To represent beta decay, we use a nuclear equation where the sum of the mass numbers and atomic numbers must be balanced on both sides of the arrow.
The beta particle is written as an electron with a mass number of and an atomic number (charge) of : or {}^{0}_{-1}eta.
The general form of the equation is:
Step-by-step balancing: First, keep the top number (mass) the same. Second, add 1 to the bottom number (atomic number) to find the new element on the periodic table.
Beta radiation occupies a 'middle ground' in terms of physical properties when compared to alpha and gamma radiation.
| Property | Beta Particle | Alpha Particle | Gamma Ray |
|---|---|---|---|
| Composition | High-energy electron | 2 protons + 2 neutrons | EM Wave |
| Charge | |||
| Mass | Negligible (approx. ) | ||
| Penetration | Stopped by few mm Aluminium | Stopped by paper | Reduced by thick lead |
| Ionisation | Medium | High | Low |
Beta particles have a range in air of about one meter to a few meters, significantly further than alpha particles but much less than the infinite range of gamma rays.
The 'Plus One' Rule: Always remember that in beta decay, the atomic number goes UP by one. Students often mistakenly subtract one because the electron has a charge.
Mass Consistency: Ensure the mass number remains identical. If you change the mass number, you are likely describing alpha decay instead.
Shielding Identification: If an exam question describes radiation that passes through paper but is blocked by a thin sheet of metal (like aluminium), it is almost certainly beta radiation.
Conservation Check: Always verify that the total charge on the right side () equals the original charge () on the left side.