Unstable nuclei spontaneously transform to lower-energy configurations through radioactive decay. Alpha decay emits a helium-4 nucleus (2 protons + 2 neutrons), reducing mass number by 4 and atomic number by 2; it occurs in heavy nuclei and proceeds via quantum tunneling through the Coulomb barrier. Beta-minus decay converts a neutron to a proton with emission of an electron and antineutrino; beta-plus decay converts a proton to a neutron with emission of a positron and neutrino. Gamma decay releases excess nuclear energy as a high-energy photon with no change in nucleon number. Each decay mode conserves charge, lepton number, and mass-energy.
Write out balanced decay equations for representative nuclides (Ra-226, C-14, Co-60). Verify conservation laws. Distinguish the penetrating power of each radiation type (alpha: blocked by paper; beta: by aluminum; gamma: requires lead/concrete).
You know from nuclear structure that a nucleus is held together by the strong nuclear force competing against electromagnetic repulsion between protons. Not all combinations of protons and neutrons form stable nuclei — those that are too heavy, too neutron-rich, or too proton-rich will spontaneously reorganize to reach a lower-energy state. This spontaneous reorganization is radioactive decay.
There are three main decay modes, each addressing a different kind of nuclear instability. Alpha decay occurs in very heavy nuclei (typically Z > 82) where the nucleus is simply too large for the strong force to hold together stably. It ejects a helium-4 nucleus (two protons, two neutrons), reducing the mass number by 4 and atomic number by 2. Crucially, the alpha particle can only escape by *tunneling* through the Coulomb energy barrier — it does not have enough energy to classically surmount the barrier, but quantum mechanics allows a finite probability of it appearing on the other side. This is quantum tunneling applied directly.
Beta decay addresses a wrong ratio of neutrons to protons. In beta-minus decay, a neutron converts to a proton via the weak nuclear force, emitting an electron and an antineutrino. In beta-plus decay, a proton converts to a neutron, emitting a positron and a neutrino. A common misconception is that the electron was somehow stored in the nucleus — it was not. The electron is created from the energy released by the mass difference between the original neutron and the resulting proton plus electron. Conservation of lepton number requires the antineutrino to accompany the electron.
Gamma decay is different in character: no particles are emitted, only a high-energy photon. After alpha or beta decay, the daughter nucleus often remains in an excited energy state. It sheds this excess energy as a gamma ray, transitioning to its ground state. Nothing about the nuclear composition changes — the atomic number and mass number are the same before and after.
All three modes obey strict conservation laws: charge, mass-energy, lepton number, and baryon number are all conserved in every decay. Writing balanced decay equations — verifying that the numbers on both sides match — is the most reliable way to check your understanding of each mode.