Describe key properties of alpha, beta, and gamma radiation
Write and balance equations of nuclear reactions; recognize symbols for protons, neutrons, electrons, positrons, alpha particles, beta particles, and gamma rays
Recognize a band of stability plot and predict decay type
Calculate half-life, radiochemical dating, and remaining amounts of radioisotopes
Deduce half-life from graphical representations
Calculate nuclear binding energy in MEV
Compare nuclear fission and fusion
Differentiate nuclear reactions from chemical reactions
Alpha Radiation (Symbol: a)
Composition: Helium nuclei (He)
Charge: 2+
Mass: 6.64 × 10⁻²⁷ kg
Energy: ~5 MeV
Penetrating Power: Blocked by paper
Beta Radiation (Symbol: β)
Composition: Electrons
Charge: 1-
Mass: 9.11 × 10⁻³¹ kg
Energy: 0.05 to 1 MeV
Penetrating Power: Blocked by metal foil
Gamma Radiation (Symbol: Y)
Composition: Photons
Charge: 0
Mass: 0
Energy: ~1 MeV
Penetrating Power: Not completely blocked by lead or concrete
In balanced nuclear equations, mass number and atomic number must equal on both sides.
Example:
Alpha Radiation: 238U → 234Th + 4He
Alpha Decay: Loss of He nucleus from heavy nuclei
Beta Decay: Conversion of a neutron to a proton and emission of a beta particle
Electron Capture: Nucleus captures an electron, converting a proton to a neutron
Positron Emission: Conversion of a proton to a neutron with emission of a positron
Stability is determined by the neutron-to-proton ratio (N/Z).
Points within the band of stability indicate stable nuclei; outside indicates instability and potential for different decay processes.
Half-life is the time required for half of a sample to decay.
Calculation Example: A = A0 × (1/2)ⁿ where n = number of half-lives.
Example for Radium-226 decay over 4800 years: 25 mg remaining after 3 half-lives.
Binding energy relates to the difference between the mass of nucleons and the mass of the nucleus.
Nuclear binding energy is the energy required to disassemble a nucleus into its constituent protons and neutrons.
Fission: Splitting of a large nucleus into lighter nuclei (e.g., U-235).
Fusion: Combining of light nuclei into a heavier nucleus (e.g., hydrogen into helium in stars).
Chemical Reactions | Nuclear Reactions |
---|---|
Involves breaking/formation of bonds | Involves changes in the nucleus |
Involves only valence electrons | Can involve protons, neutrons, electrons |
Small energy changes | Large energy changes |
Identity of atoms remains the same | Atoms can change into different elements |
Identify organic compounds by functional groups
Name substituted hydrocarbons
Classify reactions: substitution, addition, elimination, oxidation-reduction, condensation
Identify compounds by physical properties
Halocarbon: R-X (Halogen)
Alcohol: R-OH (Hydroxy)
Ester: R-C-O-R
Amine: R-NH2 (Amino)
Aldehyde: O=C
Carboxylic Acid: R-C(O)OH
Halocarbon: Named as substituents (e.g., chloro-, bromo-)
Alcohol: -ol suffix
Aldehyde: -al suffix, Ketone: -one suffix, Carboxylic acids: -oic suffix
Esters: Name alkyl group followed by carboxylic acid part’s name with "oate" suffix
Substitution: One atom/group replaces another
Addition: Atoms/groups added to unsaturated compounds
Elimination: Two groups removed, resulting in double bonds
Oxidation-Reduction: Involves electron loss/gain
Condensation: Two molecules combine with the loss of a small molecule (e.g., water)
Boiling point influenced by intermolecular forces (stronger forces = higher boiling points)
Solubility influenced by functional groups (e.g. hydroxyl groups in alcohols increase solubility).
### Summary:
Carboxylic acids have highest boiling points due to hydrogen bonding; lower for aldehydes and ketones.
Amines are basic in water; alcohols and acids display acidic behavior.