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Chapter 2
PROPERTIES OF RADIATION AND
RADIOISOTOPES

ROBERT ESHUN
S.L.T Department
Accra Polytechnic
 Electromagnetic radiation is a series of energy

waves composed of oscillating electric and
magnetic fields traveling at the speed of light
through a medium or space.
 Two broad categories: ionizing and non-ionizing

radiations.
 The energy of the radiation shown on the

2

spectrum below increases from left to right as the
frequency rises.
Type of radiation
Effects
Source
3
4
5
 Both ionizing and non-ionizing radiation can be

harmful to organisms and can result in changes to
the natural environment.
 The different forms of electromagnetic radiation are

distinguished from each other by the amount of
energy they can transfer to matter, which depends
on their wavelength (frequency).

6
IONISING RADIATION
 Radiations with enough high energy to ionize atoms.

 Ionizing radiation has the power to create charged ions

by displacing electrons in atoms.
 They have enough energy to remove tightly bound

electrons from atoms, thus creating ions.
 They can cause chemical changes by breaking

chemical bonds. This effect can cause damage to living
tissue.

7
 Ionizing radiations include alpha, beta, x-ray and

gamma rays.
 Shorter wavelength u.v. radiation have enough

energy to break chemical bonds, hence are
classified as ionizing.
 Uses include generation of electric power, killing of

cancerous cells, and in many manufacturing
processes.
 Ionizing radiation can produce a number of
8

physiological effects, such as those associated with
risk of mutation or cancer.
 Alpha, beta particles and gamma radiation
Type of radiation

Alpha particle

Penetrating power

Mass

Charge

Speed

α

Stopped by paper or skin

4

+2

Slow

Beta particle

β

Stopped by thin metal

Negligible

-1

Fast

Gamma ray

9

Symbol

Formula

γ

Reduced by many cms of No mass
lead or a few metres of
concrete

No charge

Speed
light

of
Alpha Beta Gamma:
 Alpha particles - Fast moving helium atoms. They have
high energy, typically in the MeV range, but due to their
large mass, they are stopped by just a few inches of air,
or a piece of paper.
 Beta - Fast moving electrons. They typically have

energies in the range of a few hundred keV to several
MeV. Since electrons are much lighter than helium
atoms, they are able to penetrate further, through
several feet of air, or several millimeters of plastic or
less of very light metals.
 Gamma - These are photons, just like light, except of

10

much higher energy, typically from several keV to
several MeV. X-Rays and gamma rays are really the
same thing, the difference is how they were produced.
Depending on their energy, they can be stopped by a
11
NON-IONIZING RADIATION
 Radiation with enough energy to move atoms in a
molecule around or cause them to vibrate, but not
enough to remove electrons from them.
 They have the capacity to change the position of

atoms but not to alter their structure, composition,
and properties.
 Non-ionizing radiations include the spectrum of

12

ultraviolet (UV), visible light, infrared (IR),
microwave (MW), radio frequency (RF), and
extremely low frequency (ELF). Lasers commonly
operate in the UV, visible, and IR frequencies.
 Extremely Low Frequency Radiation (ELF)

ELF radiation at 60 HZ is produced by power lines, electrical
wiring, and electrical equipment. Common sources of
intense exposure include ELF induction furnaces and highvoltage power lines.
 Radiofrequency and Microwave radiation

Microwave radiation is absorbed near the skin, while
Radiofrequency (RF) radiation may be absorbed throughout
the body. At high intensities both will damage tissue through
heating. Sources of RF and MW radiation include radio
emitters and cell phones.
 Infrared Radiation (IR)

13

The skin and eyes absorb infrared radiation (IR) as heat.
Workers normally notice excessive exposure through heat
sensation and pain. Sources of IR radiation include
furnaces, heat lamps, and IR lasers.
 Visible Light Radiation

The different visible frequencies of the electromagnetic (EM)
spectrum are "seen" by our eyes as different colors. Good
lighting is conducive to increased production, and may help
prevent incidents related to poor lighting conditions.
Excessive visible radiation can damage the eyes and skin.
 Ultraviolet Radiation (UV)

Ultraviolet radiation (UV) has a high photon energy range
and is particularly hazardous because there are usually no
immediate symptoms of excessive exposure. Sources of UV
radiation include the sun, black lights, welding arcs, and UV
lasers.
 Laser hazards

