentum are conserved during a photon-electron collision. •A photon cannot decay on its own. •The energy of a photon can be transferred during an interaction with other particles. •A photon is a spin-1 particle, unlike electrons which are ½ spin. It’s spin axis is parallel to the direction of travel. Concept of Photon:
  • 47. 47 18PYB101J Module-III Lecture-3 de-Broglie Concept of Dual Nature The universe is made of Radiation (light) and matter (particles). The light exhibits the dual nature (i.e.,) it can behaves both as a wave (Interference, diffraction phenomenon) and as a particle (Compton effect, photo-electric effect etc). Since the nature loves symmetry, in 1924 Louis de-Broglie suggested that an electron (or) any other material particle must exhibit wave like properties in addition to particle nature. The waves associated with a material particle are called as Matter waves.
  • 54. 54
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  • 57. 57 18PYB101J Module-III Lecture-4 Work examplev 3.1 : A particle is dropped from height H, find its de Broglie wavelength.
  • 58. 58 18PYB101J Module-III Lecture-4 Work example 3.2: Determine the de Broglie wavelength of an electron that has been accelerate through a potential difference of 100 eV. Solution:- The energy gained by the electron = 100 eV eV m p 100 2 2  Therefore,   2 / 1 10 31 ) 10 6 . 1 100 ( ) 10 11 . 9 ( 2       kg p Or, = 5.399  10-24 kg ms 1 24 34 10 399 . 5 10 626 . 6         ms kg Js p h =1.23  10-10 m = 1.23 A 
  • 59. 59 18PYB101J Module-III Lecture-4 Please note that C1=8πhc Please note that C2=hc Work example 3.3
  • 60. 60 18PYB101J Module-III Lecture-4 Work example 3.4: In the Compton scattering the photon of wavelength 22 pm is scattered at angle of 85 degree. Find the change wavelength and fractional loss of energy of the photon.
  • 61. 61 18PYB101J Module-III Lecture-4 1. A particle of rest mass m0 has kinetic energy K which is not negligible compared with moc2. Prove that the de-Broglie wavelength is given by   2 2 2 4 0 E p c m c   2 ( 2 ) o hc K m c    Hint: use
  • 62. 62 18PYB101J Module-III Lecture-4 2. A light with a frequency of 8.3 × 1014 Hz shines on calcium, which has a work function of 2.9 eV. What is the maximum kinetic energy of an electron released due to the photoelectric effect? Estimate h as 4.14 × 10-15 eVs. We will use the equation KEmax = hf-ϕ. We plug in our known values and get KEmax = (8.3 × 1014) (4.14 × 10-15) -2.9 = 0.54eV. Hint:
  • 63. 63 18PYB101J Module-III Lecture-4 3. What is the de Broglie wavelength of a photon with a momentum 7.6 × 10-35 kg∙m/s? Estimate h as 6.63 × 10-34J s and keep 3 significant figures. We can use the formula: λ = h/p. In this case, we know that p = 7.6 × 10-35 kg∙m/s. Thus, λ = (6.63 × 10-34) / (7.6 × 10-35) = 8.72 eV Hint:
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  • 68. 68 18PYB101J Module-III Lecture-13 BORN INTERPRETATION OF WAVE FUNCTION:

Editor's Notes

  1. Black Body Radiation Curve Obtained by Kirchoff
  2. Threshold Frequency is intimately related to Particle Nature of Light
  3. Spiral Path of Electron
  4. Young Slit Double Slit Experiment
  5. Philips Leonard had done experiment to measure photo-current
  6. Q 3.2: A particle is dropped from height H, find its de Broglie wavelength.
  7. In the Compton scattering the photon of wavelength 22 pm is scattered at angle of 85 degree. Find the change wavelength and fractional loss of energy of the phtotn
  8. Hint: use