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Understanding Nuclear Chemistry and Radioactivity

Apr 28, 2025

Chapter 21: Nuclear Chemistry

21.1 Radioactivity and Nuclear Equations

Review of Isotopes

  • Mass Number: Total number of protons and neutrons.
  • Atomic Number: Number of protons.
  • Nucleus contains:
    • Protons: +1 charge
    • Neutrons: No charge

Isotopes

  • Atoms of the same element with different masses due to different numbers of neutrons.
  • Example: Uranium isotopes - Uranium-234, Uranium-235, Uranium-238.
  • Radioactive nuclei emit radiation and are called radionuclides.

Nuclear Equations

  • Nuclear Reactions: Affect the nucleus, must balance atomic and mass numbers, unlike chemical reactions.

Properties of Radioactive Decay

  • Types of Radiation:
    • Alpha (α): Charge +2, low penetration, helium nucleus.
    • Beta (β): Charge -1, more penetration, high-speed electrons.
    • Gamma (γ): No charge, high penetration, high-energy photons.

Types of Decay

  • Alpha Decay: Loss of an alpha particle (He nucleus).
  • Beta Decay: Loss of a beta particle (electron).
  • Gamma Decay: Loss of a high-energy photon, often accompanies other decays.
  • Positron Emission: Proton converts to neutron, positron emitted.
  • Electron Capture: Electron absorbed by the nucleus, converts proton to neutron.

Nuclear Reaction Changes

  • Beta Emission: Neutron to proton.
  • Positron Emission & Electron Capture: Proton to neutron.

21.2 Patterns of Nuclear Stability

Stability Forces

  • Strong Nuclear Force: Binds nucleus despite proton-proton repulsion.
  • Balance of protons and neutrons is key.

Stability Indicators

  • Proton/Neutron Ratio: 1:1 for smaller nuclei, more neutrons needed for larger nuclei.
  • Belt of Stability: Represents stable nuclides.
  • Unstable Nuclei:
    • Above belt: Too many neutrons, decay by beta emission.
    • Below belt: Too many protons, decay by positron emission or electron capture.
    • Large atomic numbers (>83): Alpha decay.

Radioactive Decay Chains

  • Series of decays required to reach a stable nuclide, often ending in lead.

"Magic Numbers" for Stability

  • Certain numbers of protons/neutrons provide extra stability, favoring even numbers.

21.3 Nuclear Transmutations

Nuclear Transmutations

  • Occur when nuclei collide with other particles (e.g., nuclei or neutrons).

Particle Accelerators

  • Linear accelerators, cyclotrons, synchrotrons used to speed up particles for collisions.

Creation of Synthetic Isotopes

  • Neutrons used for creating isotopes for medical use.
  • Transuranium elements (>92) created by bombarding with neutrons.

21.4 Kinetics of Radioactive Decay

Decay Kinetics

  • First-order processes.
  • Half-Life: Time for half a sample to decay.

Radiometric Dating

  • Uses decay information to date objects, e.g., carbon dating (C-14).

Measuring Radioactivity

  • Units: Becquerel (Bq), Curie (Ci).

Detection Methods

  • Film badges, Geiger counters, scintillation counters.

Medical Applications

  • Radiotracers: Used in diagnostics (e.g., PET scans).

21.5 Energy Changes in Nuclear Reactions

Mass-Energy Equivalence

  • E=mc²: Mass defect contributes to nuclear binding energy.

Fission vs Fusion

  • Fission: Splits heavy nuclei, releases energy.
  • Fusion: Combines light nuclei, requires high energy, releases more energy.

21.7 Nuclear Power

Fission Power

  • Nuclear reactors use controlled fission to generate energy.
  • Components: Fuel rods, control rods, coolant.

Fusion Power

  • Produces no radioactive by-products, requires extreme conditions.

21.9 Radiation in the Environment

Ionizing Radiation

  • Causes radical formation, affects DNA/RNA.

Biological Impact

  • Type and location of exposure determine damage severity.
  • External vs internal radiation risks.

Radiation Dose Measurement

  • Units: Gray (Gy), Rad.
  • Biological effectiveness measured by RBE (relative biological effectiveness).

Short-Term Exposure Effects

  • Ranges from no effect to fatal, depending on dose (rem).