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Dr. Y. S. THAKARE
M.Sc. (CHE) Ph D, NET, SET
Assistant Professor in Chemistry,
Shri Shivaji Science College, Amravati
Email: yogitathakare_2007@rediffmail.com
B Sc- III Year
SEM-V
PAPER-III
PHYSICAL CHEMISTRY
UNIT- V and VI
Introduction to syllabus
Photochemistry
Electromagnetic radiation
Parameters of electromagnetic radiation
29-August -20 1
Unit V
Photochemistry
Introduction, Electromagnetic radiation, parameters of
electromagnetic radiation, spectrum of electromagnetic
radiation, problems, Interaction of radiation with matter, types
of chemical reaction- thermal reaction and photochemical
reaction, laws of absorption of light- Lambert law and beers
law, problems, laws of photochemistry- Grotthus Draper law
and stark Einstein's law of photochemical equivalence,
Quantum yield, experimental arrangement, reasons for high
and low Quantum yield, problems, photochemical reactions,
kinetics of photochemical decomposition of HI,
photosensitized reaction, mechanism of photosensitization,
Joblonski diagram, chemiluminescence, bioluminescence,
problems.
Electrode – The metal rod dipped in its salt solution29 -August -20 Dr. Yogita Sahebrao Thakare 2
Unit VI
Molecular spectroscopy
Molecular spectroscopy, electromagnetic radiation, parameters of
electromagnetic radiation, spectrum of electromagnetic radiation,
problems, types of spectra, degree of freedom, energy level
diagram, rotational spectroscopy, expression for moment of inertia
for diatomic rigid rotator, rotational quantum number, origin of line
in rotational spectrum, isotopic effect, applications of rotational
spectra for microwave spectroscopy, problems, Vibrational
spectroscopy, condition for IR active diatomic molecule,
expression for vibrational energy of diatomic molecule considering
it as a simple harmonic oscillator, zero point energy, relationship
between vibrational frequency and force constant, problems
Raman spectroscopy, characteristics of Raman spectrum, origin of
stokes and antistokes line in Raman spectrum, rotational Raman
spectrum vibrational Raman spectrum, problems
29 -August -20 Dr. Yogita Sahebrao Thakare
Unit V
Photochemistry
Photochemistry : Branch of chemistry which deals with the study of chemical
reactions that proceed with the absorption of light by atoms or molecules.
Example: photosynthesis, the degradation of plastics and the formation of vitamin D
with sunlight.
Principles
Light is a type of electromagnetic radiation, a source of energy. The
Grotthuss- Draper law states that light must be absorbed by a chemical substance in
order for a photochemical reaction to take place. According Stark-Einstein law in
primary photochemical reaction each molecule of reacting substance absorbs one
quantum of radiation which leads to photochemical change. For each photon of light
absorbed by a chemical system, no more than one molecule is activated for a
photochemical reaction.
29-August -20 Dr. Yogita Sahebrao Thakare
OR
Photochemistry deals with the study of photochemical reactions.
The photochemical reactions are caused by the absorption of light
radiations (photons) from visible and ultra violet regions (200-800nm).
The photons supply the necessary energy to the reactants so then the
excited reacting molecule reacts to produce product.
29-August -20 Dr. Yogita Sahebrao Thakare
29-August -20 Dr. Yogita Sahebrao Thakare
Electromagnetic radiations
Electromagnetic Radiation
Electromagnetic radiation is a form of energy that is transmitted through space with
velocity of light (C = 3 Γ— 108 ms-1). Electromagnetic radiation is the combination of
electric & magnetic fields which are perpendicular to each other and also
perpendicular to direction of propagation ( Fig. 1).
