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Title: Intro to Nuclear Chemistry


1
Intro to Nuclear Chemistry
  • DECEMBER 12

http//www.chem.orst.edu/graduate/pics/Reactor.jpg

2
How does a nuclear reactor work?
http//www.lanl.gov/science/1663/images/reactor.jp
g
3
How does a small mass contained in this bomb
cause
  • Nuclear Bomb of 1945 known as fat man

http//www.travisairmuseum.org/assets/images/fatma
n.jpg
4
this huge nuclear explosion?
http//library.thinkquest.org/06aug/01200/Graphics
/705px-Nuclear_fireball.jpg
5
Is there radon in your basement?
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070625_ssh.jpg
6
Notation

7
Nucleons
  • Protons and Neutrons

8
  • The nucleons are bound together by a strong force
    called binding force.

9
Isotopes
  • Atoms of a given element with
  • same protons
  • but
  • different neutrons

10
  • H H H

http//education.jlab.org/glossary/isotope.html
11
Isotopes of Carbon
12
Radioactive Isotopes
  • Isotopes of certain unstable elements that
    spontaneously emit particles and energy from the
    nucleus.
  • Henri Beckerel 1896 accidentally observed
    radioactivity of uranium salts that were fogging
    photographic film.
  • His associates were Marie and Pierre Curie.

13
Marie Curie born 1867, in Poland as Maria
Sklodowska
  • Lived in France
  • 1898 discovered the elements polonium and radium.

http//www.radiochemistry.org/nuclearmedicine/pion
eers/images/mariecurie.jpg
14
Marie Curie a Pioneer of Radioactivity
  • Winner of 1903 Nobel Prize for Physics with Henri
    Becquerel and her husband, Pierre Curie.
  • Winner of the sole 1911 Nobel Prize for
    Chemistry.

15
RADIOACTIVITY
  • Emission of rays and particles from unstable
    nuclei.
  • When a nucleus is emitting rays or particles it
    is said that is DECAYING or is disintegrating.

16
Stability of nuclei
  • Depend on the ratio between the neutrons and
    protons. Too many or too few neutrons lead to an
    unstable nucleus. All elements with more than 83
    protons are unstable.

17
Transmutation
  • When the nucleus of one element is changed into
    the nucleus of another element. IT CAN ONLY
    HAPPEN IN A NUCLEAR REACTION!!!

18
Nuclear Reactions
  • The chemical properties of the nucleus are
    independent of the state of chemical combination
    of the atom.
  • In writing nuclear equations we are not concerned
    with the chemical form of the atom in which the
    nucleus resides.
  • It makes no difference if the atom is as an
    element or a compound.
  • Mass and charges MUST BE BALANCED!!!

19
Types ofRadioactive Decay
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SeparationAlphaBetaGamma.MOV Separation of
Radiation
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24
Alpha Decay
  • Emission of alpha particles a
  • helium nuclei
  • two protons and two neutrons
  • charge 2e 
  • can travel a few inches through air
  • can be stopped by a sheet of paper, clothing.

25
Alpha Decay
Uranium Thorium
26
Alpha Decay
http//education.jlab.org/glossary/alphadecay.gif
27
Alpha Decay
  • Loss of an ?-particle (a helium nucleus)

28
Alpha Decay
  • Mass changes by 4
  • The remaining fragment has 2 less protons
  • Alpha radiation is the less penetrating of all
    the nuclear radiation (it is the most massive
    one!)

29
Alpha decay
  • When a nucleus emits alpha particles.
  • Atomic number decreases by 2.
  • Mass number decreases by 4.
  • Neutrons decrease by 2.

30
Beta Decay
  • Loss of a ?-particle (a high energy electron)

31
Beta Decay
  • Beta particles b electrons ejected from the
    nucleus when neutrons decay
  • ( n -gt p b- )
  • Beta particles have the same charge and mass as
    "normal" electrons.

32
Beta Decay
  • Beta particles b electrons ejected from the
    nucleus when neutrons decay
  • n -gt p b-
  • Beta particles have the same charge and mass as
    "normal" electrons.
  • Can be stopped by aluminum foil or a block of
    wood.

33
Beta Decay
  • When a neutron becomes a proton and emits an
    electron.
  • Atomic Number or number of protons increases by
    1
  • Number of neutrons decreases by one.
  • Mass number remains the same.
  •  

34
Beta Decay
35
Beta Decay
Thorium
Protactinium
36
Beta Decay
  • Involves the conversion of a neutron in the
    nucleus into a proton and an electron.
  • Beta radiation has high energies, can travel up
    to 300 cm in air.
  • Can penetrate the skin

37
Beta decay
  • Write the reaction of decay for C-14

38
Positron Emission
  • When a proton changes to a neutron emits a
    positron.
  • Atomic number (number of protons)decreases by 1
  • Number of neutrons increase by 1.
  • Mass number remains same

39
Gamma Emission
  • Loss of a ?-ray (high-energy radiation that
    almost always accompanies the loss of a nuclear
    particle)

40
Gamma Decay
  • Gamma radiation g electromagnetic energy that
    is released. 
  • Gamma rays are electromagnetic waves.
  • They have no mass.
  • Gamma radiation has no charge.
  • Most Penetrating, can be stopped by 1m thick
    concrete or a several cm thick sheet of lead.

