Content deleted Content added
m Open access bot: url-access=subscription updated in citation with #oabot. |
|||
(20 intermediate revisions by 15 users not shown) | |||
Line 1:
{{Short description|Function of seven variables}}
In molecular [[kinetic theory of gases|kinetic theory]] in [[physics]], a
<math display="block">\begin{align}
▲In molecular [[kinetic theory of gases|kinetic theory]] in [[physics]], a particle's '''distribution function''' is a function of seven variables, <math>f(x,y,z,t;v_x,v_y,v_z)</math>, which gives the number of particles per unit volume in single-particle [[phase space]]. It is the number of particles per unit volume having approximately the [[velocity]] <math>(v_x,v_y,v_z)</math> near the place <math>(x,y,z)</math> and time <math>(t)</math>. The usual normalization of the distribution function is
n(\mathbf{r},t) &= \int f(\mathbf{r}, \mathbf{v}, t) \,dv_x \,dv_y \,dv_z, \\
\end{align} </math>
where
▲where, ''N'' is the total number of particles, and ''n'' is the [[number density]] of particles – the number of particles per unit volume, or the [[density]] divided by the mass of individual particles.
A distribution function may be specialised with respect to a particular set of dimensions. E.g. take the quantum mechanical six-dimensional phase space, <math>f(x,y,z;p_x,p_y,p_z)</math> and multiply by the total space volume, to give the momentum distribution, i.e. the number of particles in the momentum phase space having approximately the [[momentum]] <math>(p_x,p_y,p_z)</math>.
Particle distribution functions are often used in [[plasma physics]] to describe wave–particle interactions and velocity-space instabilities.
The [[Maxwell–Boltzmann distribution|basic distribution function]] uses the [[Boltzmann constant]] <math>k</math> and temperature <math>T</math> with the number density to modify the [[normal distribution]]:
<math display="block">\begin{align}
&= n\left(\frac{m}{2 \pi kT}\right)^{3/2} \exp\left(-\frac{m(v_x^2 + v_y^2 + v_z^2)}{2kT}\right).
\end{align} </math>
Related distribution functions may allow bulk fluid flow, in which case the velocity origin is shifted, so that the
▲:<math> f = n\left(\frac{m}{2 \pi kT}\right)^{3/2} \exp\left({-\frac{m(v_x^2 + v_y^2 + v_z^2)}{2kT}}\right). </math>
[[Plasma (physics)|Plasma]] theories such as [[magnetohydrodynamics]] may assume the particles to be in [[thermodynamic equilibrium]].
▲Related distribution functions may allow bulk fluid flow, in which case the velocity origin is shifted, so that the [[exponent]]'s [[numerator]] is <math>m((v_x - u_x)^2 + (v_y - u_y)^2 + (v_z - u_z)^2)</math>, where <math>(u_x, u_y, u_z)</math> is the bulk velocity of the fluid. Distribution functions may also feature non-isotropic temperatures, in which each term in the exponent is divided by a different temperature.
The mathematical
▲Plasma theories such as [[magnetohydrodynamics]] may assume the particles to be in [[thermodynamic equilibrium]]. In this case, the distribution function is ''[[Maxwell–Boltzmann distribution|Maxwellian]]''. This distribution function allows fluid flow and different temperatures in the directions parallel to, and perpendicular to, the local magnetic field. More complex distribution functions may also be used, since [[Plasma (physics)|plasmas]] are rarely in thermal equilibrium.
==References==
▲The mathematical analog of a distribution is a [[measure (mathematics)|measure]]; the time evolution of a measure on a phase space is the topic of study in [[dynamical systems]].
{{reflist}}
[[Category:Statistical mechanics]]
[[Category:Dynamical systems]]
{{statisticalmechanics-stub}}
|