⚛️Intro to Applied Nuclear Physics Unit 2 – Radioactivity and Nuclear Decay

Radioactivity and nuclear decay are fundamental processes in atomic physics. They involve unstable atomic nuclei emitting radiation, leading to the transformation of elements. Understanding these phenomena is crucial for applications in medicine, energy, and environmental science. This unit covers key concepts like types of radioactive decay, nuclear stability, and half-life. It also explores radiation detection, safety considerations, and practical applications. Calculations involving decay rates, activity, and dosimetry are essential skills in this field.

Key Concepts and Definitions

  • Radioactivity is the spontaneous emission of radiation from unstable atomic nuclei
  • Radioactive decay is the process by which an unstable atomic nucleus loses energy by emitting radiation
  • Isotopes are atoms of the same element with different numbers of neutrons in their nuclei
  • Radioisotopes are isotopes that undergo radioactive decay
  • Activity is the rate of decay of a radioactive substance, measured in becquerels (Bq) or curies (Ci)
    • 1 Bq = 1 decay per second
    • 1 Ci = 3.7 × 10^10 decays per second
  • Ionizing radiation is radiation with sufficient energy to ionize atoms or molecules, including alpha particles, beta particles, and gamma rays

Types of Radioactive Decay

  • Alpha decay involves the emission of an alpha particle (two protons and two neutrons) from the nucleus
    • Alpha particles have a positive charge and are relatively heavy
    • They have low penetrating power but high ionizing power
  • Beta decay involves the emission of a beta particle (an electron or positron) from the nucleus
    • Beta minus (β\beta^-) decay occurs when a neutron transforms into a proton, emitting an electron and an antineutrino
    • Beta plus (β+\beta^+) decay occurs when a proton transforms into a neutron, emitting a positron and a neutrino
  • Gamma decay involves the emission of a gamma ray (high-energy photon) from the nucleus
    • Gamma rays have no charge or mass and have high penetrating power
  • Electron capture is a process where an inner shell electron is captured by the nucleus, causing a proton to transform into a neutron
  • Spontaneous fission is the spontaneous splitting of a heavy nucleus into two smaller nuclei, releasing neutrons and energy

Nuclear Stability and Decay Rates

  • Nuclear stability depends on the ratio of protons to neutrons in the nucleus
    • Stable nuclei have a specific range of proton-to-neutron ratios
    • Nuclei with too many or too few neutrons are unstable and undergo radioactive decay
  • The nuclear binding energy is the energy required to break apart a nucleus into its constituent protons and neutrons
    • Nuclei with higher binding energies per nucleon are more stable
  • The decay rate is the number of radioactive decays per unit time
    • Decay rate is proportional to the number of radioactive nuclei present
  • The decay constant (λ\lambda) is the probability of a single atom decaying per unit time
    • λ=ln2t1/2\lambda = \frac{\ln 2}{t_{1/2}}, where t1/2t_{1/2} is the half-life

Radioactive Half-Life

  • The half-life (t1/2t_{1/2}) is the time required for half of a given quantity of a radioactive substance to decay
  • The number of radioactive nuclei remaining after a given time can be calculated using the exponential decay equation:
    • N(t)=N0eλtN(t) = N_0 e^{-\lambda t}, where N0N_0 is the initial number of nuclei and tt is the elapsed time
  • The activity of a radioactive sample decreases by half after each half-life
  • The mean lifetime (τ\tau) is the average time a radioactive nucleus exists before decaying
    • τ=1λ=t1/2ln2\tau = \frac{1}{\lambda} = \frac{t_{1/2}}{\ln 2}
  • Carbon-14 dating is a method for determining the age of organic materials based on the ratio of carbon-14 to carbon-12