Thus electromagnetic radiation can be considered as a simple harmonic wave
prorogated in space, in a straight line. Electromagnetic radiations are spread over a
range of wavelengths. Visible light, UV light, IR radiations, X-ray,
29-August -20 Dr. Yogita Sahebrao Thakare
29-August -20 Dr. Yogita Sahebrao Thakare
29-August -20 Dr. Yogita Sahebrao Thakare
Electromagnetic radiations exhibit dual nature (Wave as well as particle)
some phenomena like reflection of light, refraction of light, interference
of light etc. could be explain only in terms of wave characters where as
other phenomena like blackbody radiations spectrum, photoelectric
effect, Compton effect etc. could not be explain in terms of wave nature.
However, the later phenomena could be explained in terms of particle
nature.
According Planck’s Quantum Theory of Radiation radiant energy emits
or absorbed not continuously (not as continuous wave) but
discontinuously or discretely in the form of small packets or bundles or
discrete unit of waves. Each of this unit is called a quantum (plural
quanta) which can exist independently.
The energy associated with each quantum or photon (in case of light) is
proportional to the frequency (Ξ½) of emitted radiation,
i.e. E Ξ± Ξ½ or E = h Ξ½29-August -20 Dr. Yogita Sahebrao Thakare
General characteristics of electromagnetic radiations:
1. All the electromagnetic radiations are associated with oscillating
electrical and magnetic vectors at right angle to each other and
also right angle to the direction of propagation.
2. All the electromagnetic radiations have the same speed in vacuum.
They travels in vacuum with speed of light.
3. Energy can be transmitted through space by electromagnetic
radiations.
4. Different types of electromagnetic radiations differ from one
another in their wavelength.
5. Since velocity of all types of electromagnetic radiations is constant,
the grater the frequency of radiations smaller is its wave length.
6. A electromagnetic radiation is characterized by the nature of its
wave which are characterized by wave length, wave number,
frequency, time period, amplitude wave front and velocity
29-August -20 Dr. Yogita Sahebrao Thakare
Parameters of EMR : Electromagnetic radiation can be characterized in terms
of following parameters-
I) Wavelength : Distance between two successive crests (maxima) or
troughs (minima) in an electromagnetic wave is defined as wavelength.
It is denoted by the Greek letter Lambda (Ξ»).
Units of Wavelength
nm (nanometer), Β΅m (micrometer), mm (millimeter), cm(centimeter) or m
(meter), Ao (Angstron)
1 nm = 10-9m, 1 Β΅m = 10-6m, 1 mm = 10-3m,
1 cm = 10-2m, 1 Ao = 10 -8 cm 1=10-10 m
II) Frequency : The number of waves passing through a given point in unit
time is called as the frequency of radiation.
It is denoted by the Greek letter Ξ½ (nu) and has a unit of reciprocal time.
It is generally expressed in cycles per second or in Hertz or kilocycles per
second or megacycles per second.
1 Hz = cycle / second or S-1
1 MHz = 103 KHz = 106 Hz
29-August -20 Dr. Yogita Sahebrao Thakare
III) Wave number :- It is defined as the number of waves per unit length and it is
denoted by Ξ½ (nu bar). In spectroscopy, wave number is usually expressed in terms of
cm-1 or m-1
Ξ½ =
1

=
1
π‘€π‘Žπ‘£π‘’π‘™π‘’π‘›π‘”π‘‘β„Ž
But Ξ½ =
𝐢

OR  =
𝐢
Ξ½
OR
1

=
Ξ½
C
OR Ξ½ =
Ξ½
C
IV) Velocity: - The distance travelled by the wave in one second is called the velocity
of the wave. It is denoted by C and expressed as centimeter per second (cm/s) or
meter per second (m/s).
The product of wavelength and frequency
gives the velocity of the wave
i.e. C = ν. 
Where C= Velocity of light in vacuum
But for velocity in air C=V
Where V= velocity of light in air
OR V= ν. 
