Lecture 5: Natural Radioactivity
Natural Radioactivity
Introduction to Natural Radioactivity
Nucleogenesis produces nuclides which can be either stable or unstable.
Unstable nuclei decay through various mechanisms involving the release of high kinetic energy particles or gamma (γ) radiation.
High-energy products of these processes are referred to as radioactivity.
Major Radioactive Decay Mechanisms
Alpha (α) Decay
General Equation Representation:
{}^{212}{83}Bi ightarrow {}^{4}{2}He + {}^{208}_{81}TlDefinition: α decay is the process in which an α particle, basically a helium nucleus, is emitted from a parent nucleus.
Key Features of α Particle:
Mass = 4
Charge = 2+
This decay is exemplified by uranium-238:
{}^{238}{92}U ightarrow {}^{4}{2}He + {}^{234}_{90}Th
In this reaction, uranium transmutates into thorium, emitting an α particle.
Characteristics of α Particle:
Symbol: {}^{4}_{2}He
Composition: 2 protons and 2 neutrons (total mass number of 4).
Another example of α decay is thorium-230: {}^{230}_{90}Th .
Beta (β) Decay
Definition: β (or β-) is an electron emitted from the nucleus as a result of nuclear decay where one neutron is converted into a proton to balance charge.
Example General Equation:
{}^{12}{5}B ightarrow {}^{12}{6}C + {}^{0}_{-1}eKey Features:
β particle is essentially an electron that balances nuclear charge post decay.
Positron Emission (β+)
Definition: A positron (β+) is emitted from the nucleus when a proton is converted into a neutron.
General Equation Example:
{}^{12}{7}N ightarrow {}^{12}{6}C + {}^{0}_{+1}eAntiparticle Interaction: Positron often collides with an electron leading to annihilation:
e^{+} + e^{-}
ightarrow ext{γ-rays}
Electron Capture
Definition: This involves a nucleus capturing an electron leading to a decrease in atomic number, often followed by emissions of x-rays.
Characteristics: X-rays are produced as other electrons transition to fill the vacancy left by the captured electron.
Note: X-rays are not typically classified as radioactivity, though they can cause radiation damage.
Nuclear Equation Considerations
To ensure proper atomic equations when inserting electrons:
Assigned mass number for an electron is zero (0).
Assigned atomic number for an electron is negative one (-1).
Representation of a beta particle (electron):
{}^{0}_{-1}eExample of Beta Decay:
{}^{234}{90}Th ightarrow {}^{0}{-1}e + {}^{234}_{91}Pa
Gamma Radiation
Gamma rays are frequently emitted during nuclear reactions.
Example during U-238 decay:
{}^{238}{92}U ightarrow {}^{4}{2}He + {}^{234}{90}Th + 2 imes {}^{0}{0} ext{γ}
Additional gamma rays of various energies accompany the decay process.
Nuclear Stability
Factors affecting nuclear stability include:
Size of the nucleus
Composition of the nucleus (proton/neutron ratio) or N/P ratio.
Observations on Stable Nuclides:
All known stable nuclides exist in a zone of stability.
Zone is approximately where the N:Z ratio is close to 1, bending towards more neutrons as nucleus size increases.
Stability Rule:
Unstable isotopes decay towards the zone of stability and stabilize below {}^{209}_{83}Bi .
Periodic Table Observation:
The periodic table shows a band of stable isotopes including radioactive elements from lanthanides and actinides.
Graphical Representation of Decaying Isotopes
Radioactive decay sequences illustrated graphically show atomic number vs neutron number:
Alpha Decay: Decrease of two protons (Z) and two neutrons (N).
Beta Decay: Decrease of one neutron and increase of one proton.
Isotopes (same Z, different N) are depicted along vertical lines in the graph.
Example: Uranium-238 generates a family of daughter isotopes via decay series.
Radio Nuclides in Nature
Definition of Radio Nuclides:
Radioactive isotopes are present in the environment as a result of natural nuclear reactions or anthropogenic contamination.
1. Primary Radio Nuclides
Definition: Long-lived radio nuclides formed through nucleogenesis referred to as primary or primordial radio nuclides.
Characteristics:
About 20 primary radio nuclides exist, challenging to detect due to:
Long half-lives (T > 10^{10} years).
Isotopic abundance potentially below 1%.
Low energy emissions of alpha and beta particles.
Gamma photons being highly converted.
Implications:
They are often treated as stable nuclides in elemental isotopic compositions.
Example: Potential existence of primary 244Pu.
2. Isotopic Composition and Atomic Weights of Primary Radio Nuclides
Consequence of long-lived primary radio nuclides: progressive nucleogenesis of stable elements originated at the Big Bang.
Formation timeline:
Hydrogen as the oldest element formed.
Most elements formed approximately 5 imes 10^{9} years ago.
Continuous decay of parent nuclides alters isotopic composition and atomic weights over time.