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[NOTES/SM-06006] Mean Occupation Number for Identical Fermions and Bosons

Using occupation number representation for identical particles, the grand canonical partition function is expressed in terms of single particle partition function. This is then used to discuss cases of identical fermions and identical bosons. Mean occupation number for fermions and bosons is obtained.

[NOTES/SM-06004] Grand Canonical Ensemble --- Pressure and Chemical Potential

Using thermodynamics to express TdS in terms of Gibbs energy and comparing TdS expression in terms of the grand canonical partition function we obtain pressure and chemical potential function in terms of grand canonical partition function.

[NOTES/SM-06005] Entropy and Energy in Terms of Grand Canonical Partition Function

In this article various thermodynamic functions are expressed in terms of the grand canonical partition function.

[NOTES/SM-06003] Grand Canonical Ensemble

In this article various thermodynamic functions are expressed in terms of the grand canonical partition function.

[NOTES/SM-04018] Boltzmann Entropy from Canonical Partition Function

We derive the Boltzmann relation for entropy using the canonical partition function. This derivation uses the fact that the number of micro states \(\Omega(E)\) as a function energy has a sharp peak around the mean energy.

[NOTES/SM-04019] Properties of an Ideal Gas

Several properties such as internal energy, entropy etc. of perfect gases are calculated using the canonical partition function.

[NOTES/SM-04009] The Imperfect Gas

The ideal gas equation \(pV=NkT\) is good approximation for low densities. In this section a scheme of obtaining corrections to the ideal gas equation is discussed.

[NOTES/SM-04005] Applications of Canonical Ensemble to Paramanetism

In this section the method of canonical ensemble is applied to paramagnetism. For a paramagnetic substance the variation of paramagnetic susceptibility with temperature is derived.

[NOTES/SM-04015] Equilibrium of a System with a Heat Reservoir

For a system in equilibrium with a heat bath at temperature \(T\) the energy is not constant. We start with the Boltzmann relation \(S=k\log \Omega\). It will be shown that if of a microstate has energy \(E_r\), its probability \(p_r\) is proportional to \(e^{-\beta E_r}\) and is given by
\[p_r = \frac{\exp(-\beta E_r)}{Z} \]
where \(Z\) is function of \(T,V,N\), called the canonical partition function and is given by
\[Z = \sum_{\text{MS }r} \exp(-\beta E_r).\]

[NOTES/SM-04010] Classical Theory of Specific Heat of Gases

In this lecture we derive law of equipartition of energy under the assumption that the energy is quadratic function of some variable such as coordinates and momenta. As an application, the classical theory of specific heat of gases is given.

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