29-August -20 Dr. Yogita Sahebrao Thakare
V) Energy (E) :- The energy (E) associate with quantum of electromagnetic
radiation is given by
E = h ν = h C / = h Cν (It is called as energy per
Where ,
h = planck`s constant (h= 6.62 Γ— 10-34 JS),
Ξ½ = frequency (Hz)
 = Wavelength of EMR (m)
C = Velocity of light (C = 3 Γ— 108 m/s)
The energy of radiation can be calculated in earg mol-1 or J mol-1 or Kcal mol-1
Energy per mole or energy in Einstein is given by
E = NA h ν = NA h C / = NA h C ν
Where, 𝑁𝐴 = π΄π‘£π‘œπ‘”π‘Žπ‘‘π‘Ÿπ‘œπ‘  π‘›π‘’π‘šπ‘π‘’π‘Ÿ = 6.023 Γ— 1023
π‘šπ‘œπ‘™βˆ’129-August -20 Dr. Yogita Sahebrao Thakare
Impotant Formulae:
1. 𝜈 =
1

=
1
π‘€π‘Žπ‘£π‘’π‘™π‘’π‘›π‘”π‘‘β„Ž
2. 𝜈 =
𝐢

3. E = h 𝜈
4. E = h 𝜈 = h c / = hc 𝜈
5. h = plank constant= 6.626 x 10βˆ’34 𝐽𝑆
6. 1nm = 10βˆ’9m
7. 1𝐴0
= 10βˆ’10
π‘š
8. 1 𝐽 = 107
π‘’π‘Žπ‘Ÿπ‘” = 0.239 π‘π‘Žπ‘™
9. 1 π‘π‘Žπ‘™ = 4.184 𝐽
10. 1 𝑒𝑉 = 1.6021 Γ— 10βˆ’19 𝐽
11. 𝑁𝐴 = π΄π‘£π‘œπ‘”π‘Žπ‘‘π‘Ÿπ‘œπ‘  π‘›π‘’π‘šπ‘π‘’π‘Ÿ = 6.023 Γ— 1023
π‘šπ‘œπ‘™βˆ’1
29-August -20 Dr. Yogita Sahebrao Thakare

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Lect. 1 photochemistry introduction-emr-parameters of emr

  • 1. Dr. Y. S. THAKARE M.Sc. (CHE) Ph D, NET, SET Assistant Professor in Chemistry, Shri Shivaji Science College, Amravati Email: yogitathakare_2007@rediffmail.com B Sc- III Year SEM-V PAPER-III PHYSICAL CHEMISTRY UNIT- V and VI Introduction to syllabus Photochemistry Electromagnetic radiation Parameters of electromagnetic radiation 29-August -20 1
  • 2. Unit V Photochemistry Introduction, Electromagnetic radiation, parameters of electromagnetic radiation, spectrum of electromagnetic radiation, problems, Interaction of radiation with matter, types of chemical reaction- thermal reaction and photochemical reaction, laws of absorption of light- Lambert law and beers law, problems, laws of photochemistry- Grotthus Draper law and stark Einstein's law of photochemical equivalence, Quantum yield, experimental arrangement, reasons for high and low Quantum yield, problems, photochemical reactions, kinetics of photochemical decomposition of HI, photosensitized reaction, mechanism of photosensitization, Joblonski diagram, chemiluminescence, bioluminescence, problems. Electrode – The metal rod dipped in its salt solution29 -August -20 Dr. Yogita Sahebrao Thakare 2
  • 3. Unit VI Molecular spectroscopy Molecular spectroscopy, electromagnetic radiation, parameters of electromagnetic radiation, spectrum of electromagnetic radiation, problems, types of spectra, degree of freedom, energy level diagram, rotational spectroscopy, expression for moment of inertia for diatomic rigid rotator, rotational quantum number, origin of line in rotational spectrum, isotopic effect, applications of rotational spectra for microwave spectroscopy, problems, Vibrational spectroscopy, condition for IR active diatomic molecule, expression for vibrational energy of diatomic molecule considering it as a simple harmonic oscillator, zero point energy, relationship between vibrational frequency and force constant, problems Raman spectroscopy, characteristics of Raman spectrum, origin of stokes and antistokes line in Raman spectrum, rotational Raman spectrum vibrational Raman spectrum, problems 29 -August -20 Dr. Yogita Sahebrao Thakare
