Radioactive decay occurs when an unstable nucleus loses energy by emitting radiation. The three main types are:
Alpha Decay
Emits an alpha particle (2 protons and 2 neutrons; same as a helium nucleus)
Decreases atomic number by 2 and mass number by 4
Low penetration power; stopped by paper
Beta Decay
Emits a beta particle (an electron or positron)
A neutron changes into a proton (for decay) or a proton changes into a neutron (for decay)
Increases or decreases atomic number by 1 but does not change mass number
Moderate penetration power; stopped by aluminum foil
Gamma Decay
Emits a gamma ray (high-energy electromagnetic wave)
No change in atomic number or mass number
High penetration power; requires lead or thick concrete to stop it
Atoms are stable when the ratio of neutrons to protons (N/Z ratio) is within a certain range.
The belt of stability shows stable isotopes based on their neutron-to-proton ratio.
Elements with atomic numbers greater than 83 are typically radioactive.
Half-life: The time it takes for half of a radioactive substance to decay.
Formula:
As= initial amount
AE= remaining amount
t = total time elapsed
h = half-life duration
Example Problem:
A sample has a half-life of 10 years. If you start with 80g, how much remains after 30 years?
Nuclear Fission
Splitting of a heavy nucleus into smaller nuclei
Releases a large amount of energy
Used in nuclear power plants (e.g., uranium-235 fission)
Produces radioactive waste
Nuclear Fusion
Combining of two light nuclei to form a heavier nucleus
Releases even more energy than fission
Powers the sun and stars (e.g., hydrogen fusion into helium)
Requires extremely high temperature and pressure