1. Mass and Energy

2. The unified mass unit
The mass number of a nuclide refers to the number of protons and nucleons in an atom
Eg 1H 7Li U C etc
However 1 hydrogen nucleus is only approximately 1/238 the mass of a uranium nucleus. This is because some of the mass is lost as “binding energy” when larger nuclei form.
Therefore there is the need to define a unit of mass with which we can compare the masses of nuclei. This unit of mass is called the unified mass unit.

3. The unified mass unit
The unified mass unit is defined as 1/12 of the mass of a 12C atom.
(Iu = x 10-27kg)
The relative atomic mass (Ar) of any atom as a consequence of this is
Mass of the atom ÷ 1/12 mass of 12C atom

4. The mass energy relationship
According to the special theory of relativity mass has an energy equivalent. Any change in mass corresponds to a change in energy according to the equation
ΔE = c2Δm
Correspondingly any change in energy corresponds to a change in mass

5. The energy equivalent of u
Iu = x 10-27kg
ΔE = c2Δm
1u = (2.998 x 108)2 x x 10-27= x10-9J
Equivalently in eV
i.e. 932MeV
The unit MeV is often used as a measure of mass and this correctly emphasises the equivalence of mass and energy.

6. Mass Defect and Binding Energy
The mass of a nucleus is always less than the total mass of its constituent nucleons. ( this is called mass defect)
This is because the formation of a nucleus involves the conversion of some of the mass of the constituents to energy. This is released as gamma rays. It is called binding energy.
To separate the components would require the input of that same amount of energy.
The binding energy of a nucleus is the energy necessary to separate it into its component nucleons.

9. Mass of neutrons 2 x u
Mass of protons 2 x u
Mass of He nucleus u
Mass defect = (2 x x 1.007) – 4.002= 28.3MeV

10. Binding energy per nucleon
The binding energy per nucleon of a nucleus is a measure of the stability of a nucleus.(This is the binding energy divided by the mass number.)
The larger the binding energy per nucleon, the more stable the nucleus.

11. The nuclei at the top of the curve are most stable with the largest binding energy per nucleon. Those to the those nuclei to the left and right have less binding energy per nucleon

12. Atoms with low numbers of nucleons can become more stable by fusing together to become larger nuclei and in the process releasing binding energy.
Those to the right can achieve stability by becoming less massive by fission

13. Fission

14. A typical fissile material is uranium 235
A typical fissile material is uranium 235. This process occurs quite naturally in the material.
If enough nuclei are present (ie the mass is above “critical mass”) the fusion process becomes an uncontrollable chain reaction.

15. Fusion provides a much greater increase in binding energy per nucleon and therefore a much higher energy release per kg.