  • 4. Unit V Photochemistry Photochemistry : Branch of chemistry which deals with the study of chemical reactions that proceed with the absorption of light by atoms or molecules. Example: photosynthesis, the degradation of plastics and the formation of vitamin D with sunlight. Principles Light is a type of electromagnetic radiation, a source of energy. The Grotthuss- Draper law states that light must be absorbed by a chemical substance in order for a photochemical reaction to take place. According Stark-Einstein law in primary photochemical reaction each molecule of reacting substance absorbs one quantum of radiation which leads to photochemical change. For each photon of light absorbed by a chemical system, no more than one molecule is activated for a photochemical reaction. 29-August -20 Dr. Yogita Sahebrao Thakare
  • 5. OR Photochemistry deals with the study of photochemical reactions. The photochemical reactions are caused by the absorption of light radiations (photons) from visible and ultra violet regions (200-800nm). The photons supply the necessary energy to the reactants so then the excited reacting molecule reacts to produce product. 29-August -20 Dr. Yogita Sahebrao Thakare
  • 6. 29-August -20 Dr. Yogita Sahebrao Thakare
  • 7. Electromagnetic radiations Electromagnetic Radiation Electromagnetic radiation is a form of energy that is transmitted through space with velocity of light (C = 3 Γ— 108 ms-1). Electromagnetic radiation is the combination of electric & magnetic fields which are perpendicular to each other and also perpendicular to direction of propagation ( Fig. 1). Thus electromagnetic radiation can be considered as a simple harmonic wave prorogated in space, in a straight line. Electromagnetic radiations are spread over a range of wavelengths. Visible light, UV light, IR radiations, X-ray, 29-August -20 Dr. Yogita Sahebrao Thakare
  • 8. 29-August -20 Dr. Yogita Sahebrao Thakare
  • 9. 29-August -20 Dr. Yogita Sahebrao Thakare
  • 10. Electromagnetic radiations exhibit dual nature (Wave as well as particle) some phenomena like reflection of light, refraction of light, interference of light etc. could be explain only in terms of wave characters where as other phenomena like blackbody radiations spectrum, photoelectric effect, Compton effect etc. could not be explain in terms of wave nature. However, the later phenomena could be explained in terms of particle nature. According Planck’s Quantum Theory of Radiation radiant energy emits or absorbed not continuously (not as continuous wave) but discontinuously or discretely in the form of small packets or bundles or discrete unit of waves. Each of this unit is called a quantum (plural quanta) which can exist independently. The energy associated with each quantum or photon (in case of light) is proportional to the frequency (Ξ½) of emitted radiation, i.e. E Ξ± Ξ½ or E = h Ξ½29-August -20 Dr. Yogita Sahebrao Thakare
