The mass density ( ρ) of a nucleus is defined as the ratio of its mass to its volume:
ρ= Mass of nucleus / Volume of nucleus
For a spherical nucleus with radius R , the volume is:
Volume =(4/3)πR3
The mass of the nucleus is related to the mass number A :
\text { Mass }-\mathrm{A} \times \mathrm{m} \text { _u }
(where m_u is the atomic mass unit, approximately 1.66×10−27 kg)
Therefore:
ρ=(A×m_u)/[(4/3)πR3]
Now, there's an important relationship between the mass number A and nuclear radius R. Empirically, it has been found that:
R=Ro∗ A∧(1/3)
Where Ro is a constant approximately equal to 1.2×10−15 m(1.2 fermi).
Substituting this into the density equation:
$\begin{aligned}
& \rho=\left(\mathrm{A} \times \mathrm{m} _\mathrm{u}\right) /\left[(4 / 3) \pi\left(\mathrm{Ro} \times \mathrm{A}^{\wedge}(1 / 3)\right)^3\right] \
& \rho=(\mathrm{A} \times \mathrm{m} \text { _u }) /\left[(4 / 3) \pi \mathrm{Ro}^3 \times \mathrm{A}\right] \
& \rho=\mathrm{m} _\mathrm{u} /\left[(4 / 3) \pi \mathrm{Ro}^3\right]
\end{aligned}$
This shows that the nuclear density is approximately constant for all nuclei, regardless of their mass number. This is a fundamental property of nuclear matter known as nuclear saturation density.
The numerical value is:
ρ=2.3×1017 kg/m3