41
3 Main Types of Radioactive Decay
  • Alpha a
  • Beta b
  • Gamma g

42
Examples of Radioactive Decay
  • Alpha Decay
  • Po ? Pb He
  • Beta Decay p? n e
  • n ? p e
  • C ? N e
  • Gamma Decay
  • Ni ? Ni g
  • (excited nucleus)

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46
Which is more penetrating? Why?
47
December 14
  • Nuclear stability
  • Half life
  • HW review book
  • Question 34 to 47

48
Nuclear Stability
  • Depends on the neutron to proton ratio.

49
Band of Stability
Number of Neutrons, (N)
Number of Protons (Z)
50
What happens to an unstable nucleus?
  • They will undergo decay
  • The type of decay depends on the reason for the
    instability

51
What type of decay will happen if the nucleus
contains too many neutrons?
  • Beta Decay

52
Example
14
0
14
  • C ? N e
  • In N-14 the ratio of neutrons to protons is 11

-1
6
7
53
  • Nuclei with atomic number gt 83 are radioactive

54
Radioactive Half-Life (t1/2 )
  • The time required for one half of the nuclei in a
    given sample to decay.
  • After each half life the mass of sample remaining
    is half.
  • Different Isotopes have different half lives. Use
    table N

55
Common Radioactive Isotopes
Isotope Half-Life Radiation
Emitted Carbon-14 5,730 years b,
g Radon-222 3.8 days a Uranium-235 7.0 x
108 years a, g Uranium-238 4.46 x 109 years
a
56
Radioactive Half-Life
  • After one half life there is 1/2 of original
    sample left.
  • After two half-lives, there will be
  • 1/2 of the 1/2 1/4 the original sample.

57
Graph of Amount of Remaining Nuclei vs Time
AAoe-lt
A
58
Example
  • You have 100 g of radioactive C-14. The half-life
    of C-14 is 5730 years.
  • How many grams are left after one half-life?
    Answer50 g
  • How many grams are left after two half-lives?

59
Problem
  • If 80 g of a radioactive sample decays to 10 g in
    30 min what is the elements half life?

60
  • How many days will take a sample of I-131 to
    undergo three half life periods?

61
  • What is the total mass of Rn-222 remaining in an
    original mass 160 mg sample of Rn-222 after 19.1
    days?

62
Measuring Radioactivity
  • One can use a device like this Geiger counter to
    measure the amount of activity present in a
    radioactive sample.
  • The ionizing radiation creates ions, which
    conduct a current that is detected by the
    instrument.

63
Transmutations
  • To change one element into another.
  • Only possible in nuclear reactions never in a
    chemical reaction.
  • In order to modify the nucleus huge amount of
    energy are involved.
  • These reactions are carried in particle
    accelerators or in nuclear reactors

64
Nuclear transmutations
  • Alpha particles have to move very fast to
    overcame electrostatic repulsions between them
    and the nucleus.
  • Particle accelerators or smashers are used. They
    use magnetic fields to accelerate the particles.

65
Particle Accelerators(only for charged
particles!)
  • These particle accelerators are enormous, having
    circular tracks with radii that are miles long.

66
Cyclotron
  • Nuclear transformations can be induced by
    accelerating a particle and colliding it with the
    nuclide.

67
Neutrons
  • Can not be accelerated. They do not need it
    either (no charge!).
  • Neutrons are products of natural decay, natural
    radioactive materials or are expelled of an
    artificial transmutation.
  • Some neutron capture reactions are carried out in
    nuclear reactors where nuclei can be bombarded
    with neutrons.

68
Mass defect
  • The mass of the nucleus is always smaller than
    the masses of the individual particles added up.
  • The difference is the mass defect.
  • That small amount translate to huge amounts of
    energy ?E (?m) c2
  • That energy is the Binding energy of the nucleus,
    and is the energy needed to separate the nucleus.

69
Energy in Nuclear Reactions
  • For example, the mass change for the decay of 1
    mol of uranium-238 is -0.0046 g.
  • The change in energy, ?E, is then
  • ?E (?m) c2
  • ?E (-4.6 ? 10-6 kg)(3.00 ? 108 m/s)2
  • ?E -4.1 ? 1011 J This amount is 50,000 times
    greater than the combustion of 1 mol of CH4

70
Types of nuclear reactionsfission and fusion
  • The larger the binding energies, the more stable
    the nucleus is toward decomposition.
  • Heavy nuclei gain stability (and give off energy)
    if they are fragmented into smaller nuclei.
    (FISSION)

71
  • Even greater amounts of energy are released if
    very light nuclei are combined or fused together.
    (FUSION)

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Nuclear Fission
  • Nuclear fission is the type of reaction carried
    out in nuclear reactors.