  • 11. General characteristics of electromagnetic radiations: 1. All the electromagnetic radiations are associated with oscillating electrical and magnetic vectors at right angle to each other and also right angle to the direction of propagation. 2. All the electromagnetic radiations have the same speed in vacuum. They travels in vacuum with speed of light. 3. Energy can be transmitted through space by electromagnetic radiations. 4. Different types of electromagnetic radiations differ from one another in their wavelength. 5. Since velocity of all types of electromagnetic radiations is constant, the grater the frequency of radiations smaller is its wave length. 6. A electromagnetic radiation is characterized by the nature of its wave which are characterized by wave length, wave number, frequency, time period, amplitude wave front and velocity 29-August -20 Dr. Yogita Sahebrao Thakare
  • 12. Parameters of EMR : Electromagnetic radiation can be characterized in terms of following parameters- I) Wavelength : Distance between two successive crests (maxima) or troughs (minima) in an electromagnetic wave is defined as wavelength. It is denoted by the Greek letter Lambda (Ξ»). Units of Wavelength nm (nanometer), Β΅m (micrometer), mm (millimeter), cm(centimeter) or m (meter), Ao (Angstron) 1 nm = 10-9m, 1 Β΅m = 10-6m, 1 mm = 10-3m, 1 cm = 10-2m, 1 Ao = 10 -8 cm 1=10-10 m II) Frequency : The number of waves passing through a given point in unit time is called as the frequency of radiation. It is denoted by the Greek letter Ξ½ (nu) and has a unit of reciprocal time. It is generally expressed in cycles per second or in Hertz or kilocycles per second or megacycles per second. 1 Hz = cycle / second or S-1 1 MHz = 103 KHz = 106 Hz 29-August -20 Dr. Yogita Sahebrao Thakare
  • 13. III) Wave number :- It is defined as the number of waves per unit length and it is denoted by Ξ½ (nu bar). In spectroscopy, wave number is usually expressed in terms of cm-1 or m-1 Ξ½ = 1  = 1 π‘€π‘Žπ‘£π‘’π‘™π‘’π‘›π‘”π‘‘β„Ž But Ξ½ = 𝐢  OR  = 𝐢 Ξ½ OR 1  = Ξ½ C OR Ξ½ = Ξ½ C IV) Velocity: - The distance travelled by the wave in one second is called the velocity of the wave. It is denoted by C and expressed as centimeter per second (cm/s) or meter per second (m/s). The product of wavelength and frequency gives the velocity of the wave i.e. C = Ξ½.  Where C= Velocity of light in vacuum But for velocity in air C=V Where V= velocity of light in air OR V= Ξ½.  29-August -20 Dr. Yogita Sahebrao Thakare
  • 14. V) Energy (E) :- The energy (E) associate with quantum of electromagnetic radiation is given by E = h Ξ½ = h C / = h CΞ½ (It is called as energy per Where , h = planck`s constant (h= 6.62 Γ— 10-34 JS), Ξ½ = frequency (Hz)  = Wavelength of EMR (m) C = Velocity of light (C = 3 Γ— 108 m/s) The energy of radiation can be calculated in earg mol-1 or J mol-1 or Kcal mol-1 Energy per mole or energy in Einstein is given by E = NA h Ξ½ = NA h C / = NA h C Ξ½ Where, 𝑁𝐴 = π΄π‘£π‘œπ‘”π‘Žπ‘‘π‘Ÿπ‘œπ‘  π‘›π‘’π‘šπ‘π‘’π‘Ÿ = 6.023 Γ— 1023 π‘šπ‘œπ‘™βˆ’129-August -20 Dr. Yogita Sahebrao Thakare
  • 15. Impotant Formulae: 1. 𝜈 = 1  = 1 π‘€π‘Žπ‘£π‘’π‘™π‘’π‘›π‘”π‘‘β„Ž 2. 𝜈 = 𝐢  3. E = h 𝜈 4. E = h 𝜈 = h c / = hc 𝜈 5. h = plank constant= 6.626 x 10βˆ’34 𝐽𝑆 6. 1nm = 10βˆ’9m 7. 1𝐴0 = 10βˆ’10 π‘š 8. 1 𝐽 = 107 π‘’π‘Žπ‘Ÿπ‘” = 0.239 π‘π‘Žπ‘™ 9. 1 π‘π‘Žπ‘™ = 4.184 𝐽 10. 1 𝑒𝑉 = 1.6021 Γ— 10βˆ’19 𝐽 11. 𝑁𝐴 = π΄π‘£π‘œπ‘”π‘Žπ‘‘π‘Ÿπ‘œπ‘  π‘›π‘’π‘šπ‘π‘’π‘Ÿ = 6.023 Γ— 1023 π‘šπ‘œπ‘™βˆ’1 29-August -20 Dr. Yogita Sahebrao Thakare