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Radioactive decay is a natural process where unstable atomic nuclei lose energy by emitting radiation in the form of particles or electromagnetic waves. This process transforms the original atom into a different element or isotope, continuing until a stable configuration is reached.
Emission of helium-4 nuclei (2 protons + 2 neutrons). Reduces atomic number by 2 and mass number by 4.
Conversion of neutron to proton (β⁻) or proton to neutron (β⁺). Changes atomic number by ±1.
High-energy electromagnetic radiation. No change in atomic or mass number, only energy release.
Half-life (t₁/₂) is the time required for exactly half of a radioactive sample to decay. This is a probabilistic measure that becomes highly accurate for large numbers of atoms. The half-life is constant for each isotope, regardless of the sample size or external conditions.
Key Insight: The time for decay from 100% to 50% is the same as from 50% to 25%, demonstrating the exponential nature of radioactive decay.
The stability of atomic nuclei depends on the balance between the strong nuclear force (which holds protons and neutrons together) and the electromagnetic force (which causes protons to repel each other). This balance determines whether an isotope is stable or radioactive.
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Essential terms and definitions for radioactive decay and nuclear physics
Avoid these frequent errors when working with half-life calculations
Mistake: Mixing time units (years with seconds)
Solution: Always convert to consistent units before calculation
Mistake: Using log₁₀ instead of natural log (ln)
Solution: Use ln for exponential decay: λ = ln(2)/t₁/₂
Mistake: Using 85% instead of 0.85 in calculations
Solution: Convert percentages to decimal form
Mistake: Using positive exponent for decay
Solution: Always use negative exponent: e^(-λt)
Comprehensive resources for deeper understanding of radioactive decay and nuclear physics
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Common questions about half-life calculations and radioactive decay
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