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Four major domains of physics
Classical
mechanics
Quantum
mechanics
Relativistic
mechanics
Quantum
field theory
Much larger
than 10-10 m
Of the order of
10-10 m or smaller
Much less
than 3 x 10 8 m/s
Of the order of
3 x 10 8 m/s
Quantum Mechanics
(The physics of the microscopic world)
1.Introduction to Quantum Mechanics, by D. J. Griffiths
2.Introduction to Quantum Mechanics, by C. W. Sherwin
3.Quantum Mechanics: An Introduction, by W. Greiner
4.The Feynman Lectures on Physics, Volume III
5.Lecture Notes and Problems Bank, by R. S. Saraswat
and G. P. Sastry,
6. Physics I: Oscillations and Waves, by S. Bharadwaj
and S. P. Khastgir,
References:
3
Evolution in Mechanics
@Citizendium
Classical concept
Two distinct categories :
1. Material body (particle)
Newton’s laws of motion
2. Electromagnetic field (wave)
Maxwell’s equation
Additionally
Laws of thermodynamics
Fundamental constants :
1. velocity of light c
2. Avogadro Number N
3. Boltzman constant k
4. Unit of charge e
Position and velocity (momentum) are
precisely measurable
Spread over the space, amplitude gives
energy/intensity, frequency is nothing
but time periodicity of oscillator
E = kT
E = mc2
Velocity << c : non-relativistic
Velocity comparable to c : relativistic
Classical concepts never allow to think that
1. Wave may also behave like particle.
(Planck’s hypothesis)
2. Particle may behave like wave.
(de Broglie hypothesis)
3. Position and momentum of a particle cannot
be measured accurately simultaneously.
(Heisenberg uncertainty principle)
4. Energy of wave is related with frequency
and quantised.
These new concepts are basically quantum concepts
Wave‐particle duality
Dr. T. K. Nath
Is light consists of particles or waves?
Interference, Diffraction Phenomena
proves wave nature of light
EARLY 19TH CENTURY
Dr. T. K. Nath
Planck’s theory of Black body radiation (1900)
Photoelectric effect by Einstein (1904)
Compton effect by Compton (1920)
Dr. T. K. Nath
•Theory of Black body radiation (Planck 1900)
•Photoelectric effect (Einstein 1905)
•Atomic Structure and Spectroscopy (Bohr 1913)
•Compton effect (Compton 1920)
Failures of Classical Physics
The Experimental Basis of Quantum Mechanics
lies in the
Quantum Mechanics – A New Interpretation of Nature
Birthday
of
Quantum Physics
on
14th December, 1900
On this date German physicist Max
Planck first presented his new
quantum concepts.
Max Karl Ernst Ludwig Planck
1858-1947

