Step 1: Definition of \( r_1 \) and \( r_2 \).
For a gas, the ratio \( r = \frac{c_p}{c_v} \),
where:
- \( c_p \) is the specific heat at constant pressure,
- \( c_v \) is the specific heat at constant volume.
Step 2: Value of \( r_1 \) for a rigid diatomic gas.
For a rigid diatomic gas, \( r_1 = \frac{c_p}{c_v} = \frac{7}{5} \). This is because the degrees of freedom for a rigid diatomic gas are 5 (3 translational and 2 rotational), and using the ideal gas law:
\[
r_1 = 1 + \frac{2}{f} = 1 + \frac{2}{5} = \frac{7}{5}
\]
Step 3: Value of \( r_2 \) for a non-rigid diatomic gas.
For a non-rigid diatomic gas, the number of degrees of freedom increases because the molecule can undergo vibration as well. The specific value of \( r_2 \) depends on the exact nature of the gas, but for most practical cases, it is approximately:
\[
r_2 = \frac{9}{7}
\]
This is because for non-rigid diatomic gases, the number of degrees of freedom is 7 (3 translational, 2 rotational, and 2 vibrational), and the corresponding ratio \( r \) is:
\[
r_2 = 1 + \frac{2}{7} = \frac{9}{7}
\]