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Nuclear Decay Processes

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Title: Nuclear Decay Processes


1
Nuclear Decay Processes
http//www.curtin.edu.au/curtin/centre/waisrc/OKLO
/
2
Nuclear Processes
  • Chemical processes have been involved with the
    electron (outside the nucleus)
  • Sharing, losing, or gaining
  • Speed of reaction
  • Energy involved in change
  • Nuclear processes are involved in processes
    involving the nucleus (inside)
  • What is being lost, gained?
  • Speed of reaction
  • Energy involved in change

3
Nucleus
Nucleons Protons and neutrons in the nucleus
4
Representing the Nucleus
  • 23892U (or U-238)
  • 238 Mass number (A)
  • 92 Atomic number (Z)
  • 92 represents the number of protons
  • 238 represents the number protons neutrons
  • 146 neutrons
  • Isotopes occur due to variations in the numbers
    of neutrons found in the nucleus

5
Nuclear Equations
  • Representations which show the changes in the
    nuclear structure, that is, changes in protons
    and neutrons.
  • 23892U
  • 23892U ? 23490Th ?
  • Radioactive decay spontaneous decomposition of
    the nucleus
  • Radioisotopes atoms containing nuclei that are
    spontaneously decomposing.

Alpha particle (a)
42He
6
Nuclear Stability
  • n to p ratio
  • High
  • Above belt
  • Low
  • Below belt
  • Z gt 84
  • Magic numbers
  • Even-Even

7
Types of Radioactive Decay
  • Alpha radiation
  • Beta radiation
  • Gamma radiation
  • Positron emission
  • Electron capture

8
Alpha Radiation
  • 23892U ? 23490Th 42He
  • Properties of an alpha particle
  • Charge Mass Alias Penetrating Power 2 4
    amu He low
  • nuclei

9
Beta Radiation
  • 6328Ni ? 6329Cu 0-1b
  • Properties of an beta particle
  • Charge Mass Alias Penetrating Power -1 0
    amu electron moderate

10
Gamma Radiation
  • 23892U ? 23490Th 42He 2 00g
  • Properties of an beta particle
  • Charge Mass Alias Penetrating Power
    0 0 amu photon high

11
Positron Emission
  • 116C ? 115B 01b
  • Properties of an beta particle
  • Charge Mass Alias Penetrating Power
    1 0 amu Anti- moderate
  • electron

12
Electron Capture
  • 5526Fe 0-1b ? 5525Mn hn (x-ray)
  • Electron captured from
  • low-energy electron orbital

13
Decaying TowardStability
Z gt 84 Alpha
Beta
23892U ? 23490Th 42He
6328Ni ? 6329Cu 0-1b
Positron or electron capture
116C ? 115B 01b
5526Fe 0-1b ? 5525Mn
14
Rate of Radioactive Decay
  • Uses 1st order kinetics
  • ln Nt -kt ln No
  • Where N can be various measurements.
  • g, Ci, counts/minute, disintegrations/min
  • t1/2 0.693
  • k
  • Radioactive dating

15
Problem
  • A sample of waste has a radioactivity, measured
    at 0.245 Ci/g, caused solely strontium-90.
  • What reason might be used to explain why
    strontium-90 is radioactive?
  • Write an equation representing the most likely
    decay process for strontium-90.
  • How much time will it take for this sample of
    waste to decrease in radiation to a level of 1.00
    x 10-6 Ci/g? (t1/2 28.1 yr)

16
Rate of Radioactive Decay
Rate k No
  • Uses 1st order kinetics
  • ln Nt -kt ln No t1/2 0.693/k
  • Where N can be various measurements.
  • g, Ci, counts/minute, disintegrations/min

Radioactive dating
Carbon-14
17
Problem
  • A sample of waste has a radioactivity, measured
    at 0.245 Ci/g, caused solely strontium-90.
  • How much time will it take for this sample of
    waste to decrease in radiation to a level of 1.00
    x 10-6 Ci/g? (t1/2 28.1 yr)

18
Rate of Decay
  • According to current regulations, the maximum
    permissible dose of strontium-90 in the body of
    an adult is 1mCi. Calculate the number of atoms
    of strontium-90 to which this dose corresponds.
    What mass of strontium-90 is this? (t1/2 28.8
    years)

19
Radioactive Dating (kinetics)
  • A sample of carbon of mass 1.00 g from scrolls
    found near the Dead Sea underwent 1.4 x 104
    carbon-14 disintegrations in 20 hours. Estimate
    the approximate time since the sheepskins were
    removed from the sheep, assuming that 1.00 g from
    a modern source underwent 1.84 x 104
    disintegrations in 20 hours. The t1/2 of C-14 is
    5730 years.

