Neutron-rich unstable nuclides have an excess of neutrons, making them unstable. To achieve stability, they undergo β⁻ (negatron) decay.
In β⁻ decay, a neutron (\( n \)) is converted into a proton (\( p \)), emitting an electron (\( e^- \)) and an antineutrino (\( \bar{\nu}_e \)):
\[ n \rightarrow p + e^- + \bar{\nu}_e \]
Since a neutron is converted into a proton, the atomic number (\( Z \)) of the nuclide increases by 1, but the mass number (\( A \)) remains unchanged.
Consider the beta decay of carbon-14:
\[ {}^{14}_6C \rightarrow {}^{14}_7N + e^- + \bar{\nu}_e \]
Here, carbon-14 (\( ^{14}_6C \)) transforms into nitrogen-14 (\( ^{14}_7N \)), increasing its atomic number while keeping the mass number constant.
β⁻ decay is a fundamental nuclear process that allows neutron-rich nuclides to move toward a stable configuration by converting excess neutrons into protons.