⚛️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.
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−) decay occurs when a neutron transforms into a proton, emitting an electron and an antineutrino
Beta plus (β+) 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) is the probability of a single atom decaying per unit time
λ=t1/2ln2, where t1/2 is the half-life
Radioactive Half-Life
The half-life (t1/2) 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)=N0e−λt, where N0 is the initial number of nuclei and t is the elapsed time
The activity of a radioactive sample decreases by half after each half-life
The mean lifetime (τ) is the average time a radioactive nucleus exists before decaying
τ=λ1=ln2t1/2
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)=N0e−λt, where N0 is the initial number of nuclei, λ is the decay constant, and t is the elapsed time
t=λln(N0/N(t)), where N(t) is the number of nuclei remaining after time t
Activity calculations involve determining the rate of radioactive decay or the number of radioactive nuclei present based on the activity
A(t)=λN(t)=A0e−λt, where A0 is the initial activity and A(t) is the activity after time t
N(t)=λA(t)
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)
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)=I0e−μx, where I0 is the initial radiation intensity, μ is the linear attenuation coefficient of the shielding material, and x is the thickness of the shielding