Lasers typically emit optical (UV, visible light, IR) radiations
and are primarily an eye and skin hazard. Common lasers
include CO2 IR laser; helium - neon, neodymium YAG, and
ruby visible lasers, and the Nitrogen UV laser.
14
 Microwave ovens use microwaves to heat food, toasters

use infrared waves to heat; televisions, cell phones, and
fm radios use radio waves.
 Some forms of non-ionizing radiation can damage

tissues if we are exposed too much. For instance, too
much ultraviolet (UV) light from the sun is known to
cause some skin cancers.
 Apart from the sun, UV radiation are emitted by lights

used in tanning beds, black lights, and lights used to
pasteurize fruit juices.
 Some UV waves have an energy that is high enough to
15

cause a structural change within atoms.
Interaction of various radiations with matter

16
Radioactivity
 This is the spontaneous disintegration of an unstable

atomic nucleus and the emission of alpha or beta
particles and gamma rays.
 It also be defined as the spontaneous disintegration of

an unstable nucleus to form a stable nucleus, with the
emission of alpha (α), beta (β) or gamma radiation (γ).
 All naturally occurring elements with atomic numbers

greater than 83, as well as some isotopes of lighter
elements, are radioactive.

 The emitting nuclide is known as the parent, and the
17

particles emitted with the stable nuclide formed are
known as daughter.
Radioactive decay is the process in which an
unstable atomic nucleus loses energy by
emitting radiation in the form of particles or
electromagnetic waves.
There are numerous types of radioactive decay.
The general idea:

An unstable nucleus releases
energy to become more stable
 Two categories of radioactivity
 Natural radioactivity: This is the spontaneous

disintegration of naturally occurring radio–nuclides
to form a more stable nuclide with the emission of
radiations of alpha, beta and gamma.

 Artificial radioactivity: This is the spontaneous

disintegration of a nuclide when bombarded with a
fast moving thermal neutron to produce a new
nuclide with the emission of radiations of alpha, beta
and gamma and a large amount heat.
19
Derive radioactive decay
and half-life equations
(solve questions)
Discuss the features of
radioactive decays (pg. 18
& 19)
20
 Alpha decay
 An example is the decay of Radon-222 (Rn-222) as

shown in the following equation:

21
 Beta decay
 A beta particle is essentially an electron that’s emitted

from the nucleus. Iodine-131 (I-131), which is used in
the detection and treatment of thyroid cancer, is a
beta particle emitter:

22
 Gamma emission
 Alpha and beta particles have the characteristics of

matter: They have definite masses, occupy space,
and so on. However there is no mass change
associated with gamma emission.
 Gamma radiation is similar to x-rays — high energy,

short wavelength radiation. Gamma radiation
commonly accompanies both alpha and beta
emission, but it’s usually not shown in a balanced
nuclear reaction.
 Some isotopes, such as Cobalt-60 (Co-60), give off
23

large amounts of gamma radiation. Co-60 is used in
the radiation treatment of cancer. Gamma rays are
focused on the tumor to destroy it.
 Positron emission
 A positron is essentially an electron that has a positive

charge instead of a negative charge.
 It is formed when a proton in the nucleus decays into

a neutron and a positively charged electron. The
positron is then emitted from the nucleus.

24
 Electron capture
 This is a rare type of nuclear decay in which an electron

from the innermost energy level is captured by the
nucleus. This electron combines with a proton to form a
neutron. The atomic number decreases by one, but the
mass number stays the same.
 The following equation shows the electron capture of

Polonium-204 (Po-204):

 This creates an isotope of bismuth (Bi-204). The capture

of the 1s electron leaves a vacancy in the 1s orbitals.
Electrons drop down to fill the vacancy, releasing energy
in the X-ray portion of the electromagnetic spectrum.
25
 Note that for any element:

 Number of Electrons = Number of Protons = Atomic

Number (Z)
 Number of Neutrons (n) = Mass Number(A) - Atomic

Number(Z)

26
Mass defect and Nuclear binding
 Two forces exist in the nucleus: electrostatic

repulsion and strong force.
 Electrostatic force is the repulsion between the

similarly charged protons.
 Strong force is an attractive short range force.

 If the electrostatic forces are greater than the strong

force, the nuclide becomes unstable.
27
 For most atoms the strong forces are greater than

the electrostatic repulsion.
 Binding energy is the energy holding protons and

neutrons together in an atomic nucleus.
 This is obtained from the energy equivalence of

mass.
 The mass of a nucleus is not the same as the sum

of the masses of its individual nucleons.
28
 The mass of an atom is always slightly less than

the sum of the masses of its individual neutrons,
protons and electrons.
 The difference between the mass of the atom and

the sum of the masses of its component protons,
neutrons and electrons is the mass defect (∆m).
 The mass defect can be calculated using the

equation below.

