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Unit 1
Quantum Mechanics
Basics of Quantum Mechanics
Why Quantum Physics?
The three theories, namely Newtonian mechanics, thermodynamics
and Maxwell's electromagnetic theory together constitute the classical
physics.
The classical physics is based on:
1) The physical quantities can take any value.
2. An object can be isolated from its environment and treated as an
2. An object can be isolated from its environment and treated as an
independent quantity for the investigation.
Classical mechanics (Newton's mechanics) and Maxwell's equations
(electromagnetics theory) can explain MACROSCOPIC phenomena
such as motion of billiard balls or rockets.
Basics of Quantum Mechanics
There are a few phenomena which classical mechanics failed to explain
such as Stability of atom, spectral series of hydrogen atom (line
spectra), black body radiation, photoelectric effect etc.
Failures of Classical mechanics led to the Need of Quantum
mechanics
Quantum mechanics is used to explain microscopic phenomena such
as photon-atom scattering and flow of the electrons in a
semiconductor.
QUANTUM MECHANICS is a collection of postulates based on a huge
number of experimental observations.
Basics of Quantum Mechanics
1) According to Planck's hypothesis in 1900, the radiating body consists
of an enormous number of atomic oscillators vibrating at all possible
frequencies and that each oscillator emits or absorb energy in discrete
portions.
2) This discrete portions cannot be further subdivided.
Einstein extended Planck’s hypothesis.
. An electromagnetic wave having a frequency ν contains
. An electromagnetic wave having a frequency ν contains
identical photons, each photon having an energy h ν
Photoelectric effect:
h ν = K.E + W
K.E = h ν –W
In 1921 A. Einstein received Nobel Prize
De BROGLIE HYPOTHESIS
Light can exhibit both kind of nature of waves and particles so the
light shows wave particle duality nature.
In some cases like interference ,diffraction and polarization it
behaves as a wave while in other cases like photoelectric effect and
Compton effect it behaves as a particle (photon)
Not only light but every materialistic particle such as electron,
proton or even heavier object exhibits wave particle duality nature.
De Broglie proposed that a moving particle whatever its nature has
waves associated with it these waves are called matter waves.
De BROGLIE HYPOTHESIS
De BROGLIE HYPOTHESIS
De BROGLIE HYPOTHESIS
Properties of matter waves
Properties of matter waves
Properties of matter waves
Properties of matter waves
Problems
Problems
Obtain an expression for the de Broglie wavelength associated with
an electron accelerated through V volts. Also find the wavelength for
100v and 54V
Solution: The k.E. Acquired by the electron accelerated through V
volts is
(½)mv2 = eV
mv2 = 2eV
m2v2=2meV
m2v2=2meV
mv= 2meV or p = 2meV ------(1)
= h/p or  = h/2meV (h= 6.625 x 10-34 J-s, m=9.1 x 10-31kg,
e= 1.6 x 10-19 C
Using all these values  = (12.27 /V) AU
For v=100V ,  = 1.227 AU
For v=54V  = 1.67AU
Problems
Problems
Calculate the de Broglie wavelength of an electron moving with
speed 1/10 th of the velocity of light.
m = 9.1 x 10-31kg, h= 6.625 x 10-34 J-s, c = 3x108m/s
V = c/10 = 3 x 107 m/s
P = mv = 2.73 x 10-23kg-m/s
= h/p = 2.43 x 10-11 m
 = 0.243 AU
Find the De broglie wavelength of neutron whose K.E. is 1eV.
Given: mass of neutron = 1.676 x 10-27kg
k.E. of neutron = 1ev
k.E. of neutron = 1 x 1.6 x 10-19 J
(½) mv2 = 1.6 x 10-19 J
V2 = (2 x 1.6 x 10-19 J) / m = 1.9093 x 108
V = 1.38 x 104m/s
 = h / mv = 0.286AU
Physical Significance of Wave Function and Probability Density
Interpretation
 We know there is a wave associated with a moving particle and the
motion of a particle is guided by the wave group.
 The mathematical function which describes wave group is the wave
function ψ.
 As the particle moves under the action of external forces the wave
function changes with time.
