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Atomic Energy

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Atomic Energy 3U Physics Mass-Energy Equivalence All matter is a form of stored energy. Mass-Energy Equivalence All matter is a form of stored energy. – PowerPoint PPT presentation

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Title: Atomic Energy


1
Atomic Energy
  • 3U Physics

2
Mass-Energy Equivalence
  • All matter is a form of stored energy.

3
Mass-Energy Equivalence
  • All matter is a form of stored energy.
  • If matter of mass m is converted to energy, the
    amount of energy E that can be released is equal
    to

4
Mass-Energy Equivalence
  • All matter is a form of stored energy.
  • If matter of mass m is converted to energy, the
    amount of energy E that can be released is equal
    to
  • E mc2

5
Mass-Energy Equivalence
  • All matter is a form of stored energy.
  • If matter of mass m is converted to energy, the
    amount of energy E that can be released is equal
    to
  • E mc2
  • c 3.0 x 108 m/s

6
Mass-Energy Equivalence Example
  • What is the energy equivalent of a 52 kg person?

7
Mass-Energy Equivalence Example
  • What is the energy equivalent of a 52 kg person?

8
Mass-Energy Equivalence Example
  • What is the energy equivalent of a 52 kg person?

9
The Mass Defect
  • More practically, we look at the energy
    equivalent of the mass defect.

10
The Mass Defect
  • More practically, we look at the energy
    equivalent of the mass defect.

11
The Mass Defect
  • Consider a Carbon 12 nucleus

12
The Mass Defect
  • Consider a Carbon 12 nucleus
  • 6 protons, 1.007276 amu each
  • 6 neutrons, 1.008665 amu each
  • 12.095646 amu

13
The Mass Defect
  • Consider a Carbon 12 nucleus
  • 6 protons, 1.007276 amu each
  • 6 neutrons, 1.008665 amu each
  • 12.095646 amu
  • Actual mass of Carbon 12 nucleus
  • 11.996709 amu

14
The Mass Defect
  • The 0.098937 amu mass defect is the binding
    energy of the nucleus.
  • E mc2
  • E (0.098937)(1.66 x 10-27 kg)(3.0 x 108 m/s)2
  • E 1.5 x 10-11 J

15
The Mass Defect
  • Energy stored in the nucleus can be released in
    nuclear reactions such as radioactive decay

16
The Mass Defect
  • Energy stored in the nucleus can be released in
    nuclear reactions such as radioactive decay
  • The energy is released in the form of kinetic
    energy (of the resulting particles).

17
Nuclear Fission
  • However, in a nuclear reactor, we dont sit
    around waiting for a radioactive decay.

18
Nuclear Fission
  • However, in a nuclear reactor, we dont sit
    around waiting for a radioactive decay. We
    trigger them by bombarding nuclei with neutrons

19
Nuclear Fission
  • Notice that the reaction produces more neutrons,
    which can then bombard more nuclei in a chain
    reaction

20
Nuclear Fusion
  • Energy can also be obtained by fusing together
    light elements, e.g. hydrogen into helium

21
Nuclear Fusion
  • However, fusing nuclei requires overcoming the
    electrostatic repulsion between the nuclei.

22
Nuclear Fusion
  • However, fusing nuclei requires overcoming the
    electrostatic repulsion between the nuclei.
  • This requires enormous temperatures and pressures
    such as those produced in the core of the Sun.

23
Nuclear Power
  • The ejected neutron has too much energy to start
    another nuclear reaction on its own

24
CANDU Reactor
  • Fuel rods are surrounded by heavy water
  • Deuterium istotope of hydrogen with one neutron
  • Makes water 11 more dense
  • Heavy water heats up free neutrons slow down
  • Chain reaction continues
  • EK of neutron becomes Eth of water
  • Steam turns turbine, generates power

25
CANDU Reactor
  • http//www.youtube.com/watch?vjNOzh4Kwgpw
  • Is it environmentally friendly?

26
Radioactive Waste
  • Unstable atoms are called radioactive
  • They have the ability to decay into another
    substance and emit radiation
  • The rate of decay is predictable

27
Half-Life
  • The average length of time it takes a radioactive
    material to decay to half its original mass
  • Ex. If a 10 kg sample of radioactive material has
    a half-life of 5 years, how much will be left
    after 5 years? 10 years?

28
Types of Decay
Type of Decay Radiation Emitted Particle Penetrating Power
alpha alpha particle helium nucleus skin or paper (slow moving)
beta negative beta particle electron a few sheets of aluminum foil
gamma gamma rays photon a few centimetres of lead
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