29
 Neutron = 1.6749286*10-27 kg

Proton = 1.6726231*10-27 kg
Electron = 9.1093897*10-31 kg

Neutron = 939.56563 MeV
Proton = 938.27231 MeV
Electron = 0.51099906 MeV

1 amu = 1.6606 x 10-27 kg

30
Summary/Questions
 What causes a nucleus to decay? What makes a

nucleus radioactive?
 Arrange these emissions from least to greatest
penetrability: Gamma, Alpha, Beta.
 What is the greatest source of exposure to
radioactivity in our everyday lives?
 If I tell you that that the half-life of Fellmanium-250 is
10 days, how much would be left after 30 days if I
started with 1600 atoms?
NUCLEAR REACTIONS
 Bombardment of atomic nuclei with energetic
particles, resulting in a change in the structure of
the nuclei.

32
 Fission reaction
 Nuclear reaction in which the nucleus of an atom

with a large mass number splits into smaller, lighter
nuclei, often producing free neutrons and photons
(gamma rays) and releasing a tremendous amount
of energy.
 It is induced by a slow moving neutron.
 Energy released is in the form of both

electromagnetic radiation and kinetic energy of
resulting fragments.
33
 It produces millions times the amount of energy

obtainable from the same mass of chemical fuels
such as petrol.
 This makes it a very dense source of energy.

 However, the products of nuclear fission are very

radioactive giving rise to nuclear waste problems.

34
 Nuclear power plant convert energy in the nuclei of

atoms into electrical energy.
 Nuclear fuels undergo fission when bombarded with

neutrons.
 More neutrons are produced resulting in a self-

sustaining chain reaction that releases energy at a
controlled rate in a nuclear reactor,...
 or at a very rapid uncontrolled rate in a nuclear
35

bomb… booom!!!!
uranium nucleus

neutron

fission fragments

The nuclear chain reaction

36

neutrons
37
Reactor charge face
3m thick concrete biological shield

Hot gas out

Steam out to turbines

Reactor core

Cold water in

Heat exchanger

Uranium fuel
rods

Boron control rods
Steel pressure vessel

Graphite moderator

38

Cold gas in
 Fissionable material - enriched 3% uranium-235

and 97% uranium-238 in the form of pellets
encased in long tubes known as fuel rods.
 Control rods - inserted between the fuel rods to

absorb neutrons. They moderate the chain
reaction.
 Pressurised water – flowing round fuel rods carries

away energy released and acts as a coolant. The
high pressure is to prevent extremely hot water
from boiling.
 Pressurised water - also slows down the neutrons,
39

making them easy to be absorbed. This process is
known as thermalization or moderation.
 The pressurised high temperature water is passed

through small tubes (primary loop) inside the
generator.
 Feed-water from secondary tubes gets heated as

they flow over the small tubes.
 This water is returned to the reactor to be heated

again and again till the temperature is about 2350C
and pressurised to about 68 atmospheres.
 This steam is directed to turn turbines to generate
40

electricity.
 1kg of uranium U235 can potentially release

4.9x1013J of energy!
 This is enough energy to heat a house, with a

5kW heater, 24 hours a day, 7 days a week, 52
weeks a year for over 300 years!
 It is not quite that simple because its difficult to

get ALL the nuclei to split.

41
 Fusion reaction
 The combination of two light nuclei to form a single

heavier nucleus, with the release of a large amount
of energy.

42
 This reaction releases energy which is more than a

million times greater than that obtainable from a
typical chemical reaction.
 The sum of the masses of the product nuclei is less

than the sum of the masses of the initial fusing
nuclei.
 The mass deficit (‘lost mass’) is converted to

energy, carried away by the fusion products.
 Most of this energy is released as kinetic energy of

the resulting particles.
43
 Large electrostatic repulsion between reacting

nuclei since both are positively charged
 Large initial energy is required to overcome

repulsion and start reaction.
 When nuclei are close enough, repulsion is

overcome by the attractive strong nuclear force,
which is stronger at very short distances.

44
 1 kg of deuterium can potentially release 8.45 x

1014 J of energy.

45
Discuss
 Peaceful uses of nuke reactions
 Health hazards from radioactive

substances.
 Applications of radioactivity.

