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[NOTES/SM-04011] Specific Heat of Diatomic Gases --- Quantum Effects

The quantum effect of  vibrations on specific heat of diatomic gases is presented. The results are in agreement with experimentally observed facts.

[NOTES/SM-04014] Partition Function of an Ideal Gas

In this section the classical canonical partition function of an ideal gas is computed.

[NOTES/SM-04008] `Distribution of Molecules under Gravity

Distribution function of molecules in presence of gravity is as function of height is derived. 

[NOTES/SM-04007] Applications of Maxwell's Distribution

The equation of state of a perfect gas is derived using Maxwell distribution of velocities of molecules in a perfect gas. The Maxwell distribution can be verified by means of an experiment on effusion of a gas through a hole. This also lead to determination of the Boltzmann constant

[NOTES/SM-04006] Maxwell Distribution of speeds in an ideal gas

For an ideal gas Maxwell's distribution of velocities is obtained using canonical ensemble.

[NOTES/SM-04012] Statistical Entropy

It is shown that the statistical entropy coincides with the thermodynamic expression for entropy.

[NOTES/SM-04017] Internal Energy

For a system in contact with heat bath, the energy is not well defined. The system being in a micro state with energy value \(E_k\) is given by Boltzmann distribution. We compute average energy and show that the average energy  it in terms of the  canonical partition function is given by \[ U = -k \pp[\ln Z]{\beta}.\] It is shown that for macroscopic systems the variance of energy is negligible compared to the energy, but not for microscopic systems. Hence \(\bar E\) can be identified with the thermodynamic internal energy.

[NOTES/SM-04004] Thermodynamic Functions in Terms of Canonical Partition Function

Using the expression for energy in terms of the canonical partition function and the \(TdS\) equation \[dU=TdS -pdV\] <

[NOTES/SM-04001] The Canonical Ensemble

In this lecture canonical ensemble and canonical partition function are introduced. This topic has a central place in equilibrium  statistical mechanics. This ensemble describes the microstates of a system in equilibrium with a heat bath at temperature \(T\). The probability of a microstate having energy \(E\) is proportional to \(\exp(-\beta E\), where \(\beta=kT\) and \(k\) is Boltzmann constant. 

[CHAT/SM-04001] Systems in Equilibrium with a Heat Reservoir


We are interested in a statistical description of a system in contact with a heat bath (reservoir).Such a system can exchange energy with the heat bath and is not an isolated system. Therefore, in equilibrium all micro states will not have equal a priori probabilities. It turns out that micro states with different energies have different probabilities.An ensemble of system in contact with a heat bath is called canonical ensemble.We need to find the probability of micro state as function of energy and the temperature of the heat bath.

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