Binding Energy Per Nucleon Equation:
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Binding energy per nucleon is the average energy required to remove a nucleon from an atomic nucleus. It represents the nuclear stability, with higher values indicating more stable nuclei.
The calculator uses the binding energy per nucleon equation:
Where:
Explanation: The equation calculates the mass defect (difference between the mass of separated nucleons and the actual nuclear mass) and converts it to energy using Einstein's equation.
Details: Binding energy per nucleon helps understand nuclear stability, predict nuclear reactions, and explain energy release in nuclear fission and fusion.
Tips: Enter all values in atomic mass units (u). Default values are for Calcium-40 (Z=20, A=40). For other isotopes, adjust values accordingly.
Q1: Why is binding energy per nucleon important?
A: It shows how tightly nucleons are bound together, indicating nuclear stability and potential energy release in reactions.
Q2: What's the typical range for BE/A?
A: Most nuclei range from 7-9 MeV/nucleon, with iron-56 having one of the highest values (~8.8 MeV/nucleon).
Q3: Why does the curve peak at iron?
A: Iron-56 has the highest binding energy per nucleon, making it the most stable nucleus in terms of nuclear binding.
Q4: How does this relate to nuclear fusion and fission?
A: Both processes move nuclei toward the peak of the binding energy curve, releasing energy in the process.
Q5: What units are used in this calculation?
A: Masses are in atomic mass units (u) and the result is in mega-electron volts (MeV) per nucleon.