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