Nuclear Chemistry Study Guide: C19.1 & C19.3
1. Basics of Nuclear Chemistry
Nucleus: The dense center of an atom, contains protons (+) and neutrons (neutral).
Proton: Positive charge, ~1 amu.
Neutron: Neutral, ~1 amu.
Electron: Negative charge, negligible mass.
Atomic Number (Z): Number of protons → defines element.
Mass Number (A): Protons + neutrons.
Isotope: Same number of protons, different number of neutrons.
Check: Can you find protons, neutrons, electrons for any atom/isotope?
2. Nuclear Stability
Atoms are unstable if nucleus has too many or too few neutrons compared to protons.
Unstable nuclei emit radiation (particles & energy) to become more stable.
Factors affecting stability:
Ratio of neutrons to protons
Size of the nucleus (larger nuclei are more likely to decay)
3. Types of Radiation
Type | Symbol | Particle/energy | Mass | Charge | Penetration |
---|---|---|---|---|---|
Alpha | α | Helium nucleus (2p + 2n) | 4 | +2 | Low, stopped by paper/skin |
Beta (-) | β- | Electron from nucleus | 0 | -1 | Medium, stopped by thin metal |
Gamma | γ | Electromagnetic wave | 0 | 0 | High, needs lead/concrete |
Key:
Alpha decay → daughter nuclei are different elements, a type of fission reaction.
Beta decay → neutron → proton + electron; changes element.
Gamma decay → pure energy, no particle emission, often follows alpha/beta decay.
4. Nuclear Reactions
Nuclear Process: Involves change in the nucleus (protons/neutrons) → releases much more energy than chemical reactions.
Total nucleons (protons + neutrons) are conserved, but element may change.
Fission
A large nucleus splits into smaller nuclei + energy + neutrons.
Example: Uranium-235 + neutron → Barium-141 + Krypton-92 + 3 neutrons + energy
Fragments have fewer protons than original nucleus.
Used in nuclear reactors and atomic bombs.
Fusion
Two small nuclei combine to form a larger nucleus + energy.
Example: Hydrogen isotopes → Helium + energy (sun & hydrogen bombs).
Resulting nucleus has more protons than either original nucleus.
Requires high temperatures and pressures.
Energy:
Both processes release or absorb energy; huge compared to chemical reactions.
5. Radioactive Decay & Half-Life
Spontaneous nuclear reaction → unstable nucleus emits particle/energy.
Daughter nucleus: Product of decay.
Half-life (t½): Time it takes for half of a radioactive sample to decay.
Can calculate remaining atoms:
N=N0(12)t/t1/2N = N_0 \left(\frac{1}{2}\right)^{t/t_{1/2}}
Energy released can be kinetic (moving particles) or electromagnetic (gamma).
6. Vocabulary Connections
Absorption: Nucleus absorbs energy → may trigger fusion/fission.
Particle Emission: Release of alpha, beta, or other particles.
Nuclear Reactor: Device for controlled fission to produce energy.
Nonionizing Radiation: Radiation that doesn’t remove electrons (opposite of alpha, beta, gamma).
Nuclear Mass: Mass of the nucleus, slightly less than sum of parts (mass defect → energy release).
7. Quick Comparisons
Concept | Nuclear | Chemical |
---|---|---|
Energy change | Huge (hundreds of thousands to millions of times larger) | Small |
Particles changed | Protons/neutrons | Electrons |
Reaction location | Nucleus | Electron cloud |
Example | Fission, fusion, alpha decay | Combustion, acid-base reactions |