TABLE OF CONTENTS
BINDING ENERGY PER NUCLEON
INTRODUCTION
The binding energy per nucleon represents the average amount of energy required to remove one nucleon from the nucleus.Binding energy per nucleon is an atomic nucleus stability measurement that explains why some elements are more stable than others.Higher binding energy per nucleon nuclei are more stable and need more energy to disintegrate.It may be used to calculate how much energy is emitted during a nuclear reaction.
Scientists may measure the energy release and efficiency of nuclear processes by estimating the binding energy per nucleon, which aids in the design and optimization of nuclear power plants.This section will explain how to compute binding energy per nucleon.
NUCLEAR BINDING ENERGY-IMAGE

MASS DEFECT
The complete mass of a core(nucleus) is not exactly the all out mass of the nucleons that make up the core(nucleus). This is known as a mass defect.
According to Einstein’s extraordinary hypothesis of relativity, mass is the proportion of the complete energy of a framework.

ATOMIC BINDING ENERGY
The base energy(minimum energy)would be needed to dismantle the core of a molecule into its constituent protons and neutrons.(see the picture)
Larger binding energy per nucleon implies more prominent work is needed to eliminate the nucleons from the core(nucleus). Binding energy is an action the solidness(stability) of the core(nucleus).
BINDING ENERGY PER NUCLEON
Binding energy per nucleon is dictated by isolating(dividing) the absolute binding energy per mass number.

NUCLEAR BINDING ENERGY CURVE

HOW TO CALCULATE BINDING ENERGY PER NUCLEON?
BINDING ENERGY PER NUCLEON FOR CHLORINE NUCLEUS


BINDING ENERGY PER NUCLEON FOR CALCIUM NUCLEUS

BINDING ENERGY PER NUCLEON FOR HELIUM NUCLEUS

CONCLUSION
Calculating the binding energy per nucleon gives vital insight into the behavior, stability, and energy release of atomic nuclei, allowing for improvement in a variety of scientific and technical domains.It has several uses in nuclear power plants, nuclear weapons, nuclear energy, cosmology, medical imaging, astronomy, and basic research.

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