Mass-energy equivalence is a fundamental concept introduced by Albert Einstein, described by the famous equation \(E=mc^2\). This equation tells us that mass can be converted into energy and vice versa.
In the context of binding energy calculations, the mass defect calculated from the isotopes can be used to find the energy released or required to hold that nucleus together.
To convert the mass defect into energy:
- Multiply the mass defect by the speed of light squared (\(c^2\)).
This results in energy typically expressed in MeV (mega-electronvolts), a convenient unit in nuclear physics. Understanding mass-energy equivalence is crucial in explaining why nuclear reactions release such large amounts of energy.