Radiation Detection and Measurement

  • Geiger-Müller (GM) counters detect ionizing radiation by measuring the ionization of a gas in a sealed tube
    • GM counters are sensitive to alpha, beta, and gamma radiation
  • Scintillation detectors use materials that emit light when exposed to ionizing radiation
    • The light is then converted into an electrical signal by a photomultiplier tube
  • Semiconductor detectors (silicon or germanium) create electron-hole pairs when exposed to ionizing radiation
    • The number of electron-hole pairs is proportional to the energy of the incident radiation
  • Thermoluminescent dosimeters (TLDs) measure accumulated radiation dose using materials that emit light when heated after exposure to ionizing radiation
  • Radiation dose is measured in units of gray (Gy) or sievert (Sv)
    • 1 Gy = 1 joule of energy absorbed per kilogram of matter
    • 1 Sv = 1 joule of energy absorbed per kilogram of tissue, weighted by the biological effectiveness of the radiation type

Applications of Radioactivity

  • Medical imaging techniques use radioactive tracers to visualize internal structures and functions
    • Positron emission tomography (PET) uses positron-emitting radioisotopes to create 3D images of metabolic processes
    • Single-photon emission computed tomography (SPECT) uses gamma-emitting radioisotopes to create 3D images of organ function
  • Radiation therapy uses targeted ionizing radiation to destroy cancer cells
    • External beam radiation therapy (EBRT) delivers radiation from an external source
    • Brachytherapy involves placing radioactive sources directly inside or near the tumor
  • Radioisotopes are used as tracers in biological and environmental research to study processes such as nutrient uptake, gene expression, and pollutant transport
  • Radiocarbon dating is used to determine the age of organic materials by measuring the ratio of carbon-14 to carbon-12
  • Industrial radiography uses high-energy gamma rays to inspect materials for defects, such as cracks or voids in welds or castings

Safety and Environmental Considerations

  • Ionizing radiation can cause damage to living tissues, leading to health effects such as radiation sickness, cancer, and genetic mutations
  • The biological effects of radiation depend on the type and energy of the radiation, the dose received, and the sensitivity of the exposed tissue
  • The ALARA principle (As Low As Reasonably Achievable) is used to minimize radiation exposure to workers and the public
    • Time: Minimize the time spent in radiation areas
    • Distance: Maximize the distance from radiation sources
    • Shielding: Use appropriate shielding materials to reduce radiation exposure
  • Radioactive waste management involves the safe handling, storage, and disposal of radioactive materials
    • Low-level waste (LLW) has low concentrations of radioactivity and short half-lives
    • High-level waste (HLW) has high concentrations of radioactivity and long half-lives, requiring long-term isolation
  • Environmental monitoring is used to detect and quantify the presence of radioactive materials in air, water, soil, and biota
  • Nuclear accidents (Chernobyl, Fukushima) can release radioactive materials into the environment, leading to contamination and potential health risks

Calculations and Problem-Solving

  • Radioactive decay calculations involve determining the number of radioactive nuclei remaining after a given time or the time required for a specific fraction of the original nuclei to decay
    • N(t)=N0eλtN(t) = N_0 e^{-\lambda t}, where N0N_0 is the initial number of nuclei, λ\lambda is the decay constant, and tt is the elapsed time
    • t=ln(N0/N(t))λt = \frac{\ln (N_0/N(t))}{\lambda}, where N(t)N(t) is the number of nuclei remaining after time tt
  • Activity calculations involve determining the rate of radioactive decay or the number of radioactive nuclei present based on the activity
    • A(t)=λN(t)=A0eλtA(t) = \lambda N(t) = A_0 e^{-\lambda t}, where A0A_0 is the initial activity and A(t)A(t) is the activity after time tt
    • N(t)=A(t)λN(t) = \frac{A(t)}{\lambda}
  • Dosimetry calculations involve determining the absorbed dose, equivalent dose, or effective dose based on the type and energy of the radiation and the properties of the exposed material or tissue
    • Absorbed dose (Gy) = Energy absorbed (J) / Mass of material (kg)
    • Equivalent dose (Sv) = Absorbed dose (Gy) × Radiation weighting factor (WR)
    • Effective dose (Sv) = Σ (Equivalent dose to organ × Tissue weighting factor)
  • Shielding calculations involve determining the thickness of shielding material required to reduce the radiation dose to a specific level
    • I(x)=I0eμxI(x) = I_0 e^{-\mu x}, where I0I_0 is the initial radiation intensity, μ\mu is the linear attenuation coefficient of the shielding material, and xx is the thickness of the shielding


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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.