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The work done by (or on ) a gas per mole...

The work done by (or on ) a gas per mole per kelvin is called

A

Universal gas constant

B

Boltizmann's constant

C

Gravitational constant

D

Entropy

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The correct Answer is:
To solve the question "The work done by (or on) a gas per mole per kelvin is called," we can follow these steps: ### Step 1: Understand the Concept of Work Done by Gas The work done by a gas during expansion or compression can be expressed mathematically as \( W = P \Delta V \), where \( P \) is the pressure and \( \Delta V \) is the change in volume. ### Step 2: Relate Work Done to the Ideal Gas Law We know the ideal gas law is given by the equation: \[ PV = nRT \] where: - \( P \) = pressure of the gas - \( V \) = volume of the gas - \( n \) = number of moles of the gas - \( R \) = universal gas constant - \( T \) = temperature in Kelvin ### Step 3: Work Done per Mole per Kelvin To find the work done per mole per Kelvin, we can rearrange the ideal gas law. The work done \( W \) can be expressed in terms of \( R \) when we consider one mole of gas: \[ W = P \Delta V = nRT \] For one mole of gas (\( n = 1 \)): \[ W = RT \] ### Step 4: Work Done per Mole per Kelvin To find the work done per mole per Kelvin, we divide the work done by the temperature \( T \): \[ \text{Work done per mole per Kelvin} = \frac{W}{T} = \frac{RT}{T} = R \] ### Conclusion Thus, the work done by (or on) a gas per mole per Kelvin is called the **universal gas constant \( R \)**. ### Final Answer The work done by (or on) a gas per mole per kelvin is called **R (Universal Gas Constant)**. ---

To solve the question "The work done by (or on) a gas per mole per kelvin is called," we can follow these steps: ### Step 1: Understand the Concept of Work Done by Gas The work done by a gas during expansion or compression can be expressed mathematically as \( W = P \Delta V \), where \( P \) is the pressure and \( \Delta V \) is the change in volume. ### Step 2: Relate Work Done to the Ideal Gas Law We know the ideal gas law is given by the equation: \[ PV = nRT \] ...
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