74
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Nuclear Fission
  • Bombardment of the radioactive nuclide with a
    neutron starts the process.
  • Neutrons released in the transmutation strike
    other nuclei, causing their decay and the
    production of more neutrons.

76
Nuclear Fission
  • This process continues in what we call a nuclear
    chain reaction.

77
Controlled vs Uncontrolled nuclear reaction
  • Controlled reactions inside a nuclear power
    plant
  • Uncontrolled reaction nuclear bomb

78
Nuclear Reactors
  • In nuclear reactors the heat generated by the
    reaction is used to produce steam that turns a
    turbine connected to a generator.

79
Nuclear Reactors
  • The reaction is kept in check by the use of
    control rods.
  • These block the paths of some neutrons, keeping
    the system from reaching a dangerous
    supercritical mass.

80
FUSION
  • Combining small nucleii to form a larger one.
  • Require millions of K of temperature

81
Fusion
  • 1H 1H ? 2H 1e energy
  • 1H 2H ? 3He energy
  • 3He 3He ? 4He 21H energy
  • Reaction that occurs in the sun
  • Temperature 107 K
  • Heavier elements are synthesized in hotter stars
    108 K using Carbon as fuel

82
Nuclear Fusion
  • Fusion would be a superior method of generating
    power.
  • The good news is that the products of the
    reaction are not radioactive.
  • The bad news is that in order to achieve fusion,
    the material must be in the plasma state at
    several million kelvins.

83
Nuclear Fusion(thermonuclear reactions)
  • Tokamak apparati like the one shown at the right
    show promise for carrying out these reactions.
  • They use magnetic fields to heat the material.
  • 3 million K degrees were reached inside but is
    not enough to begin fusion which requires 40
    million K

84



Fission is the release of energy by splitting
heavy nuclei such as Uranium-235 and Plutonium-239
Fusion is the release of energy by combining two
light nuclei such as deuterium and tritium
D-T Fusion
4He 3.52 MeV
D
Neutron 14.1 MeV
T
  • The goal of fusion research is to confine fusion
    ions at high enough temperatures and pressures,
    and for a long enough time to fuse
  • This graph shows the exponential rate of progress
    over the decades
  • How does a nuclear plant work?
  • Each fission releases 2 or 3 neutrons
  • These neutrons are slowed down with a moderator
    to initiate more fission events
  • Control rods absorb neutrons to keep the chain
    reaction in check

Controlled Fission Chain Reaction
Confinement Progress
There are two main confinement approaches
The energy from the reaction drives a steam cycle
to produce electricity
  • Magnetic Confinement uses strong magnetic fields
    to confine the plasma
  • This is a cross-section of the proposed
    International Thermo-nuclear Experimental Reactor
    (ITER)

Nuclear Power Plant
  • Nuclear Power produces no greenhouse gas
    emissions each year U.S. nuclear plants prevent
    atmospheric emissions totaling
  • 5.1 million tons of sulfur dioxide
  • 2.4 million tons of nitrogen oxide
  • 164 million tons of carbon
  • Nuclear power in 1999 was the cheapest
  • source of electricity costing 1.83 c/kWh
  • compared to 2.04 c/kWh from coal
  • Inertial Confinement uses powerful lasers or ion
    beams to compress a pellet of fusion fuel to the
    right temperatures and pressures
  • This is a schematic of the National Ignition
    Facility (NIF) being built at Lawrence Livermore
    National Lab

85
Uses of radioisotopes
  • Medicine
  • Medical imaging trace amounts of short half
    life isotopes can be ingested and the path of the
    isotope traced by the radiation given off
  • cancer treatment radiation kills cancerous
    cells more easily than healthy cells

86
  • Sterilisation ? rays can be used to kill
    germs and hence sterilise food and plastic
    equipment
  • Industry used to trace blockages in pipes, or
    to test the thickness of materials (by putting a
    source on one side of the material and detector
    on the other)

87
  • Carbon dating
  • Once a living organism dies, it is no longer
    taking in any Carbon.
  • C14 is radioactive, and decays over time.
  • By measuring the activity of C14 in an object and
    comparing it with the amount of C14 which was
    present initially you can estimate when the
    organism died

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Smoke detectors
  • a radioactive source ionises the air between
    two electrodes. Thus current flows between them
  • If smoke particles enter this space they stick to
    the ions and the current is reduced.
  • This reduced current triggers the alarm
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