Monatomic Gases
Monatomic gases are characterized by having only three translational degrees of freedom. The average energy of these molecules at a given temperature (T) can be expressed as
\[ E = \frac{3}{2} k_B T \]
where \( k_B \) is the Boltzmann constant. Consequently, the total internal energy (U) of one mole of a monatomic gas is given by:
\[ U = 3 \cdot \frac{3}{2} k_B T N_A = \frac{3}{2} RT \]
where \( N_A \) is Avogadro's number and R is the gas constant. The molar specific heat at constant volume (\(C_v\)) is derived as follows:
\[ C_v = \frac{dU}{dT} = \frac{3}{2} R \]
For the relationship between the specific heats at constant pressure (\(C_p\)) and constant volume (\(C_v\)), we have:
\[ C_p - C_v = R \]
This leads to:
\[ C_p = \frac{5}{2} R \]
The ratio of specific heats for monatomic gases (denoted as \(\gamma\)) is:
\[ \gamma = \frac{C_p}{C_v} = \frac{5/2 R}{3/2 R} = \frac{5}{3} \]
This derivation illustrates the energy distribution laws across degrees of freedom in a thermodynamic context relevant for monatomic gases.