Binding Energy Per Nucleon Formula:
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Binding Energy Per Nucleon is the binding energy divided by the total number of nucleons in the nucleus. It represents the average energy required to remove a nucleon from the atomic nucleus and is a key indicator of nuclear stability.
The calculator uses the Binding Energy Per Nucleon formula:
Where:
Explanation: The formula calculates the average binding energy per nucleon by converting the mass defect to energy using Einstein's mass-energy equivalence principle and then dividing by the total number of nucleons.
Details: Calculating binding energy per nucleon is crucial for understanding nuclear stability, predicting nuclear reactions, and studying nuclear fusion and fission processes. Elements with higher binding energy per nucleon are more stable.
Tips: Enter mass defect in kilograms and mass number as a positive integer. Both values must be valid (mass defect > 0, mass number ≥ 1).
Q1: What is mass defect in nuclear physics?
A: Mass defect is the difference between the sum of masses of individual nucleons and the actual mass of the nucleus, representing the mass converted to binding energy during nucleus formation.
Q2: Why is 931.5 used in the formula?
A: 931.5 MeV/u is the conversion factor that relates atomic mass units to energy using Einstein's equation E=mc², where 1 u = 931.5 MeV.
Q3: What does binding energy per nucleon indicate?
A: It indicates the stability of a nucleus - higher values mean more stable nuclei. Iron-56 has the highest binding energy per nucleon, making it the most stable nucleus.
Q4: How is mass defect measured?
A: Mass defect is calculated by subtracting the measured atomic mass from the sum of masses of individual protons, neutrons, and electrons.
Q5: What are typical values for binding energy per nucleon?
A: Most nuclei have binding energy per nucleon values between 7-9 MeV. The maximum value of about 8.8 MeV occurs for iron-56 nuclei.