To solve this, we need to calculate the entropy changes for both the free expansion and the isothermal expansion.
Step 1: Entropy Change for Free Expansion (\( \Delta S_1 \))
For free expansion, the process is irreversible, and since the gas expands into a vacuum, there is no heat exchange with the surroundings. Therefore, the entropy change \( \Delta S_1 \) for the gas during free expansion is given by: \[ \Delta S_1 = nR \ln \left( \frac{V_f}{V_i} \right), \] where \( V_f \) and \( V_i \) are the final and initial volumes of the gas, respectively, and \( n \) is the number of moles. Since the volume doubles, \( \frac{V_f}{V_i} = 2 \), and we get: \[ \Delta S_1 = nR \ln(2). \] Step 2: Entropy Change for Isothermal Expansion (\( \Delta S_2 \))
For the isothermal expansion, the process is reversible, and the gas is at a constant temperature. The entropy change \( \Delta S_2 \) for the gas during an isothermal expansion is given by: \[ \Delta S_2 = nR \ln \left( \frac{V_f}{V_i} \right), \] where \( V_f \) and \( V_i \) are the final and initial volumes of the gas, respectively. Since the volume also doubles in this case, \( \frac{V_f}{V_i} = 2 \), and we get: \[ \Delta S_2 = nR \ln(2). \] Step 3: Comparing the Two Entropy Changes.
We are asked to find the ratio \( \frac{\Delta S_1}{\Delta S_2} \). Since both entropy changes are equal: \[ \frac{\Delta S_1}{\Delta S_2} = \frac{nR \ln(2)}{nR \ln(2)} = 1. \] Thus, the value of \( \frac{\Delta S_1}{\Delta S_2} \) is \( 1 \).
A wheel of mass \( 4M \) and radius \( R \) is made of a thin uniform distribution of mass \( 3M \) at the rim and a point mass \( M \) at the center. The spokes of the wheel are massless. The center of mass of the wheel is connected to a horizontal massless rod of length \( 2R \), with one end fixed at \( O \), as shown in the figure. The wheel rolls without slipping on horizontal ground with angular speed \( \Omega \). If \( \vec{L} \) is the total angular momentum of the wheel about \( O \), then the magnitude \( \left| \frac{d\vec{L}}{dt} \right| = N(MR^2 \Omega^2) \). The value of \( N \) (in integer) is: