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Nuclear Chemistry
Reactions
Chemical• Involve electrons• Affected external
factors (temp, pressure, catalyst)
Nuclear• Involve the nucleus• Release WAY more
energy• Not affected by
external factors
Electrostatic force
• Interaction between charged particles• Opposite charges attract• Same charges repel
How does the nucleus stay together?
Strong Nuclear Force
• Attractive force that acts between all nuclear particles that are extremely close together• Keeps the nucleus together• Much stronger than electrostatic force!
Radiation
• The emission (and transmission) of energy through space in the form of waves
Radioactivity
Alpha α
Beta β
Gama γ
Neutron n
Proton p
42
0-1
00
10
11
Radioactive
• Any element that spontaneously emits radiation (shows signs of radioactivity)• Transmutation—changing of an atom’s nucleus such
that an new element is formed• Alpha, beta, and proton not neutron or gamma
• Transuranium elements
Why does an element go undergo transmutation?
• The stability of the nucleus depends on the neutron to proton ratio
• Unstable nuclei are found outside the band of stability
• If a nucleus is unstable, it will emit radiation (decay) to gain stability
Radioactive decay
• Unstable nuclei (those that can be found outside the band of stability) losing energy by emitting radiation in a spontaneous process
Radioisotope
• Isotopes of atoms with unstable nuclei and go through radioactive decay to obtain a more stable nuclei• Small nuclei—up to 20 protons usually stable• Exception: Carbon—14
• Large nuclei—tend to be radioactive, based on the ratio of protons to neutrons; ALL nuclei with 83 protons or more are radioactive
Nuclear Equations
• In a balanced nuclear equation, mass numbers and atomic numbers are conserved• Example• Electron capture
Th Ra + He230 90
226 88
42
Rb + e → Kr 0- 1
8137
8136
Vocab for Equations
Word Location in the equation
Bombardment Reactant
Capture Reactant
Decay Product
Emission (emit) Product
Reactant Product
Practice
1. Zr e + ?
2. Po He + ?
3. ? Rn + He
4. Ca e + ?
5. Cm He + ?
0-1
218 84
4 2
222 86
97 40
4 2
0-1
47 20
4 2
244 96
Half-life
• Time required for ½ of a radioisotope’s nuclei to decay into its products
• Equation: NT = N0 (1/2)n
NT =Amount remaining at time T N0 = initial amountn= number of half-lives
Practice
1. Scientists start with 50.0 g sample of a radioisotope. How much is left after four half-lives?
Practice
2. Iron-59 is used in medicine to diagnose blood circulation disorders. The half-life of iron-59 is 44.5 days. How much of a 2.000 mg sample will remain after 133.5 days?
Carbon-14 Dating
• Carbon-14 is evenly spread in Earth’s biosphere• Carbon-14 is
radioactive and undergoes beta decay; half-life of 5730 years• Dates carbon-bearing
materials us to 62,000 years
Practice
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