46

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Chapter 2 properties of radiations and radioisotopes

  • 1. Chapter 2 PROPERTIES OF RADIATION AND RADIOISOTOPES ROBERT ESHUN S.L.T Department Accra Polytechnic
  • 2.  Electromagnetic radiation is a series of energy waves composed of oscillating electric and magnetic fields traveling at the speed of light through a medium or space.  Two broad categories: ionizing and non-ionizing radiations.  The energy of the radiation shown on the 2 spectrum below increases from left to right as the frequency rises. Type of radiation Effects Source
  • 3. 3
  • 4. 4
  • 5. 5
  • 6.  Both ionizing and non-ionizing radiation can be harmful to organisms and can result in changes to the natural environment.  The different forms of electromagnetic radiation are distinguished from each other by the amount of energy they can transfer to matter, which depends on their wavelength (frequency). 6
  • 7. IONISING RADIATION  Radiations with enough high energy to ionize atoms.  Ionizing radiation has the power to create charged ions by displacing electrons in atoms.  They have enough energy to remove tightly bound electrons from atoms, thus creating ions.  They can cause chemical changes by breaking chemical bonds. This effect can cause damage to living tissue. 7
  • 8.  Ionizing radiations include alpha, beta, x-ray and gamma rays.  Shorter wavelength u.v. radiation have enough energy to break chemical bonds, hence are classified as ionizing.  Uses include generation of electric power, killing of cancerous cells, and in many manufacturing processes.  Ionizing radiation can produce a number of 8 physiological effects, such as those associated with risk of mutation or cancer.
  • 9.  Alpha, beta particles and gamma radiation Type of radiation Alpha particle Penetrating power Mass Charge Speed α Stopped by paper or skin 4 +2 Slow Beta particle β Stopped by thin metal Negligible -1 Fast Gamma ray 9 Symbol Formula γ Reduced by many cms of No mass lead or a few metres of concrete No charge Speed light of
  • 10. Alpha Beta Gamma:  Alpha particles - Fast moving helium atoms. They have high energy, typically in the MeV range, but due to their large mass, they are stopped by just a few inches of air, or a piece of paper.  Beta - Fast moving electrons. They typically have energies in the range of a few hundred keV to several MeV. Since electrons are much lighter than helium atoms, they are able to penetrate further, through several feet of air, or several millimeters of plastic or less of very light metals.  Gamma - These are photons, just like light, except of 10 much higher energy, typically from several keV to several MeV. X-Rays and gamma rays are really the same thing, the difference is how they were produced. Depending on their energy, they can be stopped by a
  • 11. 11
  • 12. NON-IONIZING RADIATION  Radiation with enough energy to move atoms in a molecule around or cause them to vibrate, but not enough to remove electrons from them.  They have the capacity to change the position of atoms but not to alter their structure, composition, and properties.  Non-ionizing radiations include the spectrum of 12 ultraviolet (UV), visible light, infrared (IR), microwave (MW), radio frequency (RF), and extremely low frequency (ELF). Lasers commonly operate in the UV, visible, and IR frequencies.
  • 13.  Extremely Low Frequency Radiation (ELF) ELF radiation at 60 HZ is produced by power lines, electrical wiring, and electrical equipment. Common sources of intense exposure include ELF induction furnaces and highvoltage power lines.  Radiofrequency and Microwave radiation Microwave radiation is absorbed near the skin, while Radiofrequency (RF) radiation may be absorbed throughout the body. At high intensities both will damage tissue through heating. Sources of RF and MW radiation include radio emitters and cell phones.  Infrared Radiation (IR) 13 The skin and eyes absorb infrared radiation (IR) as heat. Workers normally notice excessive exposure through heat sensation and pain. Sources of IR radiation include furnaces, heat lamps, and IR lasers.
  • 14.  Visible Light Radiation The different visible frequencies of the electromagnetic (EM) spectrum are "seen" by our eyes as different colors. Good lighting is conducive to increased production, and may help prevent incidents related to poor lighting conditions. Excessive visible radiation can damage the eyes and skin.  Ultraviolet Radiation (UV) Ultraviolet radiation (UV) has a high photon energy range and is particularly hazardous because there are usually no immediate symptoms of excessive exposure. Sources of UV radiation include the sun, black lights, welding arcs, and UV lasers.  Laser hazards Lasers typically emit optical (UV, visible light, IR) radiations and are primarily an eye and skin hazard. Common lasers include CO2 IR laser; helium - neon, neodymium YAG, and ruby visible lasers, and the Nitrogen UV laser. 14