h
E 
Planck introduces a new
fundamental constant h
to explain black-body radiation
Experiments
1. Photoelectric effect
(1921, Einstein) (eV)
2. Compton effect
(1927, Compton) (k eV)
3. Pair Production
(1948, Patrick Blackett)(M eV)
Waves behaving as particles Particles behaving as waves
Electron diffraction
Davisson –Germer (USA)
and Thompson (UK) (1927)
Electron microscope
Experiments
Quantum Physics
Dual Nature
Black Body radiation
Frank Hertz Expt
Discrete energy level Concept of Spin
Stern Gerlach Expt
https://mmpant.com/2020/04/09/quantum‐mechanics‐in‐everyday‐life/
Timeline for the evolution/understanding of quantum phenomenon
Experiments on blackbody radiation Photoelectric effect
Franck Hertz experiment Davission Germer experiment
Stern Gerlach experiment
……
Theoretical development : Schrodinger’s and Heisenberg’s picture
High energy physics
Quantum optics
Statistical physics
Biophysics
Condensed matter physics
An ideal black body is an empty cavity whose walls are maintained
at a given temperature T (at thermodynamic equilibrium)
BLACKBODY RADIATION
The mother of Quantum Physics
Any object with a temperature above absolute zero emits
electromagnetic radiation at all wavelengths. If the object is
perfectly black (so it doesn't reflect any light), then the radiation
that comes from it is called blackbody radiation.
1. Blackbody Radiation
Blackbody:
Which absorbs all the radiation .
Total energy = absorbed+ reflected+ transmitted;
Eg: Two body are very close to BB;
Lamp black; a=0.96; and
Platinum black, a=0.98
Radiation:
Irreversible flow of energy away from the source, the energy per unit time
is transported out to infinity and never comes back.
A charge at rest or a steady current does NOT generate EM wave
Accelerating charge (changing current ) produces EM wave
Thermal Radiation from the Human Body:
The radiation is in the infrared region of the spectrum close to 7-15 m.
So, the thermal imaging device for human are most sensitive in this
range. eq: scanner placed at the airport during checking.
0 0.5 1 1.5 2 2.5 3 3.5 4
[Hz] 1014
0
0.5
1
1.5
2
2.5
3
3.5
4
4.5
5
10-17
1,peak
2,peak
3,peak
T
1
= 1000 K
T
2
= 1400 K
T
3
= 1800 K
One of the main
challenges was to
explain the
spectrum of
blackbody
radiation from
classical
concepts
Observed spectral density of the black body radiation
vs. frequency at different temperature
Blackbody Radiation
T=1000 K
T=1400 K
T=1800 K
ρ(υ)
(J/m3-Hz)
Energy density
in the window
υ and υ +d υ
frequency υ
h :Planck’s constant
= 6.63 x 10-34 J-s
k=:Boltzmann’s const.
= 1.38 x 10-23 J/K
= R/N
BLACKBODY RADIATION
Dr. T. K. Nath
BLACKBODY RADIATION
The mother of Quantum Physics
According to classical electrodynamics
such a cavity has infinite number of
normal modes. There is no upper limit to
the frequency of these normal modes
As there is no upper limit to the frequency
of these normal modes, there would be
infinite number of normal modes, and thus
infinite amount of energy residing in the
EM radiation within the cavity at a finite
temperature.
Ultraviolet catastrophe
Classical theory of Rayleigh-Jeans law
The amount of energy per unit volume per unit frequency interval (Spectral
density) should increase with frequency as 2. (Obeyed well at low frequencies)
T=1800 K
T=1400 K
T=1000 K
T=1800 K
frequency υ
ρ(υ)
ρ(υ)
frequency υ
T=1800 K
υ dependence
2
Simple assumption that the radiators (walls) are simple harmonic
oscillators. As classical physics predicted from the law of equipartition
energy theorem, that average energy of the oscillators is kBT ,
then the spectral energy density
= no. of standing wave modes in the cavity in the frequency range
 and +d × average energy of the oscillators (radiation field)
×
Classical theory of Rayleigh-Jeans
Ultraviolet catastrophe !!!
Rayleigh-Jeans law
Planck’s law
ρ(υ)
frequency υ
Rayleigh-Jeans law
(Classical theory)
T=1800 K
T=1400 K
T=1000 K
T=1800 K
frequency υ
ρ(υ)
2 dependence
T=1800 K

h
E 
Quantum energy of photon
h= Planck’s constant
=6.626x10-34 Jsec
: frequency of radiation
Max Karl Ernst Ludwig Planck
1858-1947
Dr. T. K. Nath
Planck’s Radiation Law
5
8 1
( , )
1
hc
kT
hc
E T
e



 

The density of radiant energy in the cavity per unit
wavelength interval, at the wavelength , and at the
temperature T
Dr. T. K. Nath
Planck’s postulate
Any physical entity with one degree of freedom and whose ``co-ordinate” is
oscillating sinusoidally with frequency  can possess only total energies E as
integral multiple of h.
E = 0
2
4
Classical
h = Planck’s constant
Planck's law of black body radiation (1900)
Planck’s assumption (1900):
Radiation of a given frequency ν
could only be emitted and
absorbed in “quanta” (discrete
bundles) of energy
h =6.626x10-34 J-sec
(Planck’s constant)
: frequency of radiation
E=hν
Planck’s Formula
Rayleigh-Jeans law
Large
>>
 ‐
In the high frequency region
it falls down exponentially with increasing
frequency, again in agreement with
the black body radiation data
0 0.5 1 1.5 2 2.5 3 3.5 4
[Hz] 10
14
0
0.5
1
1.5
2
2.5
3
3.5
4
4.5
5
10
-17
1,peak
2,peak
3,peak
T
1
= 1000 K
T
2
= 1400 K
T
3
= 1800 K
High frequency region in the BBR:
Low frequency region in the BBR
)
10
9
.
2
(
, 3
max K
m
b
T 


