
Ideal Gas Equation and Density Relationship:
For an ideal gas, the equation is given by:
\( PV = nRT \)
or,
\( P = \frac{nRT}{V} \)
where \( P \) is the pressure, \( T \) is the temperature, \( R \) is the gas constant, \( n \) is the number of moles, and \( V \) is the volume.
We can express \( P \) in terms of density \( \rho \) by substituting \( \rho = \frac{m}{V} \), where \( m \) is the mass of the gas:
\( P = \frac{\rho RT}{M} \)
where \( M \) is the molar mass of the gas. Rearranging, we get:
\( \rho = \frac{PM}{RT} \)
Analyze the PT Graph for Different Densities:
Since \( \rho = \frac{PM}{RT} \), for a given temperature \( T \), the density \( \rho \) of the gas is directly proportional to the pressure \( P \):
\( \rho \propto P \)
Therefore, at the same temperature, a higher pressure indicates a higher density.
Interpretation of the PT Diagram:
In the given PT diagram, we observe that:
\( P_1 > P_2 > P_3 \) for the same temperature \( T \)
Therefore, based on the proportional relationship \( \rho \propto P \) at constant temperature, we have:
\( \rho_1 > \rho_2 > \rho_3 \)
Conclusion:
The correct statement is: \( \rho_1 > \rho_2 \) which corresponds to Option (2).
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,



What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)