Thus, the variable quantity characterizing the De Broglie
wave is called as wave function and it is denoted by the
Thus, the variable quantity characterizing the De Broglie
wave is called as wave function and it is denoted by the
symbol ψ ( x,y,z,t ).
 ψ describes the wave as a function of position and time.
 The wave function usually contains all the information which
the uncertainty principle allows us to know about the associated
particle. But the wave function ψ itself has no physical interpretation,
as it may be positive, negative or complex.
Physical Significance of Wave Function and Probability Density Interpretation
 ψ has no direct physical significance, as it is not an observable
quantity. In general, ψ is a complex-valued function.
 According to Heisenberg uncertainty principle, we can only know the
probable value in a measurement.
 The probability cannot be negative. Hence ψ cannot be a measure of
the presence of the particle at the location (x, y, z).
 This difficulty is solved by taking IψI2 = ψ ψ*. This quantity is called
probability density.
probability density.
 The product of ψ and its complex conjugate is having physical
significance and it represents the probability of finding the particle in a
volume dxdydz.
 A probability interpretation of the wave function was given by Max
Born in 1926.
 He suggested that the square of the magnitude of the wave
function |ψ|2 evaluated in a particular region represents the
probability of finding the particle in that region.
Physical Significance of Wave Function and Probability Density
Interpretation
Probability, P, of finding the particle in an infinitesimal volume dV (=
dx dy dz) is proportional to |ψ (x, y, z)|2 dx dy dz at time t.
|ψ|2 is called the probability density and ψ is the probability
amplitude.
Since the particle is certainly somewhere in the space, the probability
Since the particle is certainly somewhere in the space, the probability
P = 1 and the integral of |ψ|2dV over the entire space must be equal
to unity. That is
The wave function ψ is in general a complex function. But the
probability must be real.
Physical Significance of Wave Function and Probability Density
Interpretation
Therefore to make probability a real quantity, ψ is to be multiplied by
its complex conjugate ψ*
Thus, ψ has no physical significance but |ψ|2 gives the probability of
finding the particle in a particular region..
finding the particle in a particular region..
The above condition on ψ is known as normalisation condition. the
wave function that satisfies above condition is called normalised wave
function.
Physical Significance of Wave Function and Probability Density
Interpretation
How to normalise a wave function?
If the wave function is not normalised in order to normalise the wave
function it is multiplied by some arbitrary constant and then the
integral is evaluated over the entire space.
The normalisation procedure is as follows:
If ψ is not normalised wave function then multiply it by some constant
A. Then evaluate the integral and equate it to unity and calculate the
A. Then evaluate the integral and equate it to unity and calculate the
constant A called normalisation constant i.e.
∫ A ψ (A ψ)* dV = 1
Or AA*∫ ψ ψ* dV = 1
As A is real constant, we get
IAI2∫ ψ ψ* dV = 1
This gives normalisation constant as
IAI2 = 1 / (∫ψ ψ* dV )
The normalisation constant can be positive square root of above
equation.
Requirements of wave function
Requirements of wave function
Conditions to be satisfied by ψ – function
1) ψ function must be finite: The wave function must be finite
everywhere.
It must remain finite for all values of x, y, z. If ψ is infinite, it would
imply an infinitely large probability of finding the particle at that point.
Not finite at x=a
Requirements of wave function
Requirements of wave function
2) ψ function must be single–valued: The function
related to a physical quantity cannot have more than one value
at that point. If it has more than one value at a point,it means
that there is more than one value of probability of finding the
particle at that point.
Not single valued
Requirements of wave function
Requirements of wave function
3) ψ function must be continuous: ψ function should be
continuous across any boundary. Since ψ is related to a
physical quantity, it cannot have a discontinuity at any point.
Therefore, the wave function ψ and its space derivatives should
be continuous across any boundary. Since ψ is related to a real
particle, it cannot have a discontinuity at any boundary where
potential changes.
Discontinuous at x=a
Well-behaved Wave Functions
4) ψ function must be normalised:
Well behaved wave function
Schrodingers time dependent wave equation
Schrodingers time dependent wave equation
.
Schrodingers time dependent wave equation
.
Schrodingers time dependent wave equation
.
Schrodingers time dependent wave equation
Schrodingers time independent wave equation
.
.
Schrodingers time independent wave equation
.
Schrodingers time independent wave equation
.
