: This is the energy required to hold the nucleus together. It is calculated using Einstein's mass-energy equation ,
Nuclear physics is essential to modern life, with diverse applications such as: Introductory Nuclear Physics
: The merging of light nuclei to form a heavier nucleus, the process that powers stars. Applications in Society : This is the energy required to hold the nucleus together
: The splitting of a heavy nucleus into smaller parts, releasing a massive amount of energy. releasing a massive amount of energy.
, which is significantly higher than bulk material densities.
, based on the "mass defect" (the difference between the mass of the nucleus and the sum of its individual components). Fundamental Interactions
: Responsible for specific radioactive processes, such as beta decay . Key Nuclear Processes