 

Experiments
1. Photoelectric effect (1902)
2. Compton effect (1922)
3. Pair Production
Waves behaving as particles
Quantum Physics
Albert Einstein
(1879-1955)
Photoelectric Effect
in 1905
Dr. T. K. Nath
Photoelectric effect
Dr. T. K. Nath

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tkn_Lec_26 (1).pdf

  • 1. Four major domains of physics Classical mechanics Quantum mechanics Relativistic mechanics Quantum field theory Much larger than 10-10 m Of the order of 10-10 m or smaller Much less than 3 x 10 8 m/s Of the order of 3 x 10 8 m/s
  • 2. Quantum Mechanics (The physics of the microscopic world) 1.Introduction to Quantum Mechanics, by D. J. Griffiths 2.Introduction to Quantum Mechanics, by C. W. Sherwin 3.Quantum Mechanics: An Introduction, by W. Greiner 4.The Feynman Lectures on Physics, Volume III 5.Lecture Notes and Problems Bank, by R. S. Saraswat and G. P. Sastry, 6. Physics I: Oscillations and Waves, by S. Bharadwaj and S. P. Khastgir, References:
  • 4. Classical concept Two distinct categories : 1. Material body (particle) Newton’s laws of motion 2. Electromagnetic field (wave) Maxwell’s equation Additionally Laws of thermodynamics Fundamental constants : 1. velocity of light c 2. Avogadro Number N 3. Boltzman constant k 4. Unit of charge e Position and velocity (momentum) are precisely measurable Spread over the space, amplitude gives energy/intensity, frequency is nothing but time periodicity of oscillator E = kT E = mc2 Velocity << c : non-relativistic Velocity comparable to c : relativistic
  • 5. Classical concepts never allow to think that 1. Wave may also behave like particle. (Planck’s hypothesis) 2. Particle may behave like wave. (de Broglie hypothesis) 3. Position and momentum of a particle cannot be measured accurately simultaneously. (Heisenberg uncertainty principle) 4. Energy of wave is related with frequency and quantised. These new concepts are basically quantum concepts
  • 6. Wave‐particle duality Dr. T. K. Nath Is light consists of particles or waves? Interference, Diffraction Phenomena proves wave nature of light
  • 8. Planck’s theory of Black body radiation (1900) Photoelectric effect by Einstein (1904) Compton effect by Compton (1920) Dr. T. K. Nath
  • 9. •Theory of Black body radiation (Planck 1900) •Photoelectric effect (Einstein 1905) •Atomic Structure and Spectroscopy (Bohr 1913) •Compton effect (Compton 1920) Failures of Classical Physics The Experimental Basis of Quantum Mechanics lies in the Quantum Mechanics – A New Interpretation of Nature
  • 10. Birthday of Quantum Physics on 14th December, 1900 On this date German physicist Max Planck first presented his new quantum concepts. Max Karl Ernst Ludwig Planck 1858-1947  h E  Planck introduces a new fundamental constant h to explain black-body radiation
  • 11. Experiments 1. Photoelectric effect (1921, Einstein) (eV) 2. Compton effect (1927, Compton) (k eV) 3. Pair Production (1948, Patrick Blackett)(M eV) Waves behaving as particles Particles behaving as waves Electron diffraction Davisson –Germer (USA) and Thompson (UK) (1927) Electron microscope Experiments Quantum Physics Dual Nature Black Body radiation Frank Hertz Expt Discrete energy level Concept of Spin Stern Gerlach Expt https://mmpant.com/2020/04/09/quantum‐mechanics‐in‐everyday‐life/
  • 12. Timeline for the evolution/understanding of quantum phenomenon Experiments on blackbody radiation Photoelectric effect Franck Hertz experiment Davission Germer experiment Stern Gerlach experiment …… Theoretical development : Schrodinger’s and Heisenberg’s picture High energy physics Quantum optics Statistical physics Biophysics Condensed matter physics
  • 13. An ideal black body is an empty cavity whose walls are maintained at a given temperature T (at thermodynamic equilibrium) BLACKBODY RADIATION The mother of Quantum Physics
  • 14. Any object with a temperature above absolute zero emits electromagnetic radiation at all wavelengths. If the object is perfectly black (so it doesn't reflect any light), then the radiation that comes from it is called blackbody radiation. 1. Blackbody Radiation
