lecture 5 - nptel · lecture – 5 title: electromagnetic radiation – matter interactions page-1...
TRANSCRIPT
Lecture – 5
TITLE: Electromagnetic Radiation – Matter Interactions
Page-1
Objectives
In the previous lecture, we have learnt that the radiation or light is following
the Wave-Particle dual nature
It can be treated as electromagnetic wave or particle nature like photon
Similarly, the electrons can also be treated as particle and also as wave
corresponding to its momentum for describing the stable structure of atom.
When both of them interact with each other, we have to understand the
mechanism to follow for describing the experimental observations such as Compton
effect, absorption and emission of light by atoms.
In this lecture, the different kinds of treatment to understand the light-matter
interactions are described. We will start with the classical phenomenon and then proceed
to understand the quantum mechanical descriptions.
Page – 2
Classical treatment:
In classical theory as shown in Figure – 5.1, we model the atom as a heavy nucleus
with electron attached to it with spring the binding force between them.
The resonant frequency for this system is 0
If we treat the light as wave then the electric field can be represented as
0E E Sin t
Equation – 5.1
Figure – 5.1
The oscillating electric field will force the electron to oscillate. The displacement of
electron with respect to nucleus will produce an oscillating dipole.
It is known that an oscillating dipole emit electromagnetic radiation with the same
frequency of vibration. This emission of light is known as scattering of light by matter.
However, if the incident radiation frequency matches with the resonant frequency of
the system ( 0 ) then the resonance occurs. Energy transfer takes place.
The oscillating dipole ( ) ( )p t e x t
Equation – 5.2
Where e is the charge of the electron and x(t) is the time dependent displacement of
electron with respect to nucleus.
When this dipole oscillates, it emits radiation. As time passes by, due to the radiation loss
the emission dies or decays. This phenomenon can be modeled as a damping oscillator
whose solution will be x(t).
The differential equation of motion of the damping oscillator with damping constant
2
0( ) ( ) ( ) 0x t x t x t
Equation – 5.3
Where 2
0k
m , here k is the force constant of the spring.
+
t t
E E
Page – 3
With the initial values i.e. at t = 0
the displacement 0(0)x x and the velocity (0) 0x , the solution is
( )
20( ) [ ( ) ]
2t
x t x e Cos t Sin t
Equation – 5.4
The frequency 2
12 20( )
4
of the damped oscillation is slightly lower than the
frequency 0 of the undamped case.
Taking 0 , we get ( )
20 0( )
tx t x e Cos t
.
Equation – 5.5
Line profile of the emitted radiation
The damped oscillation ( )x t can be described as a superposition of monochromatic
oscillations with slightly different frequencies and amplitude ( )A
1( ) ( )
2
i tx t A e d
Equation – 5.6
The amplitude ( )A can be calculated by 1
( ) ( )2
i tA x t e dt
Equation – 5.7
The intensity
*
0 0 2 2
0
1( ) ( ) ( )
( ) ( / 2)I A A I
Equation – 5.8
Figure – 5.2
I(-0)
0
x0
t
e-(/2)/t
Page-4
Momentum of a Photon
Momentum vector magnitude E
pc
E is the energy.
E hp h
c c
parallel to the direction of propagation.
From relativity, we know that 2
0
2
2
2
1
E m c
p mV
mm
Vc
Ep mV V
c
Equation – 5.9
Minkowski’s four dimensional space & time ( E & three comp. of p)
If the system is confined to a single particle so, 2 2 2E p c is invariant under changes of
ref. frame. 2 2 2
2 22 2 2 2
4 2
22 42
2 42 2 40
022
2
1
1
1
1
E p c
E VE V c E
c c
Vm cc
m c V m ccV
c
Equation – 5.10
Photon is a quantity of energy. If we consider photon as a particle, then the energy 2E mc , with this infinite energy E .
So the only way of reconciling a speed V c with a finite energy is to assume rest mass
0 0m .
So, 2 2 2 0 ; EE p c pc
Rest energy 20 0m c for photon
So, 20. .K E E m c E so for photon all energy is K.E.