Schrodingers time independent wave equation
Operators in quantum mechanics
Operators in quantum mechanics
.
Operators in quantum mechanics
Operators in quantum mechanics
.
Eigen Functions and Eigen Values
Eigen Functions and Eigen Values
.
Expectations Values
Expectations Values
.
Problems
Problems
.
.
.
.
Numericals
Numericals
.
Numericals
Numericals
.
Problem : A wave function of the free particle in the range -∞ to +∞ is given by
ψ = A e –αx2/2
Motion of a free particle
Motion of a free particle
Suppose the particle is moving with constant potential i.e
V(x) = constant.
Then the force acting on the particle F = -dV/dx = 0
Because force is called as negative gradient of potential.
Thus the particle is free particle so to predict the quantum mechanical
behaviour of a free particle, we have to solve the schrodingers time
independent wave equation
Motion of a free particle
Motion of a free particle
.
The solution of equation 4.2 are eigen functions. The possible solutions of equation
4.2 are e-ikx and eikx
The solution of the time part is given by
 (t) = e-iEt/ħ Since we have E = ħω
There fore  (t) = e-iωt
The wave function is
Ψ (x,t) = ψ (x)  (t)
Ψ (x,t) = eikx e-iωt = ei(kx-ωt) --------4.3
Ψ (x,t) = e-ikx e-iωt = e-i(kx+ωt) --------4.4
Equation 4.3 represents wave propagating along +x direction and
Equation 4.4 represents wave propagating along –ve x direction
Motion of a free particle
Motion of a free particle
. Let us consider equation 4.3 and Let A is the normalization constant
Ψ (x,t) = A ei(kx-ωt)
Ψ* (x,t) = A* e -i(kx-ωt)
Ψ Ψ* = A A* = ei(kx-ωt) e -i(kx-ωt)
Ψ Ψ* = A A* = Constant ( This probability density)
There is difficulty in the normalisation of free partcile wave function. According to
There is difficulty in the normalisation of free partcile wave function. According to
normalisation condition
A A* [x] ∞ =1
-∞
A A* ∞ = 1
A A* is the amplitude of the wave. There fore the probability of finding the particle
will be very small everywhere.
Particle in an infinite deep potential well (Rigid box)
Particle in an infinite deep potential well (Rigid box)
.
A partcile moving under the influence of infinite square well potential is often
called a particle in one dimensional rigid box
Particle in an infinite deep potential well (Rigid box)
Particle in an infinite deep potential well (Rigid box)
.
The general solution of this equation may be written as
Particle in an infinite deep potential well (Rigid box)
Particle in an infinite deep potential well (Rigid box)
.
.
.
Particle in a finite deep potential well (Non rigid box)
Particle in a finite deep potential well (Non rigid box)
.
If the particle has total energy E < V0, Then according to classical
mechanics particle may be in the region II only ( - a < x < a ). Because in
the region I and III the momentum P = (2m(E-V0) will be imaginary and
it is not possible. Thus the particle is permanently in the region II with
momentum of constant magnitude P = (2mE). If E > V0 then only
particle can go in the region I and III
Particle in a finite deep potential well (Non rigid box
Particle in a finite deep potential well (Non rigid box
.
Particle in a finite deep potential well (Non rigid box
Particle in a finite deep potential well (Non rigid box
.
Numericals
Numericals
.
.
Numericals
Numericals
.
1 ) An electron is trapped in a rigid box of width 1 Å. Find its lowest
energy level and momentum. Hence find energy of 5th level.
As P= ħk= (h/2π)x(nπ/L) and n= 1  P= h/2L
Numericals
Numericals
.2) Lowest energy of an electron trapped in a infinite potential well is
38 electron Volt. Calculate the width of the well.
Numericals
Numericals
. 3) A small object of mass 1 g is confined to move between two rigid
walls separated by a distance of 1mm.
(a) Calculate the minimum speed of the object
(b) If the speed is 3 x108 m/s, find the corresponding value of n.
Sol: (a)
Numericals
Numericals
.
Numericals
Numericals
.
4) Determine the probability that a particle trapped in a rigid box of length
L can be found between 0.45L and 0.55L for ground and first excited
state.
