91Ó°ÊÓ

The spontaneous emission of radiation in the form of particles or high-energy photons as a result of a nuclear process is known as radioactivity.

With the help of the decay equation: A= 222 - 14= 208

Z=88 - 6 = 82

N = 134- 8 = 126

Then, the nuclide we will have is:\(_Z^A{X_N}{\rm{ }} = {\rm{ }}_{82}^{208}P{b_{126}}\).

Therefore, the nuclide is: \(_Z^A{X_N}{\rm{ }} = {\rm{ }}_{82}^{208}P{b_{126}}\).

To evaluate the changing in mass which leads to the emitted energy because of the decay, the following relation is used:

\(\begin{align}{}\Delta m{\rm{ }} &= {\rm{ }}{m_{Ra}} - {m_{Pb}} - {m_C}\\ &= {\rm{ }}222.0153\,{\rm{a}}{\rm{.m}}{\rm{.u}} - 207.9766\,{\rm{a}}{\rm{.m}}{\rm{.u}} - 14.0032\,{\rm{a}}{\rm{.m}}{\rm{.u}}\\ &= {\rm{ }}0.0355\,{\rm{a}}{\rm{.m}}{\rm{.u}}\end{align}\)

Then, according to Einstein mass/energy equation, we obtain:

\(\begin{align}{}E{\rm{ }} &= {\rm{ }}\Delta m{c^2}\\ &= {\rm{ }}0.0355\,{\rm{a}}{\rm{.m}}{\rm{.u }} \times {\rm{ }}931.5\,{\rm{MeV/u}}{{\rm{c}}^{\rm{2}}}{\rm{ }} \times {\rm{ }}{c^2}\\ &= {\rm{ }}33.0683\,{\rm{MeV}}\end{align}\)

Therefore, the energy emitted is: 33.0683 MeV.