Page-5
Elastic Collisions of Photons – Compton Effect
The X-ray of wavelength 0 was incident on a target. With a crystal diffractometer, the
wavelengths of the scattered X-ray were measured by changing the angle as shown in
Figure – 5.3.
Figure – 5.3
Scattered radiation is composed by two lines:
(i) a component at the incident wavelength 0 , called the Thomson
component. Scattered radiation has the same frequency as the
incident radiation.
(ii) a component of different wavelength 0 .
Conclusion from experiment
(i) 0 is always positive.
(ii) is an increasing function of .
(iii) is independent of and the composition of the material used for
scattering.
X-Ray
source
Scatter
(electron)
Incident
beam
Scattered
beam
Crystal
(wavelength
selector)
Scattering
angle ()
Collimating
system
Detector
Page-6
Explanation
Elastic scattering between photons and free electrons (weakly bound to atoms can be
considered as free electrons) i.e. binding energy 0h .
Elastic Scattering K.E. is conserved
Figure – 5.4
We have taken into account the fact that p & E are related by relativistic invariance 2 2 2 2 4
0E p c m c .
Before Collision After Collision
Photon Energy 0
0
ch h
ch h
Momentum 0
0
hhc
along Oz hh
c
Electron
Energy 20m c
2
2 2 2 40
mc
p c m c
Momentum = Zero p making an angle with OZ
Photon
Momentum = 0hc
Energy 0E h
Electron
Z
X
O
Page-7
Conservation of energy and momentum
Energy 2 2 2 2 40 0 0h m c h p c m c
Equation – 5.11
Momentum
0 cos cos
0 sin sin
h halong OZ p
c c
halong OX p
c
0
0
cos cos
cos
sin sin
h hp
c c
h
c
hp
c
Equation – 5.12
Figure – 5.5
Photon
Momentum = 0hc
Energy 0E h
Electron
Z
Page-8
2 222 2 2
02 2
22 2 2 2 20 02
22 20 02
2 2 2 2 20 0
cos cos
cos 2 cos sin
2 cos
2 cos
h hp
c c
h
c
h
c
p c h
Equation – 5.13
From 1st equation
22 2 2 2 4
0 0 0p c h m c m c
Equation – 5.14
Equating Equation – 5.13 & Equation – 5.14,
22 2 2 2 2 4
0 0 0 0 0
22 2 40 0
2 cosh h m c m c
h m c
2 2 40 0 02h m c m c
2 20h 2 2h 2 2 2
0 02 cosh h 2 2h
2 20 0 0
2 20 0 0
0
2 2
2 2 1 cos
2
h h m c
h m c h
2h
2h
020
31002
0 0 0
20 0
00
0 0
0
1 cos
1 cos where 9.1 10
1 11 cos
1 cos
0 ; 0
21 cos ;
90 ;o
m c
hm Kg
m c
h
m c
h
m c
h h
m c m c
hCompton wavelength
m c
Page-9
So, we get
00
1 cosh
m c
Equation – 5.15
(i) is positive.
(ii) independent of 0 .
(iii) depends on only.
Hard X-ray 1
1
pm
h MeV
Energy of Compton Wavelength,
20
0
rest massof theelectronhc hc
m ch
m c
20 0 0 0h m c photons gives up very little energy.
20 0 0 0h m c photons gives up most of its energy.
Equation – 5.16
Page-10
Absorption of Photons (Inelastic Collision)
Let us define 12h is the energy difference between the two states of an atom with energy
2E and 1E ( 2 1E E ground state) 2 1 12E E h .
If there is a collision between an atom and a photon as shown in Figure – 5.6 and after the
collision they form one particle, then the initial momentum of the incident must be
preserved by the final single particle (momentum conservation). Or we can say that after
collision the atom must possess some kinetic energy that it did not have previously.
This kinetic energy can have been taken from the energy of the incident photon.
This is possible only when 12h h . We have to determine the relationship between
and 12 .
