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In 1908 P. Langevin [[#References|[a1]]] proposed the following equation to describe the natural phenomenon of [[Brownian motion|Brownian motion]] (the irregular vibrations of small dust particles suspended in a liquid):
 
In 1908 P. Langevin [[#References|[a1]]] proposed the following equation to describe the natural phenomenon of [[Brownian motion|Brownian motion]] (the irregular vibrations of small dust particles suspended in a liquid):
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574401.png" /></td> <td valign="top" style="width:5%;text-align:right;">(a1)</td></tr></table>
+
$$ \tag{a1 }
 +
 
 +
\frac{dv ( t) }{dt}
 +
  = - \gamma v ( t) + L ( t).
 +
$$
  
Here <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574402.png" /> denotes the velocity at time <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574403.png" /> along one of the coordinate axes of the Brownian particle, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574404.png" /> is a friction coefficient due to the viscosity of the liquid, and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574405.png" /> is a postulated  "Langevin forceLangevin force" , standing for the pressure fluctuations due to thermal motion of the molecules comprising the liquid. This Langevin force was supposed to have the properties
+
Here $  v ( t) $
 +
denotes the velocity at time $  t $
 +
along one of the coordinate axes of the Brownian particle, $  \gamma > 0 $
 +
is a friction coefficient due to the viscosity of the liquid, and $  L ( t) $
 +
is a postulated  "Langevin forceLangevin force" , standing for the pressure fluctuations due to thermal motion of the molecules comprising the liquid. This Langevin force was supposed to have the properties
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574406.png" /></td> </tr></table>
+
$$
 +
\mathbf E ( L ( t))  = 0 \ \
 +
\textrm{ and } \ \
 +
\mathbf E ( L ( t) L ( s))  = D \cdot \delta ( t - s).
 +
$$
  
 
The Langevin equation (a1) leads to the following diffusion (or  "Fokker–Planck" ) equation (cf. [[Diffusion equation|Diffusion equation]]) for the probability density on the velocity axis:
 
The Langevin equation (a1) leads to the following diffusion (or  "Fokker–Planck" ) equation (cf. [[Diffusion equation|Diffusion equation]]) for the probability density on the velocity axis:
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574407.png" /></td> <td valign="top" style="width:5%;text-align:right;">(a2)</td></tr></table>
+
$$ \tag{a2 }
 +
{
 +
\frac \partial {\partial  t }
 +
}
 +
\rho _ {t} ( v)  = \
 +
\gamma
 +
\frac \partial {\partial  v }
 +
 
 +
( v \rho _ {t} ( v)) +
 +
{
 +
\frac{1}{2}
 +
} D  ^ {2}
 +
 
 +
\frac{\partial  ^ {2} }{\partial  v  ^ {2} }
 +
 
 +
\rho _ {t} ( v).
 +
$$
  
The equations (a1) and (a2) provided a conceptual and quantitative improvement on the description of the phenomenon of Brownian motion given by A. Einstein in 1905. The quantitative understanding of Brownian motion played a large role in the acceptance of the theory of molecules by the scientific community. The numerical relation between the two observable constants <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574408.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l0574409.png" />, namely <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l05744010.png" /> (where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l05744011.png" /> is the temperature and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l05744012.png" /> the particle's mass), gave the first estimate of Boltzmann's constant <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l05744013.png" />, and thereby of Avogadro's number.
+
The equations (a1) and (a2) provided a conceptual and quantitative improvement on the description of the phenomenon of Brownian motion given by A. Einstein in 1905. The quantitative understanding of Brownian motion played a large role in the acceptance of the theory of molecules by the scientific community. The numerical relation between the two observable constants $  \gamma $
 +
and $  D $,  
 +
namely $  D = 2 \gamma kT/M $(
 +
where $  T $
 +
is the temperature and $  M $
 +
the particle's mass), gave the first estimate of Boltzmann's constant $  k $,  
 +
and thereby of Avogadro's number.
  
 
The Langevin equation may be considered as the first [[Stochastic differential equation|stochastic differential equation]]. Today it would be written as
 
The Langevin equation may be considered as the first [[Stochastic differential equation|stochastic differential equation]]. Today it would be written as
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l05744014.png" /></td> </tr></table>
+
$$
 +
dv ( t)  = - \gamma u ( t)  dt + D  dw ( t),
 +
$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/l/l057/l057440/l05744015.png" /> is the [[Wiener process|Wiener process]] (confusingly called  "Brownian motion"  as well). The solution of the Langevin equation is a [[Markov process|Markov process]], first described by G.E. Uhlenbeck and L.S. Ornstein in 1930 [[#References|[a2]]] (cf. also [[Ornstein–Uhlenbeck process|Ornstein–Uhlenbeck process]]).
+
where $  w ( t) $
 +
is the [[Wiener process|Wiener process]] (confusingly called  "Brownian motion"  as well). The solution of the Langevin equation is a [[Markov process|Markov process]], first described by G.E. Uhlenbeck and L.S. Ornstein in 1930 [[#References|[a2]]] (cf. also [[Ornstein–Uhlenbeck process|Ornstein–Uhlenbeck process]]).
  
