Concise Notes on Radiation and Nuclear Decay

Nuclear Decay

  • Process by which an unstable nucleus transforms into a more stable nucleus.
  • Energetic particles or electromagnetic radiation are emitted.
  • Random process; probabilities can be determined but not exact timing.
  • When a nucleus decays the atomic number, Z may change, when this happens the atom transforms from one element to another.
  • All elements with Z > 82 (lead) are radioactive
  • Three main types of radiation: alpha, beta, and gamma.

Alpha Radiation (\alpha)

  • Helium nuclei (two protons and two neutrons).
  • Positively charged (twice the electronic charge).
  • High kinetic energy (around 10% of the speed of light).
  • Strong ionizers, slowed rapidly by collisions.
  • When an atom emits alpha radiation:
    • Mass number, A, decreases by 4.
    • Atomic number, Z, decreases by 2.
  • Alpha decay equation: ^{A}{Z}X \rightarrow ^{A-4}{Z-2}Y + \alpha

Beta Radiation (\beta)

  • Electrons (\beta^{-}, e^{-}$) or positrons (\beta^{+}, e^{+}$).
  • Positron is the antiparticle of the electron.
  • Can be negatively or positively charged.
  • High speed (around 90% the speed of light).
  • Low mass, lose energy rapidly during collisions.
  • Formed in nuclear reactions when a neutron transforms into a proton or vice versa.
  • In \beta^{-}$ decay, an antineutrino is produced; in \beta^{+}$ decay, a neutrino is produced.
  • When an atom emits beta radiation:
    • Mass number stays the same.
    • Atomic number increases or decreases by 1.
  • \beta^{-}$ decay equation: ^{A}{Z}X \rightarrow ^{A}{Z+1}Y + \beta^{-} + \text{antineutrino}
  • \beta^{+} decay equation: ^{A}{Z}X \rightarrow ^{A}{Z-1}Y + \beta^{+} + \text{neutrino}

Gamma Radiation (\gamma)

  • Electromagnetic radiation (photons), no charge.
  • High end of the electromagnetic spectrum (high energy, high frequency).
  • When an atom emits gamma radiation:
    • Atomic number and mass number do not change.
    • The structure of the nucleus does not change, but its state of excitation does.
  • Gamma decay equation: ^{A}{Z}X^{*} \rightarrow ^{A}{Z}X + \gamma

Electron Capture

  • An electron is captured by the nucleus.
  • A proton changes to a neutron, and a neutrino is emitted.

Pair Production and Annihilation

  • Annihilation: When a particle and its antiparticle meet (e.g., an electron and a positron):
    • They annihilate, and mass converts to energy (E = mc^2).
    • Conservation laws are obeyed (charge, energy, momentum).
    • Two photons of equal energy are created to conserve momentum (about 511 keV).

Nuclear Decay Theory

  • The number of atoms which decay in a given time depends on the number of atoms present at the beginning of that time:
    • \frac{\Delta N}{\Delta t} \propto N
    • \frac{\Delta N}{\Delta t} = -\lambda N (where \lambda is the decay constant).
  • Exponential decay: N(t) = N_0 e^{-\lambda t}
    • N_0 is the number of radioactive atoms at the start.
    • \lambda is the decay constant.
  • Nuclear activity: A = \lambda N
    • A(t) = A_0 e^{-\lambda t}

Units of Nuclear Activity

  • Becquerel (Bq): 1 Bq = 1 disintegration per second (dps).
    • 1 Bq = 2.7 \times 10^{-11} Ci
  • Curie (Ci): Based on the decay rate of 1 g of radium.
    • 1 Ci = 3.7 \times 10^{10} dps

Half-Life (\tau_{1/2})

  • Time required for the amount of radionuclide to decrease to half the starting value.
  • The probability of decay is fixed, and the half-life is constant.
  • e^{-\lambda \tau_{1/2}} = \frac{1}{2}
  • \tau_{1/2} = \frac{\ln 2}{\lambda}
  • \lambda = \frac{0.693}{\tau_{1/2}}
  • N(t) = N0 \exp\left(-\frac{0.693t}{\tau{1/2}}\right)
  • A(t) = A0 \exp\left(-\frac{0.693t}{\tau{1/2}}\right)

Carbon Dating

  • Cosmic rays create neutrons, which interact with Nitrogen to create radioactive carbon-14 (^{14}C).
  • $^{14}C is radioactive with a half-life of 5730 years.
  • An equilibrium of 1 part $^{14}C to 10^{12} parts $^{12}C exists in living things.

X-Rays

  • Bremsstrahlung ("Braking radiation")
    • Electrons decelerate and emit energy as photons.
    • Maximum photon energy equals the kinetic energy gained by electrons.
  • Characteristic X-rays
    • Generated via inner-shell electron transitions.
    • Use Z_{eff} = (Z - 1) for energy calculations.
  • Crookes' Tube
    • Ions accelerate towards cathode, liberate electrons that generate X-rays upon hitting the glass face.
    • Tungsten is the best target material.
  • Coolidge or Thermionic Tubes
    • Heated filament emits electrons.
    • Electric field accelerates electrons, which strike the anode to generate X-rays.
    • Heat is generated in the target; large heat capacity required.
    • Independent control of current (beam intensity) and voltage (penetration ability).