Given : ψ = (2/L) ( sin(nπx/L) )
Numericals
Numericals
. 5) Ruby laser emits light of wavelength 693.4 nm. If the light is due to
transition from n=2 to n=1 state of an electron in one dimensional
rigid box, find the width of the box.
Numerical
Numerical
.
.
Numerical
Numerical
.
Numerical
Numerical
.
Numerical
Numerical
.
Numerical
Numerical
.
Numerical
Numerical
.
Numerical
Numerical
.

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Unit 1 Quantum Mechanics_230924_162445.pdf

  • 2. Basics of Quantum Mechanics Why Quantum Physics? The three theories, namely Newtonian mechanics, thermodynamics and Maxwell's electromagnetic theory together constitute the classical physics. The classical physics is based on: 1) The physical quantities can take any value. 2. An object can be isolated from its environment and treated as an 2. An object can be isolated from its environment and treated as an independent quantity for the investigation. Classical mechanics (Newton's mechanics) and Maxwell's equations (electromagnetics theory) can explain MACROSCOPIC phenomena such as motion of billiard balls or rockets.
  • 3. Basics of Quantum Mechanics There are a few phenomena which classical mechanics failed to explain such as Stability of atom, spectral series of hydrogen atom (line spectra), black body radiation, photoelectric effect etc. Failures of Classical mechanics led to the Need of Quantum mechanics Quantum mechanics is used to explain microscopic phenomena such as photon-atom scattering and flow of the electrons in a semiconductor. QUANTUM MECHANICS is a collection of postulates based on a huge number of experimental observations.
  • 4. Basics of Quantum Mechanics 1) According to Planck's hypothesis in 1900, the radiating body consists of an enormous number of atomic oscillators vibrating at all possible frequencies and that each oscillator emits or absorb energy in discrete portions. 2) This discrete portions cannot be further subdivided. Einstein extended Planck’s hypothesis. . An electromagnetic wave having a frequency ν contains . An electromagnetic wave having a frequency ν contains identical photons, each photon having an energy h ν Photoelectric effect: h ν = K.E + W K.E = h ν –W In 1921 A. Einstein received Nobel Prize
  • 5. De BROGLIE HYPOTHESIS Light can exhibit both kind of nature of waves and particles so the light shows wave particle duality nature. In some cases like interference ,diffraction and polarization it behaves as a wave while in other cases like photoelectric effect and Compton effect it behaves as a particle (photon) Not only light but every materialistic particle such as electron, proton or even heavier object exhibits wave particle duality nature. De Broglie proposed that a moving particle whatever its nature has waves associated with it these waves are called matter waves.
  • 9. Properties of matter waves Properties of matter waves
  • 10. Properties of matter waves Properties of matter waves
  • 11. Problems Problems Obtain an expression for the de Broglie wavelength associated with an electron accelerated through V volts. Also find the wavelength for 100v and 54V Solution: The k.E. Acquired by the electron accelerated through V volts is (½)mv2 = eV mv2 = 2eV m2v2=2meV m2v2=2meV mv= 2meV or p = 2meV ------(1) = h/p or  = h/2meV (h= 6.625 x 10-34 J-s, m=9.1 x 10-31kg, e= 1.6 x 10-19 C Using all these values  = (12.27 /V) AU For v=100V ,  = 1.227 AU For v=54V  = 1.67AU
  • 12. Problems Problems Calculate the de Broglie wavelength of an electron moving with speed 1/10 th of the velocity of light. m = 9.1 x 10-31kg, h= 6.625 x 10-34 J-s, c = 3x108m/s V = c/10 = 3 x 107 m/s P = mv = 2.73 x 10-23kg-m/s = h/p = 2.43 x 10-11 m  = 0.243 AU
  • 13. Find the De broglie wavelength of neutron whose K.E. is 1eV. Given: mass of neutron = 1.676 x 10-27kg k.E. of neutron = 1ev k.E. of neutron = 1 x 1.6 x 10-19 J (½) mv2 = 1.6 x 10-19 J V2 = (2 x 1.6 x 10-19 J) / m = 1.9093 x 108 V = 1.38 x 104m/s  = h / mv = 0.286AU
  • 14. Physical Significance of Wave Function and Probability Density Interpretation  We know there is a wave associated with a moving particle and the motion of a particle is guided by the wave group.  The mathematical function which describes wave group is the wave function ψ.  As the particle moves under the action of external forces the wave function changes with time. Thus, the variable quantity characterizing the De Broglie wave is called as wave function and it is denoted by the Thus, the variable quantity characterizing the De Broglie wave is called as wave function and it is denoted by the symbol ψ ( x,y,z,t ).  ψ describes the wave as a function of position and time.  The wave function usually contains all the information which the uncertainty principle allows us to know about the associated particle. But the wave function ψ itself has no physical interpretation, as it may be positive, negative or complex.
