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Binding Energy

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Physically, we define the binding energy as the positive work necessary to dissemble a nucleus into its constituents (nucleons). Equivalently  it is the energy liberated when Z proton and N neutrons combine to form a nucleus. For visualization, consider the simplest example of the deutron disintegration. The deutron atom H12 has a mass of 1.014102 a.m.u while the mass of the hydrogen atom that of the neutron H12 =   MH + MN

MH + MN   = (1.007825 + 1.008665) a.m.u

= 2.016490 a.m.u

But the observed mass of the H12 is 2.014102 a.m.u which is clearly 0.002388 a.m.u greater. It is obviously evident that a mass of 0.002388 a.m.u has been reduced. when a proton and a neutron are combine to constitute the nucleus of the deutron. A mass of 0.002388 a.m.u is equal to the Mev. This shows that when a deutron is formed for free proton and a neutron 2.23 Mev must be supplied from an external agency to dissammable a deutron into a proton and a neutron. This fact is supported by experiment in the photo disintegration of the deutron which shows that the gamma-ray photon must have energy of last 2.23 Mev to disrupt a neutron.

Since the binding energy equivalent of the mass reduction of the nucleons in the nucleus is a measure of the stability  of the nucleus and binding energies from the action of the forces which hold the nucleons together to form nuclei. Therefore the binding energy (B.E) of the nucleus in general can be written mathematically as follows:

B.E = Z MH  + (A-Z) MN – M = ΔM …………..(1)

Where MH and MN are the masses of the proton and the neutron and M is the atomic mass. Thus the mass difference in the above equation obviously appears amount of the binding energy on forming a nucleus. The same amount of the energy is required to separate the nucleons of the nucleus. It also appears that the actual mass of the nuclei is never equal to the sum of masses of its constitutions (proton + neutrons) with respect to the interior of the nucleus of the binding energy is difference between the mutual potential energy and the total kinetic energy of the constituents nucleons i.e

B.E  = P.E – K.E

The average binding energy per nucleon is obtained (from equation 1) by diving the total binding energy of the nucleus by the mass number A i.e

Average binding energy =B.E/A

Einstein’swell known energy relation E= Δmcshall we shall often need to use energy equivalent of 1 atomic mass unit, and we find it from

The nuclear Binding energy

 

This means that we can write Cas 931.5 Mev/u and can thus easily find energy equivalent in (Mev) of any mass or mass difference (in u) or conversely.

The main Features of Binding Energy

  • A +ve binding energy for all nuclei clearly shows that any nucleus is more stable that an unconnected assembly of its constituents neutrons and protons.
  • There is a rapid increase of binding energy per nucleon for the light nuclei with a notable peak at A = 4 (He4). This reflects the nucleon stability of alpha-particles structure.
  • Approximately the same binding energy per nucleon (7.3 Mev to 8.8 Mev) for all nuclei with A greater then 16 where A is atomic mass.

The broad maximum in the middle represents maximum stability from about A = 56 ( Fe) to about A = 140 ( Ce).

A gradual decrease in B.E/A from maximum to 7.3 Mev /A at A = 238 (U). Evidently the nuclei intermediate are the must stable, since the grater amount energy must be supplied to liberate each of their nucleons.

 

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