  • 15.  Microwave ovens use microwaves to heat food, toasters use infrared waves to heat; televisions, cell phones, and fm radios use radio waves.  Some forms of non-ionizing radiation can damage tissues if we are exposed too much. For instance, too much ultraviolet (UV) light from the sun is known to cause some skin cancers.  Apart from the sun, UV radiation are emitted by lights used in tanning beds, black lights, and lights used to pasteurize fruit juices.  Some UV waves have an energy that is high enough to 15 cause a structural change within atoms.
  • 16. Interaction of various radiations with matter 16
  • 17. Radioactivity  This is the spontaneous disintegration of an unstable atomic nucleus and the emission of alpha or beta particles and gamma rays.  It also be defined as the spontaneous disintegration of an unstable nucleus to form a stable nucleus, with the emission of alpha (α), beta (β) or gamma radiation (γ).  All naturally occurring elements with atomic numbers greater than 83, as well as some isotopes of lighter elements, are radioactive.  The emitting nuclide is known as the parent, and the 17 particles emitted with the stable nuclide formed are known as daughter.
  • 18. Radioactive decay is the process in which an unstable atomic nucleus loses energy by emitting radiation in the form of particles or electromagnetic waves. There are numerous types of radioactive decay. The general idea: An unstable nucleus releases energy to become more stable
  • 19.  Two categories of radioactivity  Natural radioactivity: This is the spontaneous disintegration of naturally occurring radio–nuclides to form a more stable nuclide with the emission of radiations of alpha, beta and gamma.  Artificial radioactivity: This is the spontaneous disintegration of a nuclide when bombarded with a fast moving thermal neutron to produce a new nuclide with the emission of radiations of alpha, beta and gamma and a large amount heat. 19
  • 20. Derive radioactive decay and half-life equations (solve questions) Discuss the features of radioactive decays (pg. 18 & 19) 20
  • 21.  Alpha decay  An example is the decay of Radon-222 (Rn-222) as shown in the following equation: 21
  • 22.  Beta decay  A beta particle is essentially an electron that’s emitted from the nucleus. Iodine-131 (I-131), which is used in the detection and treatment of thyroid cancer, is a beta particle emitter: 22
  • 23.  Gamma emission  Alpha and beta particles have the characteristics of matter: They have definite masses, occupy space, and so on. However there is no mass change associated with gamma emission.  Gamma radiation is similar to x-rays — high energy, short wavelength radiation. Gamma radiation commonly accompanies both alpha and beta emission, but it’s usually not shown in a balanced nuclear reaction.  Some isotopes, such as Cobalt-60 (Co-60), give off 23 large amounts of gamma radiation. Co-60 is used in the radiation treatment of cancer. Gamma rays are focused on the tumor to destroy it.
  • 24.  Positron emission  A positron is essentially an electron that has a positive charge instead of a negative charge.  It is formed when a proton in the nucleus decays into a neutron and a positively charged electron. The positron is then emitted from the nucleus. 24
  • 25.  Electron capture  This is a rare type of nuclear decay in which an electron from the innermost energy level is captured by the nucleus. This electron combines with a proton to form a neutron. The atomic number decreases by one, but the mass number stays the same.  The following equation shows the electron capture of Polonium-204 (Po-204):  This creates an isotope of bismuth (Bi-204). The capture of the 1s electron leaves a vacancy in the 1s orbitals. Electrons drop down to fill the vacancy, releasing energy in the X-ray portion of the electromagnetic spectrum. 25
  • 26.  Note that for any element:  Number of Electrons = Number of Protons = Atomic Number (Z)  Number of Neutrons (n) = Mass Number(A) - Atomic Number(Z) 26
  • 27. Mass defect and Nuclear binding  Two forces exist in the nucleus: electrostatic repulsion and strong force.  Electrostatic force is the repulsion between the similarly charged protons.  Strong force is an attractive short range force.  If the electrostatic forces are greater than the strong force, the nuclide becomes unstable. 27
  • 28.  For most atoms the strong forces are greater than the electrostatic repulsion.  Binding energy is the energy holding protons and neutrons together in an atomic nucleus.  This is obtained from the energy equivalence of mass.  The mass of a nucleus is not the same as the sum of the masses of its individual nucleons. 28
