Chapter 23 Lecture Outline


Nuclear Chemistry

  1. Nuclear Particles
  2. NameSymbolSymbolMassCharge
    Alpha[alpha]4He4+2
    Beta[beta]1-e0-1
    Gamma[gamma] 00, radiation (light)
    Neutronn  10
    Protonp1H1+1
    Positron+1e+[beta]0+1

  3. Radioactivity and reactions
    1. Alpha emission: 238U -> 234Th + 4He

    2. Beta Emission:
      1. 14C -> 14N + -1e
      2. 1n -> 1p + -1e (neutron -> proton + electron)

    3. Positron Emission
      1. 11C -> 11B + +1e
      2. 1p -> 1n + +1e (proton -> neutron + positron)

    4. Electron Capture
      1. 40K + -1e -> 40Ar
      2. 1p + -1e -> 1n (proton + electron -> neutron)

  4. Nuclear Stability. Likelihood that isotope is radioactive depends upon:
    1. >83 protons are unstable
    2. Magic Numbers 2, 8, 20, 28, 50, 82 are stable. If magic number of both protons and neutrons, then "double magic"
    3. Even numbers of neutrons or protons are stable.
      1. Both even, most stable
      2. One even one odd, less stable
      3. both odd, least stable

    4. Belt of stability
      1. If above, then decay to convert a neutron to a proton.
      2. If below, then positron emission (or electron capture) to convert a proton to a neutron.

  5. Production of New Nuclei
    1. Particle accelerators
      1. Cyclotron (Figure 24.7, page 903)
      2. Linear Accelerator (Figure24.8, page 903)

    2. Induced Radioactivity (Making a radioactive isotope)
      1. 230Th + 1H --> 223Fr + 2 4He
    3. Neutron Bombardment (Use fast neutrons to prepare isotopes)
      1. 58Fe + 1n -> 59Fe
      2. 59Fe -> 59Co + -1e
      3. 59Co + 1n -> 60Co (Used for radiation treatment of cancer)

  6. Half life of radioactive isotopes
    1. Radioactive decay is first order
    2. First order rate law
      1. For half life t1/2 = 0.693/k
      2. Amount remaining after time t

  7. Uses of Radioactivity (See Mathcad)
    1. 238U Dating (Age of Rock Problem from Page 907)
      1. 238U -> 206Pb t1/2 = 4.5*109 years
    2. 40K Dating
      1. 40K + -1e -> 40Ar t1/2 = 1.3x109 years
    3. 14C Dating
      1. 14N + 1n -> 14C + 1H
      2. 14C -> -1e + 14N t1/2 = 5730 years
      3. Shroud of Turin (Dated at 1300 AD). Determine 14C present. What would it be if 0 AD?

    4. Radioactive Tracers and Labels
      1. P-32 Biochemical Systems


C&EN Paper on Heavy-Ion Research

  1. Discovery of New Elements, using traditional accelerators
    1. 96Mo + 2H -> 97Tc + 1n
    2. 230Th + 1H -> 223Fr + 2 4He
    3. 209Bi + 4He -> 210At + 3 1n

  2. Review Elements Created at GSI Institute
  3. REACTION DATE
    54Cr + 209Bi -> 262107 + n 2/81
    58Fe + 208Pb -> 265108 + n 3/84
    58Fe + 209Bi -> 266109 + n 9/82
    62Ni + 208Pb -> 269110 + n 11/94
    64Ni + 209Bi -> 272111 + n 12/94

  4. Elements 101 to 106
    1. When 1955 to 1974 at LLL and Dubna
    2. How Heavy element + light element (at high energy)

  5. Elements 107 to 111
    1. When 1980 to present
    2. How Two Medium size elements at lower energy
    3. Is this the same thing as "cold fusion" in the late 80's?

  6. For a typical experiment discussed:
    1. How many atoms of 111 were produced?
    2. How long did it take to do?
    3. How many moles is this?
    4. How much would all the 111 ever produced weigh?
    5. What is the half life for 272111? What is the rate constant?
    6. Why does the cross section effect how difficult the experiment is?
    7. Probability of a collision (1 mm2 in 1 km2)

  7. Beam Energy
    1. Enough to overcome coulomb barrier
    2. Not to much to cause fission

  8. How the experiment works
    1. Diagram of accelerator
    2. Make ions from a source metal (ie 64Ni9+ ions)
    3. Accelerate 1 species in heavy ion accelerator
    4. Second species is on rotating target (209Bi)
    5. Detection: Products are heavy, separate from primary beam by EB Sectors

  9. Why are they interested in 114
  10. From Your Textbook, Section 24.6
    1. Mass Defect for alpha partical 4He see Mathcad (pdf)
    2. Fission
    3. 235U + 1n -> 139Ba + 94Kr + 3 1n

    4. Fusion
    5. 2H + 3H -> 4He + 1n

    6. Calculating energy from Fusion
      1. Starting mass 2.0140 + 3.01605
      2. Final mass 4.0026031 + 1.008665012
      3. mass defect 0.018781 amu
      4. energy per mole reaction?

This page is maintained by
Scott Van Bramer
Department of Chemistry
Widener University
Chester, PA 19013

Please send any comments, corrections, or suggestions to svanbram@science.widener.edu.

This page has been accessed 1337 times since 5/30/97.
Last Updated Friday, May 25, 2001 1:59:43 PM