  • 15. Physical Significance of Wave Function and Probability Density Interpretation  ψ has no direct physical significance, as it is not an observable quantity. In general, ψ is a complex-valued function.  According to Heisenberg uncertainty principle, we can only know the probable value in a measurement.  The probability cannot be negative. Hence ψ cannot be a measure of the presence of the particle at the location (x, y, z).  This difficulty is solved by taking IψI2 = ψ ψ*. This quantity is called probability density. probability density.  The product of ψ and its complex conjugate is having physical significance and it represents the probability of finding the particle in a volume dxdydz.  A probability interpretation of the wave function was given by Max Born in 1926.  He suggested that the square of the magnitude of the wave function |ψ|2 evaluated in a particular region represents the probability of finding the particle in that region.
  • 16. Physical Significance of Wave Function and Probability Density Interpretation Probability, P, of finding the particle in an infinitesimal volume dV (= dx dy dz) is proportional to |ψ (x, y, z)|2 dx dy dz at time t. |ψ|2 is called the probability density and ψ is the probability amplitude. Since the particle is certainly somewhere in the space, the probability Since the particle is certainly somewhere in the space, the probability P = 1 and the integral of |ψ|2dV over the entire space must be equal to unity. That is The wave function ψ is in general a complex function. But the probability must be real.
  • 17. Physical Significance of Wave Function and Probability Density Interpretation Therefore to make probability a real quantity, ψ is to be multiplied by its complex conjugate ψ* Thus, ψ has no physical significance but |ψ|2 gives the probability of finding the particle in a particular region.. finding the particle in a particular region.. The above condition on ψ is known as normalisation condition. the wave function that satisfies above condition is called normalised wave function.
  • 18. Physical Significance of Wave Function and Probability Density Interpretation How to normalise a wave function? If the wave function is not normalised in order to normalise the wave function it is multiplied by some arbitrary constant and then the integral is evaluated over the entire space. The normalisation procedure is as follows: If ψ is not normalised wave function then multiply it by some constant A. Then evaluate the integral and equate it to unity and calculate the A. Then evaluate the integral and equate it to unity and calculate the constant A called normalisation constant i.e. ∫ A ψ (A ψ)* dV = 1 Or AA*∫ ψ ψ* dV = 1 As A is real constant, we get IAI2∫ ψ ψ* dV = 1 This gives normalisation constant as IAI2 = 1 / (∫ψ ψ* dV ) The normalisation constant can be positive square root of above equation.
  • 19. Requirements of wave function Requirements of wave function Conditions to be satisfied by ψ – function 1) ψ function must be finite: The wave function must be finite everywhere. It must remain finite for all values of x, y, z. If ψ is infinite, it would imply an infinitely large probability of finding the particle at that point. Not finite at x=a
  • 20. Requirements of wave function Requirements of wave function 2) ψ function must be single–valued: The function related to a physical quantity cannot have more than one value at that point. If it has more than one value at a point,it means that there is more than one value of probability of finding the particle at that point. Not single valued
  • 21. Requirements of wave function Requirements of wave function 3) ψ function must be continuous: ψ function should be continuous across any boundary. Since ψ is related to a physical quantity, it cannot have a discontinuity at any point. Therefore, the wave function ψ and its space derivatives should be continuous across any boundary. Since ψ is related to a real particle, it cannot have a discontinuity at any boundary where potential changes. Discontinuous at x=a
  • 22. Well-behaved Wave Functions 4) ψ function must be normalised: Well behaved wave function
  • 28. Schrodingers time independent wave equation .
  • 32. Operators in quantum mechanics Operators in quantum mechanics .
  • 33. Operators in quantum mechanics Operators in quantum mechanics .
