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Nuclear Chemistry

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Title: Nuclear Chemistry


1
Nuclear Chemistry
2
Chemical vs. Nuclear
  • Occurs when nuclei emit particles and/or rays
  • Atoms of one element are converted into another
    element
  • May involve protons, neutrons, or electrons
  • Have large energy changes
  • Reaction rates are not affected
  • Occurs when bonds are broken and formed
  • Atoms remain unchanged, but the may be rearranged
  • Involve only valence electrons
  • Have small energy changes
  • Reaction rates are influenced by temperature,
    pressure, concentration, and catalysts

3
Nuclear Forces
  • Nucleons- the protons and neutrons of the nucleus
  • Strong Force- the force that holds protons and
    neutrons together in the nucleus.

4
Nucleus
  • Protons and Neutrons can be broken down further
    into quarks.
  • When protons and neutrons come together to form
    the nucleus, energy is released called the
    nuclear binding energy.

5
Nucleus, cont
  • When parts of the atom combine, the total mass is
    less than the beginning mass. This is the Mass
    Defect.
  • The mass defect is the result of mass being
    converted to energy during the process.

6
Nucleus, cont
  • Einsteins equation E mc2 can be used to
    determine the binding energy for an atom.

7
Stability
  • Proton Neutron ratio
  • 1 or 1.5 ratio is stable
  • If atoms have atomic numbers larger than 83 or
    mass numbers greater than 209 they are unstable.
  • Remember proton the strong force has to do with
    the proton - neutron relationship.

8
Types of Radiation
  • Unstable nuclei emit radiation to attain more
    stable atomic configurations in a process called
    radioactive decay.
  • During radioactive decay, unstable atoms lose
    energy by emitting one of several types of
    radiation.

9
Types of Radiation
  • The three most common types of radiation are
    alpha (a), beta (ß), and gamma (?).

10
Alpha
  • An alpha particle (a) has the same composition as
    a helium nucleustwo protons and two neutronsand
    is therefore given the symbol 42 He .
  • The charge of an alpha particle is 2 due to the
    presence of the two protons.

11
Alpha
  • alpha particles are relatively slow-moving
    compared with other types of radiation.
  • Thus, alpha particles are not very penetratinga
    single sheet of paper stops alpha particles.

12
Beta
  • A beta particle (?) is a very-fast moving
    electron that has been emitted from a neutron of
    an unstable nucleus.
  • Beta particles are represented by the symbol
    0-1?.
  • The 1 subscript denotes the negative charge of
    the particle.

13
Beta
  • Because beta particles are both lightweight and
    fast moving, they have greater penetrating power
    than alpha particles.
  • A thin metal foil is required to stop beta
    particles.

14
Gamma
  • Gamma rays (?) are high-energy (short wavelength)
    electromagnetic radiation. They are denoted by
    the symbol 00?
  • The emission of gamma rays does not change the
    atomic number or mass number of a nucleus.
  • Gamma rays almost always accompany alpha and beta
    radiation.

15
Gamma
  • Gamma rays are high energy radiation
  • They can only be blocked by lead

16
Writing Nuclear Reactions
  • When writing nuclear reactions, you must remember
    the Law of Conservation of Matter
  • What you start with has to equal what you end
    with
  • You also have to remember how to write formulas
    for isotopes

17
Nuclear Reactions
  • Write the reaction for radium 226 converting into
    radon 222
  • Radium 226 is 22688Ra
  • Radon 222 is 22286Rn
  • Write the equation
  • 22688Ra ? 22286Rn
  • Now you must find what is missing
  • 22688Ra ? 22286Rn 42He

18
Nuclear Reactions
  • Write the reaction of carbon-14 decaying into
    nitrogen 14
  • 146C ? 147N
  • Now see whats missing
  • Only add to the product side
  • 146C ? 147N 0-1?

19
Nuclear Reactions
  • Write the reaction of uranim-238 undergoing alpha
    and gamma decay
  • 23892U ? 42He 00?
  • Now put whats left
  • 23892U ? 42He 00? 23490Th

20
Half Life
  • Half life - time required for ½ of a radioisotope
    to decay
  • For example
  • You have 100 g of an isotope. How much is left
    after 1 half life?
  • 50g
  • How much will be left after 2 half lifes?
  • 25g

21
Carbon -14 Dating
  • A process of using radioactive decay of C-14 to
    measure the age of artifacts/remains of once
    living organisms.
  • C-14 undergoes beta decay to form N-14

22
Fission and Fusion
  • Fission splitting the nucleus into fragments
  • Releases large amounts of energy
  • Nuclear power plants use fission to generate power

23
Fission and Fusion
  • Fusion combining of atomic nuclei
  • Release large amounts of energy
  • Require extremely high temperatures
  • The lowest temperature possible is 40,000,000 K
  • Known to occur on the sun

24
Nuclear Waste
  • Nuclear waste is spent fuel that can no longer
    be used to create energy.
  • This material is still radioactive and must be
    disposed of with care.

25
Units for Radioactivity
  • Curie (C) radioactive decay
  • Rad (rad) energy absorbed by ionizing radiation
  • Rem (rem) biological effect of the absorbed
    dose in humans.
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