View source for Fermi-Dirac statistics

== Introduction ==

Fermi-Dirac statistics, named after [[Enrico Fermi|Enrico Fermi]] and [[Paul Dirac|Paul Dirac]], is a statistical distribution that describes the behavior of a collection of non-interacting fermions. Fermions are a type of [[Elementary particle|elementary particle]] that follow the Pauli Exclusion Principle, which states that no two fermions can occupy the same quantum state simultaneously. This distinguishes them from bosons, particles that follow [[Bose-Einstein statistics|Bose-Einstein statistics]] and do not have this restriction.

[[Image:Detail-45903.jpg|thumb|center|A collection of fermions in a quantum state.|class=only_on_mobile]]
[[Image:Detail-45904.jpg|thumb|center|A collection of fermions in a quantum state.|class=only_on_desktop]]

== Fermions and the Pauli Exclusion Principle ==

The [[Pauli Exclusion Principle|Pauli Exclusion Principle]], formulated by physicist Wolfgang Pauli, is a fundamental principle in quantum mechanics. It states that two or more identical fermions cannot occupy the same quantum state within a quantum system simultaneously. This principle is derived from the symmetry properties of the wavefunction for identical particles, which is antisymmetric for fermions.

Fermions include elementary particles such as quarks, which make up protons and neutrons, and leptons, which include electrons and neutrinos. Composite particles can also be fermions if they are composed of an odd number of these elementary particles. For example, protons and neutrons are fermions, while mesons (composed of two quarks) are bosons.

== Fermi-Dirac Distribution ==

The Fermi-Dirac distribution function describes the probability that a given quantum state in a system of fermions is occupied. It is given by the equation:

f(E) = 1 / (1 + exp((E - μ) / kT))

where E is the energy of the state, μ is the chemical potential, k is the Boltzmann constant, and T is the temperature. The chemical potential is a parameter that determines the probability that a particle will be in a particular state. At absolute zero temperature, the distribution becomes a step function, with all states below the Fermi energy being filled and all states above being empty.

== Fermi Energy and Fermi Temperature ==

The Fermi energy is the energy level below which all energy states are approximately filled at absolute zero temperature. It is a crucial concept in many areas of physics, including solid-state physics and quantum chemistry. The Fermi energy can be calculated using the density of states and the Fermi-Dirac distribution function.

The Fermi temperature, defined as the Fermi energy divided by the Boltzmann constant, is a measure of how much thermal energy is needed to excite an electron from the Fermi level to a higher energy state. It is a significant parameter in low-temperature physics.

== Applications of Fermi-Dirac Statistics ==

Fermi-Dirac statistics have wide-ranging applications in various fields of physics. In solid-state physics, they are used to describe the behavior of electrons in a solid, leading to an understanding of electrical conductivity and the properties of semiconductors. In nuclear physics, they are used to describe the behavior of nucleons in a nucleus. In astrophysics, they are used to describe the behavior of particles in white dwarf stars and neutron stars.

== See Also ==

[[Quantum mechanics]]

[[Statistical mechanics]]

[[Solid-state physics]]

[[Category:Quantum mechanics]]

[[Category:Statistical mechanics]]

[[Category:Particle physics]]