Difference between revisions of "Ideal Bose Gas"

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A Bose–Einstein condensate (BEC) is a state of matter of a dilute gas of bosons cooled to temperatures very close to absolute zero (that is, very near 0 K or −273.16 °C). Under such conditions, a large fraction of bosons occupies the lowest quantum state, at which point macroscopic quantum phenomena become apparent.
 
A Bose–Einstein condensate (BEC) is a state of matter of a dilute gas of bosons cooled to temperatures very close to absolute zero (that is, very near 0 K or −273.16 °C). Under such conditions, a large fraction of bosons occupies the lowest quantum state, at which point macroscopic quantum phenomena become apparent.
 
=== Overview ===
 
=== Overview ===
 +
In this section, we summarize some basic and useful thermodynamic results for Bose-Einstein condensation in a uniform, non-interacting gas of bosons.
 +
=== The Bose distribution ==
 +
For non-interacting bosons in thermodynamic equilibrium, the mean occupation number of the single-particle state <math> \nu </math> is
 +
:<math>
 +
\langle n_{\nu} \rangle = \frac{1}{e^{(\epsilon_{\nv}-\mu)/kT}-1}
 +
\,.
 +
</math>

Revision as of 00:41, 3 May 2017

A Bose–Einstein condensate (BEC) is a state of matter of a dilute gas of bosons cooled to temperatures very close to absolute zero (that is, very near 0 K or −273.16 °C). Under such conditions, a large fraction of bosons occupies the lowest quantum state, at which point macroscopic quantum phenomena become apparent.

Overview

In this section, we summarize some basic and useful thermodynamic results for Bose-Einstein condensation in a uniform, non-interacting gas of bosons.

= The Bose distribution

For non-interacting bosons in thermodynamic equilibrium, the mean occupation number of the single-particle state is

Failed to parse (MathML with SVG or PNG fallback (recommended for modern browsers and accessibility tools): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \langle n_{\nu} \rangle = \frac{1}{e^{(\epsilon_{\nv}-\mu)/kT}-1} \,. }