  • 15. Blackbody: Which absorbs all the radiation . Total energy = absorbed+ reflected+ transmitted; Eg: Two body are very close to BB; Lamp black; a=0.96; and Platinum black, a=0.98 Radiation: Irreversible flow of energy away from the source, the energy per unit time is transported out to infinity and never comes back. A charge at rest or a steady current does NOT generate EM wave Accelerating charge (changing current ) produces EM wave Thermal Radiation from the Human Body: The radiation is in the infrared region of the spectrum close to 7-15 m. So, the thermal imaging device for human are most sensitive in this range. eq: scanner placed at the airport during checking.
  • 16. 0 0.5 1 1.5 2 2.5 3 3.5 4 [Hz] 1014 0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 10-17 1,peak 2,peak 3,peak T 1 = 1000 K T 2 = 1400 K T 3 = 1800 K One of the main challenges was to explain the spectrum of blackbody radiation from classical concepts Observed spectral density of the black body radiation vs. frequency at different temperature
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  • 18. Blackbody Radiation T=1000 K T=1400 K T=1800 K ρ(υ) (J/m3-Hz) Energy density in the window υ and υ +d υ frequency υ h :Planck’s constant = 6.63 x 10-34 J-s k=:Boltzmann’s const. = 1.38 x 10-23 J/K = R/N
  • 20. BLACKBODY RADIATION The mother of Quantum Physics According to classical electrodynamics such a cavity has infinite number of normal modes. There is no upper limit to the frequency of these normal modes As there is no upper limit to the frequency of these normal modes, there would be infinite number of normal modes, and thus infinite amount of energy residing in the EM radiation within the cavity at a finite temperature. Ultraviolet catastrophe
  • 21. Classical theory of Rayleigh-Jeans law The amount of energy per unit volume per unit frequency interval (Spectral density) should increase with frequency as 2. (Obeyed well at low frequencies) T=1800 K T=1400 K T=1000 K T=1800 K frequency υ ρ(υ)
  • 23. Simple assumption that the radiators (walls) are simple harmonic oscillators. As classical physics predicted from the law of equipartition energy theorem, that average energy of the oscillators is kBT , then the spectral energy density = no. of standing wave modes in the cavity in the frequency range  and +d × average energy of the oscillators (radiation field) × Classical theory of Rayleigh-Jeans
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  • 27. Rayleigh-Jeans law (Classical theory) T=1800 K T=1400 K T=1000 K T=1800 K frequency υ ρ(υ) 2 dependence T=1800 K
  • 28.  h E  Quantum energy of photon h= Planck’s constant =6.626x10-34 Jsec : frequency of radiation Max Karl Ernst Ludwig Planck 1858-1947 Dr. T. K. Nath
  • 29. Planck’s Radiation Law 5 8 1 ( , ) 1 hc kT hc E T e       The density of radiant energy in the cavity per unit wavelength interval, at the wavelength , and at the temperature T Dr. T. K. Nath
  • 30. Planck’s postulate Any physical entity with one degree of freedom and whose ``co-ordinate” is oscillating sinusoidally with frequency  can possess only total energies E as integral multiple of h. E = 0 2 4 Classical h = Planck’s constant
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  • 37. Planck's law of black body radiation (1900) Planck’s assumption (1900): Radiation of a given frequency ν could only be emitted and absorbed in “quanta” (discrete bundles) of energy h =6.626x10-34 J-sec (Planck’s constant) : frequency of radiation E=hν
  • 39. Large >>  ‐ In the high frequency region it falls down exponentially with increasing frequency, again in agreement with the black body radiation data 0 0.5 1 1.5 2 2.5 3 3.5 4 [Hz] 10 14 0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 10 -17 1,peak 2,peak 3,peak T 1 = 1000 K T 2 = 1400 K T 3 = 1800 K
  • 40. High frequency region in the BBR: Low frequency region in the BBR ) 10 9 . 2 ( , 3 max K m b T      
  • 41. Experiments 1. Photoelectric effect (1902) 2. Compton effect (1922) 3. Pair Production Waves behaving as particles Quantum Physics