Overview of Specific Heat Capacity
Specific heat capacity is an important concept in thermodynamics representing the amount of heat required to change the temperature of a unit mass of a substance by one degree Celsius. This property varies among different gases based on their molecular structure, as understood through the law of equipartition of energy.
Monatomic Gases
For monatomic gases like helium, the internal energy at temperature T is derived using the principle of equipartition of energy. Since they possess only three translational degrees of freedom, the molar specific heat at constant volume (Cv) becomes:
Cv = (3/2)R
From this, we can derive the specific heat at constant pressure (Cp) using the relationship:
Cp = Cv + R = (5/2)R
The ratio of specific heats (γ) for monatomic gases is therefore:
γ = Cp/Cv = 5/3.
Diatomic Gases
Diatomic gases like O2 feature additional degrees of freedom due to rotation. Overall, they have five degrees – three translational and two rotational, leading to:
Cv = (5/2)R,
Cp = (7/2)R,
γ = 7/5.
At higher temperatures, if vibrational modes are considered, the specific heats increase, indicating more energy storage capacity.
Polyatomic Gases
Polyatomic gases have both rotational and vibrational modes contributing to even more kinetic energy storage. For these molecules, we find:
Cv = (3 + f)R, where f represents additional vibrational modes.
Conclusion
The specific heats align closely with experimental results, showcasing the relationship between molecular structure and thermal properties of gases.