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An ideal gas ((C(p))/(C(v))=gamma)has in...

An ideal gas `((C_(p))/(C_(v))=gamma)`has initial volume `V_(0)` is kept in a vessel. It undergoes a change and follows the following relation `P = kV^(2)` (where `P` is pressure, and `V` is volume) find the change in internal energy of the gas if its final pressure is `P_(0)`:

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To solve the problem, we will follow a systematic approach to find the change in internal energy of the ideal gas under the given conditions. ### Step-by-Step Solution: 1. **Understanding the Relationship Between \( C_p \) and \( C_v \)**: We know that for an ideal gas, the ratio of specific heats is given by: \[ \frac{C_p}{C_v} = \gamma \] We also have the relation: \[ C_p = C_v + R \] From this, we can express \( C_v \) in terms of \( R \) and \( \gamma \): \[ \gamma = \frac{C_v + R}{C_v} \implies C_v(\gamma - 1) = R \implies C_v = \frac{R}{\gamma - 1} \] 2. **Internal Energy Formula**: The change in internal energy \( \Delta U \) for an ideal gas is given by: \[ \Delta U = n C_v \Delta T \] Substituting the expression for \( C_v \): \[ \Delta U = n \left(\frac{R}{\gamma - 1}\right) \Delta T \] 3. **Using the Ideal Gas Law**: The ideal gas law states: \[ PV = nRT \] Rearranging gives us: \[ nR = \frac{PV}{T} \] For a change, we can express this as: \[ \Delta(PV) = nR \Delta T \] 4. **Relating Pressure and Volume**: From the problem, we know that: \[ P = kV^2 \] Therefore, we can express the change in \( PV \) as: \[ \Delta(PV) = P_f V_f - P_i V_i \] where \( P_f \) and \( P_i \) are the final and initial pressures, and \( V_f \) and \( V_i \) are the final and initial volumes. 5. **Substituting Values**: Given that the final pressure \( P_f = P_0 \) and the initial pressure \( P_i = kV_0^2 \), we can write: \[ V_f = \sqrt{\frac{P_0}{k}} \] Therefore, substituting these values into the equation for \( \Delta U \): \[ \Delta U = \frac{\Delta(PV)}{\gamma - 1} = \frac{P_f V_f - P_i V_i}{\gamma - 1} \] 6. **Calculating \( \Delta U \)**: Now substituting the values: \[ \Delta U = \frac{P_0 \sqrt{\frac{P_0}{k}} - kV_0^2 V_0}{\gamma - 1} \] Simplifying this gives: \[ \Delta U = \frac{P_0^{3/2}/\sqrt{k} - kV_0^3}{\gamma - 1} \] ### Final Expression: Thus, the change in internal energy of the gas is: \[ \Delta U = \frac{P_0^{3/2}/\sqrt{k} - kV_0^3}{\gamma - 1} \]

To solve the problem, we will follow a systematic approach to find the change in internal energy of the ideal gas under the given conditions. ### Step-by-Step Solution: 1. **Understanding the Relationship Between \( C_p \) and \( C_v \)**: We know that for an ideal gas, the ratio of specific heats is given by: \[ \frac{C_p}{C_v} = \gamma ...
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