1. BANGLADESH ARMY INTERNATIONAL UNIVERSITY
OF SCIENCE AND TECHNOLOGY
DEPARTMENT OF EEE
PRESENTATION
ON
BINDING ENERGY
Presented by: Kamruzzaman
Rakib
Group: B Level: 1; Term: 2
2. Binding Energy
Definition: Binding energy is the energy
required to break a whole system into separate
parts.
Nuclear Binding Energy:
Nuclear binding energy is the energy that
would be required to disassemble or break the
nucleus of an atom into its component parts.
These components parts are neutrons and
protons. Which are collectively called
“nucleons”.
3. Simple Figure
Fig1: Energy required
for
Creating a nucleus.
Fig2: Energy required
for
Breaking up a nucleus.
4. Binding Energy
Now,
Let mn and mp be the masses of the neutron and
the proton. M = Zmp+ Nmn.
The mass defect m = Zmp+ Nmn – M(A, Z)
The energy equivalent to mass defect is,
E = (m)c2
= (m)×931.49 MeV/u
5. Binding Energy
Here,
X- Chemical Symbol
Z- Atomic no. = no. of proton
A- Mass no.= proton+ neutron
N- Neutron no.
6. Binding Energy
The B.E. of the Oxygen:
B. E= 8mn + 8mp – M
= (8*1.00866 +8* 1.00782 –15.9994 ) amu
= (8.0692+8.0625- 15.9994
= 0.1323*931.49 MeV
=123.23 MeV
8. Bindin
This plot shows the amount of binding
energy per nucleon (A nucleon is either a
neutron or a proton. The nucleon number
is the sum of the number of neutrons plus
protons in a nucleus; thus, it is equal to the
atomic mass number)
This curve indicates how stable atomic
nuclei are; the higher the curve the more
stable the nucleus. Notice the
characteristic shape, with a peak near
A=60. These nuclei are the most stable in
the Universe.
Binding Energy Curve