  • 34. Eigen Functions and Eigen Values Eigen Functions and Eigen Values .
  • 37. .
  • 38. .
  • 39. .
  • 40.
  • 42. Numericals Numericals . Problem : A wave function of the free particle in the range -∞ to +∞ is given by ψ = A e –αx2/2
  • 43. Motion of a free particle Motion of a free particle Suppose the particle is moving with constant potential i.e V(x) = constant. Then the force acting on the particle F = -dV/dx = 0 Because force is called as negative gradient of potential. Thus the particle is free particle so to predict the quantum mechanical behaviour of a free particle, we have to solve the schrodingers time independent wave equation
  • 44. Motion of a free particle Motion of a free particle . The solution of equation 4.2 are eigen functions. The possible solutions of equation 4.2 are e-ikx and eikx The solution of the time part is given by  (t) = e-iEt/ħ Since we have E = ħω There fore  (t) = e-iωt The wave function is Ψ (x,t) = ψ (x)  (t) Ψ (x,t) = eikx e-iωt = ei(kx-ωt) --------4.3 Ψ (x,t) = e-ikx e-iωt = e-i(kx+ωt) --------4.4 Equation 4.3 represents wave propagating along +x direction and Equation 4.4 represents wave propagating along –ve x direction
  • 45. Motion of a free particle Motion of a free particle . Let us consider equation 4.3 and Let A is the normalization constant Ψ (x,t) = A ei(kx-ωt) Ψ* (x,t) = A* e -i(kx-ωt) Ψ Ψ* = A A* = ei(kx-ωt) e -i(kx-ωt) Ψ Ψ* = A A* = Constant ( This probability density) There is difficulty in the normalisation of free partcile wave function. According to There is difficulty in the normalisation of free partcile wave function. According to normalisation condition A A* [x] ∞ =1 -∞ A A* ∞ = 1 A A* is the amplitude of the wave. There fore the probability of finding the particle will be very small everywhere.
  • 46. Particle in an infinite deep potential well (Rigid box) Particle in an infinite deep potential well (Rigid box) . A partcile moving under the influence of infinite square well potential is often called a particle in one dimensional rigid box
  • 47. Particle in an infinite deep potential well (Rigid box) Particle in an infinite deep potential well (Rigid box) . The general solution of this equation may be written as
  • 48. Particle in an infinite deep potential well (Rigid box) Particle in an infinite deep potential well (Rigid box) .
  • 49. .
  • 50. .
  • 51. Particle in a finite deep potential well (Non rigid box) Particle in a finite deep potential well (Non rigid box) . If the particle has total energy E < V0, Then according to classical mechanics particle may be in the region II only ( - a < x < a ). Because in the region I and III the momentum P = (2m(E-V0) will be imaginary and it is not possible. Thus the particle is permanently in the region II with momentum of constant magnitude P = (2mE). If E > V0 then only particle can go in the region I and III
  • 52. Particle in a finite deep potential well (Non rigid box Particle in a finite deep potential well (Non rigid box .
  • 53. Particle in a finite deep potential well (Non rigid box Particle in a finite deep potential well (Non rigid box .
  • 55. .
  • 56. Numericals Numericals . 1 ) An electron is trapped in a rigid box of width 1 Å. Find its lowest energy level and momentum. Hence find energy of 5th level. As P= ħk= (h/2π)x(nπ/L) and n= 1  P= h/2L
  • 57. Numericals Numericals .2) Lowest energy of an electron trapped in a infinite potential well is 38 electron Volt. Calculate the width of the well.
  • 58. Numericals Numericals . 3) A small object of mass 1 g is confined to move between two rigid walls separated by a distance of 1mm. (a) Calculate the minimum speed of the object (b) If the speed is 3 x108 m/s, find the corresponding value of n. Sol: (a)
  • 60. Numericals Numericals . 4) Determine the probability that a particle trapped in a rigid box of length L can be found between 0.45L and 0.55L for ground and first excited state. Given : ψ = (2/L) ( sin(nπx/L) )
  • 61.
  • 62. Numericals Numericals . 5) Ruby laser emits light of wavelength 693.4 nm. If the light is due to transition from n=2 to n=1 state of an electron in one dimensional rigid box, find the width of the box.
  • 70. .