  • 29.  The mass of an atom is always slightly less than the sum of the masses of its individual neutrons, protons and electrons.  The difference between the mass of the atom and the sum of the masses of its component protons, neutrons and electrons is the mass defect (∆m).  The mass defect can be calculated using the equation below. 29
  • 30.  Neutron = 1.6749286*10-27 kg Proton = 1.6726231*10-27 kg Electron = 9.1093897*10-31 kg Neutron = 939.56563 MeV Proton = 938.27231 MeV Electron = 0.51099906 MeV 1 amu = 1.6606 x 10-27 kg 30
  • 31. Summary/Questions  What causes a nucleus to decay? What makes a nucleus radioactive?  Arrange these emissions from least to greatest penetrability: Gamma, Alpha, Beta.  What is the greatest source of exposure to radioactivity in our everyday lives?  If I tell you that that the half-life of Fellmanium-250 is 10 days, how much would be left after 30 days if I started with 1600 atoms?
  • 32. NUCLEAR REACTIONS  Bombardment of atomic nuclei with energetic particles, resulting in a change in the structure of the nuclei. 32
  • 33.  Fission reaction  Nuclear reaction in which the nucleus of an atom with a large mass number splits into smaller, lighter nuclei, often producing free neutrons and photons (gamma rays) and releasing a tremendous amount of energy.  It is induced by a slow moving neutron.  Energy released is in the form of both electromagnetic radiation and kinetic energy of resulting fragments. 33
  • 34.  It produces millions times the amount of energy obtainable from the same mass of chemical fuels such as petrol.  This makes it a very dense source of energy.  However, the products of nuclear fission are very radioactive giving rise to nuclear waste problems. 34
  • 35.  Nuclear power plant convert energy in the nuclei of atoms into electrical energy.  Nuclear fuels undergo fission when bombarded with neutrons.  More neutrons are produced resulting in a self- sustaining chain reaction that releases energy at a controlled rate in a nuclear reactor,...  or at a very rapid uncontrolled rate in a nuclear 35 bomb… booom!!!!
  • 36. uranium nucleus neutron fission fragments The nuclear chain reaction 36 neutrons
  • 37. 37
  • 38. Reactor charge face 3m thick concrete biological shield Hot gas out Steam out to turbines Reactor core Cold water in Heat exchanger Uranium fuel rods Boron control rods Steel pressure vessel Graphite moderator 38 Cold gas in
  • 39.  Fissionable material - enriched 3% uranium-235 and 97% uranium-238 in the form of pellets encased in long tubes known as fuel rods.  Control rods - inserted between the fuel rods to absorb neutrons. They moderate the chain reaction.  Pressurised water – flowing round fuel rods carries away energy released and acts as a coolant. The high pressure is to prevent extremely hot water from boiling.  Pressurised water - also slows down the neutrons, 39 making them easy to be absorbed. This process is known as thermalization or moderation.
  • 40.  The pressurised high temperature water is passed through small tubes (primary loop) inside the generator.  Feed-water from secondary tubes gets heated as they flow over the small tubes.  This water is returned to the reactor to be heated again and again till the temperature is about 2350C and pressurised to about 68 atmospheres.  This steam is directed to turn turbines to generate 40 electricity.
  • 41.  1kg of uranium U235 can potentially release 4.9x1013J of energy!  This is enough energy to heat a house, with a 5kW heater, 24 hours a day, 7 days a week, 52 weeks a year for over 300 years!  It is not quite that simple because its difficult to get ALL the nuclei to split. 41
  • 42.  Fusion reaction  The combination of two light nuclei to form a single heavier nucleus, with the release of a large amount of energy. 42
  • 43.  This reaction releases energy which is more than a million times greater than that obtainable from a typical chemical reaction.  The sum of the masses of the product nuclei is less than the sum of the masses of the initial fusing nuclei.  The mass deficit (‘lost mass’) is converted to energy, carried away by the fusion products.  Most of this energy is released as kinetic energy of the resulting particles. 43
  • 44.  Large electrostatic repulsion between reacting nuclei since both are positively charged  Large initial energy is required to overcome repulsion and start reaction.  When nuclei are close enough, repulsion is overcome by the attractive strong nuclear force, which is stronger at very short distances. 44
  • 45.  1 kg of deuterium can potentially release 8.45 x 1014 J of energy. 45
  • 46. Discuss  Peaceful uses of nuke reactions  Health hazards from radioactive substances.  Applications of radioactivity. 46