Binding Energy
\[E_b=\Delta mc^2\]

Variables

Ebbinding energy (J)
dm[Δm]mass defect (kg)
cspeed of light in vacuum (m/s)

Description

What is this formula?


This formula calculates the nuclear binding energy from the mass defect of a nucleus using mass-energy equivalence. Binding energy represents the energy required to completely separate a nucleus into its constituent nucleons.


When to use it


Use this equation in nuclear structure studies, isotope stability analysis, fusion calculations, and nuclear energy problems.


Example


Given:


Δm=4×10^-30 kg


c=2.9979×10^8 m/s


Formula:


Eb=Δmc²


Substitution:


Eb=(4×10^-30)(2.9979×10^8)²


Result:


Eb=3.60×10^-13 J


Applications


- Nuclear stability analysis

- Fusion calculations

- Fission studies

- Nuclear structure analysis

- Energy calculations

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