Figure – 5.6
Considering the properties of the relativistic particles:
Before Collision After Collision
Photon
Energy h
Momentum hc
Atom
Energy
2
1 1
1 rest mass
E m e
m
2 2 2 4
2W P c m e
Momentum Zero
2 1 122 2 2
where,
P
E E hm
c c
Photon
Momentum = hc
Energy E h
Atom
Atom - photon
system
E1
E2
Page-11
From the conservation of energy
2 2 2 4
1 2h E P c m e
Equation – 5.17
same as photonhMomentum pc
Equation – 5.18
2
1 12 2E h m c
From Equation – 5.17,
2 2 2 2 4
1 2
22 2 2 2 2
1 1 1 12
2 22 2 2 2
1 1 12 122
2 2
12 1 12 1212
1 1 12 1
1212 2
1
2
2
21 1
2 2 2
12
E h p c m c
E E h h p c E h
hc E E h h
c
h E h h
E h E h E
h
m c
Equation – 5.19
Page-12
So the incident photon frequency must be greater than the theoretical frequency of the
spectral lines 2 112
E E
h
.
12 10
2
1
1 1010
10 100
h to eV
m c to GeV
Comment:
(i) In the optical transitions 2
12 1h m c typically, 1012
2
1
~ 10h
m c
which means the shift
will be very small compared to other broadening 610 cannot be observed. Resonant
condition is applicable i.e. 2 1E E h .
(ii) When 12h is not very small compared to 2
1m c , the shift is appreciable.
Page-13
Emission of Photons:
Before Collision After Collision
Photon
Energy ~ h
Momentum ~ hc
along Oz
Atom
Energy 2E 2 2 2 4
1W P c m c
Momentum 2
22
0
Em
c
p along Oz
2 12121 2
E hEm
c c
2 2 2 2
2
2
2 2 2 2 2 2 4
2 2 1
2 2 2 4
1
22 2 4
2 2 1 2 12
2 2 2 2
2 2 2 12 2 12
2 2
2 2 12 12
2 2 2
2 12 12 1212
2 2 2
1212 2
2
0
2
2
2 2
2 2
2
2 2 2
12
hp p c h
c
E W h
E h W
E h h E p c m c
h m c
E h E m c E h
E h E E h E h
h E E h h
E h h h
hE E h E
h
m c
Equation – 5.20
Page-14
Application to rays
19 22
rays Very High Energy
10 to 10 Hz
Nuclear transitions also very high frequency 2
12 1h m c
Emission of ray photon is interpreted as the radiative transition between two energy
states of the nucleus (analogous to optical transition).
Frequency Displacement Line Width
Figure – 5.7
Resonance absorption and emission is not possible as in the case of optical transition. By
increasing temperature it is possible. So to get the information about the nucleus from
this is difficult.
What Mössbaur discovered that by cooling the source and the absorber the intensity
absorption increased.
It means that, below a certain temperature emitted or absorbing nucleus is embedded in a
crystalline lattice and it is the white crystal which recoils. 23~ 6 10Mass of Crystal Mass of Nucleus
The velocity of recoil is negligible.
No recoil energy loss extremely sharp lines (natural width) could be obtained.
2 2
0 3exp
2
where, . .
' .
.
Debye Waller Factor
E Tf
K
T Abs Temp
K Boltzmann s Const
Degree Temp of the Solid
Equation – 5.21
There are three main hyperfine interactions that can be observed by Mössbauer
spectroscopy. They are (i) Isomer Shift, (ii) Quadrupole Splitting and (iii) Nuclear
Zeeman Splitting.
For example :
The isomer shift of 57 3 1 14.42 2
Fe KeV in Ferricinium bromide is 82 10 eV .
8
0
3
0
0
0
810
3
0
2
3
2 10
14.4 10
2 103 10
14.4 10
6 100.04
14.4 10
h h eV
h eV
c
c v
v v
c v c
v c
cms
Mössbaur Spectrum of Ferricinium bromide
Figure – 5.8
Recap
In this lecture, we came to know that the classical physics has limitation to describe the
several experimental observations such as Compton effect and absorption and emission
of light by atoms.
We understood the different kinds of treatment for describing the light-matter
interactions: both the classical phenomenon and then the quantum mechanical
descriptions.
We also come to know the recoil energy required when both light and matter interact.
Based on this, we came to know the application of this recoil energy in Mossbaur
spectroscopy.