## Chapter 1: Review of Modern Physics |

1.4.2. Laws of thermodynamics

1.4.3. The thermodynamic identity

1.4.4. The Fermi energy

1.4.5. Some useful thermodynamics results

Thermodynamics describes the behavior of systems containing a large number of particles. These systems are characterized by their temperature, volume, number and the type of particles. The state of the system is then further described by its total energy and a variety of other parameters including the entropy. Such a characterization of a system is much simpler than trying to keep track of each particle individually, hence its usefulness. In addition, such a characterization is general in nature so that it can be applied to mechanical, electrical and chemical systems. |

The term thermodynamics is somewhat misleading as one deals primarily with systems in thermal equilibrium. These systems have constant temperature, volume and number of particles and their macroscopic parameters do not change over time, so that the dynamics are limited to the microscopic dynamics of the particles within the system. |

Statistical thermodynamics is based on the fundamental assumption that all possible configurations of a given system, which satisfy the given boundary conditions such as temperature, volume and number of particles, are equally likely to occur. The overall system will therefore be in the statistically most probable configuration. The entropy of a system is defined as the logarithm of the number of possible configurations multiplied with Boltzmann’s constant. While such definition does not immediately provide insight into the meaning of entropy, it does provide a straightforward analysis since the number of configurations can be calculated for any given system. |

Classical thermodynamics provides the same concepts. However, those were obtained through experimental observation. The classical analysis is therefore more tangible compared to the abstract mathematical treatment of the statistical approach. |

The study of semiconductor devices requires some specific results, which naturally emerge from statistical thermodynamics. In this section, we review basic thermodynamic principles as well as some specific results. These include the thermal equilibrium concept, the thermodynamic identity, the basic laws of thermodynamics, the thermal energy per particle, the Fermi function and the thermal voltage . |

## 1.4.1. Thermal equilibrium |

A system is in thermal equilibrium if detailed balance is obtained; i.e. every microscopic process in the system is exactly balanced by its inverse process so that there is no net effect on the system. |

This definition implies that in thermal equilibrium no energy (heat, work or particle energy) is exchanged between the parts within the system or between the system and the environment. Thermal equilibrium is obtained by isolating a system from its environment, removing any internal sources of energy, and waiting for a long enough time until the system does not change any more. |

The concept of thermal equilibrium is of interest since various thermodynamic results assume that the system under consideration is in thermal equilibrium. Few systems of interest rigorously satisfy this condition so that we often apply the thermodynamical results to systems that are "close" to thermal equilibrium. Agreement between theories based on this assumption and experiments justify this approach. |

## 1.4.2. Laws of thermodynamics |

Three laws must be postulated. These cannot be proven in any way and have been developed though the observation of a large number of systems. |

- Heat is a form of energy.
- The second law can be stated either (a) in its classical form or (b) in its statistical form
- Heat can only flow from a higher temperature to a lower temperature.
- The entropy of a closed system (i.e. a system of particles which does not exchange heat, work or particles with its surroundings) tends to remain constant or increases monotonically over time.
- The entropy of a system approaches a constant as the temperature approaches zero Kelvin.