Likewise, the mean electron energy is

Because, in general, the energies of the quantum states are very closely spaced, the sums in the previous two expressions can be replaced by integrals. Now, according to Section 8.12, the number of quantum states per unit volume with wavenumbers in the range to is

(8.156) |

However, the energy of a state with wavenumber is

(8.157) |

where is the electron mass. Let be the number of electrons whose energies lies in the range to . It follows that

(8.158) |

where the factor of is to take into account the two possible spin states which exist for each translational state. Hence,

Moreover, Equations (8.154) and (8.155) become

where

is the Fermi function.

The integrals on the right-hand sides of Equations (8.160) and (8.161) are both of the general form

where is a smoothly varying function of . Let

(8.164) |

We can integrate Equation (8.163) by parts to give

(8.165) |

which reduces to

because . Here, .

Now, if then is a constant everywhere, apart from a thin region of thickness , centered on . (See Figure 8.4.) It follows that is approximately zero everywhere, apart from in this region. Hence, the relatively slowly-varying function can be Taylor expanded about :

(8.167) |

Thus, Equation (8.166) becomes

(8.168) |

From Equation (8.162), we have

(8.169) |

which becomes

(8.170) |

where . However, because the integrand has a sharp maximum at , and because , we can replace the lower limit of integration by with negligible error. Thus, we obtain

(8.171) |

where

(8.172) |

Note that

(8.173) |

is an even function of . It follows, by symmetry, that is zero when is odd. Moreover,

(8.174) |

Finally, it can be demonstrated that

(8.175) |

(See Exercise 3.) Hence, we deduce that

(8.176) |

This expansion is known as the

Equation (8.160) yields

(8.177) |

However, it follows from Equation (8.159) that

(8.178) | ||

(8.179) |

Hence,

(8.180) |

which can also be written

(8.181) |

where is the Fermi energy at . [See Equation (8.144).] The previous equation can be rearranged to give

(8.182) |

which reduces to

assuming that . Figure 8.6 shows a comparison between the previous approximate expression for the temperature variation of the Fermi energy of a degenerate electron gas and the numerically-calculated exact value. It can be seen that our approximate expression is surprisingly accurate (at least, for ).

Equation (8.161) yields

(8.184) |

However, it follows from Equation (8.159) that

(8.185) | ||

(8.186) |

Hence,

(8.187) |

which can also be written

(8.188) |

Making use of Equation (8.183), and only retaining terms up to second order in , we obtain

(8.189) |

Hence, the specific heat capacity of the conduction electrons becomes

(8.190) |

and the molar specific heat is written

(8.191) |

Of course, because , this value is much less than the classical estimate, .