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Inorganic and Applied Chemistry
Example 1- D:
Mass and energy (Einstein equation)
From a thermodynamic point of view the stability of an atomic nucleus means that in terms of energy it is
favourable for the nucleus to exist as a whole nucleus rather than split into two parts or (hypothetically
thinking) exist as individual neutrons and protons. The thermodynamic stability of a nucleus can be
calculated as the change in potential energy when individual neutrons and protons join and form a nucleus.
As an example we are going to look at the tin isotope tin-118. Tin is element number 50 and thus this
isotope contains 50 protons and 118 – 50 = 68 neutrons in the nucleus. In order to calculate the change in
energy when the nucleus is “formed” we first have to determine the change in mass when the following
hypothetic reaction occurs:
5011 p 68 01 n 11850 Sn
The mass on the right side of this reaction is actually not the same at the mass on the left side. First we will
look at the masses and change in mass:
Mass on left side of the reaction:
Mass 5011 p 6801 n 501. 6726210
27 kg 681. 6749710
27 kg 1. 9752610
25 kg
Mass on right side of the reaction:
kg
mol
kg mol
Mass Sn 23 1 25
118 3
(^506). 022 10 1.^9578510
117. 9016010 /
Change in mass when reaction occurs (tin-118 formation):
Masschange 1. 9578510
25 kg
- 9578510
25 kg - 7414510
27 kg
It is thus seen that when the reaction occurs and the tin-118 nucleus is formed, mass ”disappears”. This
change in mass can be inserted into the famous Einstein equation (equation (1- 3) on page 18) and the
change in potential energy can be calculated.
E kg m s J
E m c
27 8 2 10
2
- 7414510
310 / - 610
It is seen that the “disappeared” mass has been converted into 1.6 10 -10 Joules which then are released.
This corresponds to 980 MeV (1 Mega electron Volt corresponds to 1.60 10 -13 J). This amount of energy
can be translated into an amount of energy pr. nucleon:
Atoms