Fermi gas | Wikipedia audio article
Channel: wikipedia tts
Date: 24/12/2018

This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Fermi_gas


00:00:48 1 Description
00:03:33 2 Illustration of the Fermi energy for a one-dimensional well
00:06:54 3 Three-dimensional case
00:14:34 4 Related quantities
00:16:50 5 Thermodynamic quantities
00:17:12 5.1 Degeneracy pressure
00:19:23 5.2 Chemical potential
00:21:32 6 Density of states
00:23:46 6.1 Arbitrary-dimensional case
00:28:31 7 Treatment at finite temperature
00:28:41 7.1 Grand canonical ensemble
00:33:50 7.2 Relation to Fermi-Dirac distribution
00:39:21 8 Typical values
00:39:30 8.1 Metals
00:41:23 8.2 White dwarfs
00:42:56 8.3 Nucleus
00:45:58 9 Extensions to the model
00:46:08 9.1 Relativistic Fermi gas
00:48:47 9.2 Fermi liquid
00:49:25 10 See also



Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.

Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain

Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.

Listen on Google Assistant through Extra Audio:
https://assistant.google.com/services/invoke/uid/0000001a130b3f91
Other Wikipedia audio articles at:
https://www.youtube.com/results?search_query=wikipedia+tts
Upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts



"There is only one good, knowledge, and one evil, ignorance."
- Socrates



SUMMARY
=======
An ideal Fermi gas is a state of matter which is an ensemble of a large number of non-interacting fermions. Fermions are particles that obey Fermi–Dirac statistics, like electrons, protons, and neutrons, and, in general, particles with half-integer spin. These statistics determine the energy distribution of fermions in a Fermi gas in thermal equilibrium, and is characterized by their number density, temperature, and the set of available energy states. The model is named after the Italian physicist Enrico Fermi.This physical model can be accurately applied to many systems with a large number of fermions. Some key examples are the behaviour of charge carriers in a metal, nucleons in an atomic nucleus, neutrons in a neutron star, and electrons in a white dwarf.