 
The Langevin equation is a heuristic equation. The program to give it a solid foundation in Hamiltonian mechanics has not yet fully been carried through. Considerable progress was made by G.W. Ford, M. Kac and P. Mazur [[#References|[a3]]], who showed that the process of Uhlenbeck and Ornstein can be realized by coupling the Brownian particle in a specific way to an infinite number of harmonic oscillators put in a state of thermal equilibrium.
 
The Langevin equation is a heuristic equation. The program to give it a solid foundation in Hamiltonian mechanics has not yet fully been carried through. Considerable progress was made by G.W. Ford, M. Kac and P. Mazur [[#References|[a3]]], who showed that the process of Uhlenbeck and Ornstein can be realized by coupling the Brownian particle in a specific way to an infinite number of harmonic oscillators put in a state of thermal equilibrium.

Latest revision as of 22:15, 5 June 2020


In 1908 P. Langevin [a1] proposed the following equation to describe the natural phenomenon of Brownian motion (the irregular vibrations of small dust particles suspended in a liquid):

$$ \tag{a1 } \frac{dv ( t) }{dt} = - \gamma v ( t) + L ( t). $$

Here $ v ( t) $ denotes the velocity at time $ t $ along one of the coordinate axes of the Brownian particle, $ \gamma > 0 $ is a friction coefficient due to the viscosity of the liquid, and $ L ( t) $ is a postulated "Langevin forceLangevin force" , standing for the pressure fluctuations due to thermal motion of the molecules comprising the liquid. This Langevin force was supposed to have the properties

$$ \mathbf E ( L ( t)) = 0 \ \ \textrm{ and } \ \ \mathbf E ( L ( t) L ( s)) = D \cdot \delta ( t - s). $$

The Langevin equation (a1) leads to the following diffusion (or "Fokker–Planck" ) equation (cf. Diffusion equation) for the probability density on the velocity axis:

$$ \tag{a2 } { \frac \partial {\partial t } } \rho _ {t} ( v) = \ \gamma \frac \partial {\partial v } ( v \rho _ {t} ( v)) + { \frac{1}{2} } D ^ {2} \frac{\partial ^ {2} }{\partial v ^ {2} } \rho _ {t} ( v). $$

The equations (a1) and (a2) provided a conceptual and quantitative improvement on the description of the phenomenon of Brownian motion given by A. Einstein in 1905. The quantitative understanding of Brownian motion played a large role in the acceptance of the theory of molecules by the scientific community. The numerical relation between the two observable constants $ \gamma $ and $ D $, namely $ D = 2 \gamma kT/M $( where $ T $ is the temperature and $ M $ the particle's mass), gave the first estimate of Boltzmann's constant $ k $, and thereby of Avogadro's number.

The Langevin equation may be considered as the first stochastic differential equation. Today it would be written as

$$ dv ( t) = - \gamma u ( t) dt + D dw ( t), $$

where $ w ( t) $ is the Wiener process (confusingly called "Brownian motion" as well). The solution of the Langevin equation is a Markov process, first described by G.E. Uhlenbeck and L.S. Ornstein in 1930 [a2] (cf. also Ornstein–Uhlenbeck process).

The Langevin equation is a heuristic equation. The program to give it a solid foundation in Hamiltonian mechanics has not yet fully been carried through. Considerable progress was made by G.W. Ford, M. Kac and P. Mazur [a3], who showed that the process of Uhlenbeck and Ornstein can be realized by coupling the Brownian particle in a specific way to an infinite number of harmonic oscillators put in a state of thermal equilibrium.

In more recent years, quantum mechanical versions of the Langevin equation have been considered. They can be subdivided into two classes: those which yield Markov processes and those which satisfy a condition of thermal equilibrium. The former are known as "quantum stochastic differential equations" [a4], the latter are named "quantum Langevin equations" [a5].

References

[a1] P. Langevin, "Sur la théorie de mouvement Brownien" C.R. Acad. Sci. Paris , 146 (1908) pp. 530–533
[a2] G.E. Uhlenbeck, L.S. Ornstein, "On the theory of Brownian motion" Phys. Rev. , 36 (1930) pp. 823–841
[a3] G.W. Ford, M. Kac, P. Mazur, "Statistical mechanics of assemblies of coupled oscillators" J. Math. Phys. , 6 (1965) pp. 504–515
[a4] C. Barnett, R.F. Streater, I.F. Wilde, "Quasi-free quantum stochastic integrals for the CAR and CCR" J. Funct. Anal. , 52 (1983) pp. 19–47
[a5] R.L. Hudson, K.R. Parthasarathy, "Quantum Itô's formula and stochastic evolutions" Commun. Math. Phys. , 93 (1984) pp. 301–323
How to Cite This Entry:
Langevin equation. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Langevin_equation&oldid=16399
This article was adapted from an original article by H. Maassen (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article