20
Sea of Instability
21
Fermi National Laboratory
22
Transmutation Processes
  • 3216S 10n ? 11p 3215P
  • 3216S (n,p) 3215P
  • 20983Bi 6428Ni ? 272111X 10n
  • 20983Bi (Ni-64, p) 272111X

Possible particles, symbols Proton, p Electron,
b or 0-1e
Neutron, n Positron, b or 01e Alpha, a or 42He
A variety of nuclides
23
Transmutation Processes
  • Used to generate synthetic isotopes designed for
    specific uses.
  • Co-60 radiation therapy isotope for cancer
  • 5826Fe 10n ? 5926Fe ? 5927Co 0-1b
  • 5927Co 10n ? 6027Co

This process is done inside nuclear fission
reactors because fission reactors are excellent
sources of neutrons
24
Uses for Radioisotopes
  • I-131 hyperthyroidism
  • P-32 leukemia and polycythemia vera
  • Cs-137, Ir-192, I-125, Pd-103 brachytherapy
  • B-10 neutron-capture therapy
  • Tl-201 Cardiac imaging
  • Sr-85 Bone scanning
  • Tracers use of radioisotopes as beacons
  • Chemistry used to trace chemical pathways
  • Material flow
  • NAA neutron activation analysis
  • Food irradiation

25
Biological Damage from Radiation
  • Two ways to
  • interact with matter
  • Excitation
  • Ionization
  • Ionizing radiation
  • a - ionizes the most
  • b - middle
  • g - ionizes the least

Inside body a gt b gt g
Outside body g gt b gt a
26
Biological Damage from Radiation
  • H2O g ? H2Os e-
  • H2Os H2O ? H3O OHs
  • e- H2O ? Hs OH-
  • Membrane structure changed
  • Hs RCHCHR ? RCH2-CsHR

27
Radiation Dose Measurements
  • rad - radiation absorbed dose
  • 1 x 10-2 J per kg
  • RBE relative biological
  • effectiveness
  • 1 for g and b radiation
  • 20 for a radiation
  • rem effective dosage of
  • exposure
  • rem (number of rads) (RBE)

28
Problem
  • A 5.0 gram sample of muscle tissue absorbs 2.0 J
    of energy as a result of exposure to a radiation.
    Calculate the dose in rads and gray (Gy) and the
    dose equivalent in rems and in sieverts (Sv).

29
Energy Changes
  • 23592U 10n ? 14156Ba 9236Kr 3
    10n
  • STEPS
  • 235U 234.9935 amu 1) Calculate the
  • 141Ba 140.8833 amu change in mass
  • 92Kr 91.9021 amu 2) E mc2
  • 10n 1.00866 amu mass in kg

30
Binding Energy
  • 11 11p 12 10n ? 2311Na
  • STEPS
  • 23Na 22.98733 amu 1) Calculate the mass
  • 11p 1.00728 amu defect (change
    in
  • 10n 1.00866 amu mass)
  • 2) E mc2
  • 3) Divide by nucleons

31
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32
The Most Stable Nuclei?
  • Which of the following nuclei is likely to have
    the largest mass defect per nucleon?
  • 118Sn 243Cm 59Co 11B

33
Group Problem
  • What is the nuclear binding energy of 1 x 10-7
    mol of P-31?
  • Given that P-31 has an amu of 30.965533 amu
  • H-1 has an atomic weight of 1.00728 amu
  • 10n has an atomic weight of 1.00866 amu

34
Nuclear Power
  • Nature
  • www.curtin.edu.au/curtin/centre/waisrc/OKLO/
  • Fission
  • www.world-nuclear.org
  • www.ans.org/
  • www.nuclearfiles.org
  • Fusion
  • http//europa.eu.int/comm/dg12/fusion1.html
  • www.jet.efda.org

35
Natures Fission Experiment
  • 1st Fission Process?
  • 3500 million
  • years ago
  • U mobilization
  • Ore/reactor formation
  • Reactor operation 2000 million years ago
  • operated for 1 million years
  • Waste movement (For the last 2000 million
    years)

36
Nuclear Fission
37
Fission Chain Reaction
Critical mass quantity of fissionable material
necessary to sustain reaction - 1 effective
neutron
Supercritical mass quantity of fissionable
material necessary to lead to explosion
38
23592U 10n ? 3 10n
Control rods absorb neutrons to regulate the
amount of neutrons present
Moderator slows down neutrons to enhance the
fuels ability to capture neutrons
39
Fusion
  • Proposed
  • Fusion on
  • Sun
  • 11H 11H ? 21H 01b
  • 11H 21H ? 32He
  • 32He 32He ? 42He 2 11H
  • 32He 11H ? 42He 01b

40
tokamak torus shaped magnetic chamber
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