Difference between revisions of "Langevin equation"
(Importing text file) |
Ulf Rehmann (talk | contribs) m (tex encoded by computer) |
||
Line 1: | Line 1: | ||
+ | <!-- | ||
+ | l0574401.png | ||
+ | $#A+1 = 15 n = 0 | ||
+ | $#C+1 = 15 : ~/encyclopedia/old_files/data/L057/L.0507440 Langevin equation | ||
+ | Automatically converted into TeX, above some diagnostics. | ||
+ | Please remove this comment and the {{TEX|auto}} line below, | ||
+ | if TeX found to be correct. | ||
+ | --> | ||
+ | |||
+ | {{TEX|auto}} | ||
+ | {{TEX|done}} | ||
+ | |||
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): | ||
− | + | $$ \tag{a1 } | |
+ | |||
+ | \frac{dv ( t) }{dt} | ||
+ | = - \gamma v ( t) + L ( t). | ||
+ | $$ | ||
− | Here | + | 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|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: | ||
− | + | $$ \tag{a2 } | |
+ | { | ||
+ | \frac \partial {\partial t } | ||
+ | } | ||
+ | \rho _ {t} ( v) = \ | ||
+ | \gamma | ||
+ | \frac \partial {\partial v } | ||
+ | |||
+ | ( v \rho _ {t} ( v)) + | ||
+ | { | ||
+ | \frac{1}{2} | ||
+ | } D ^ {2} | ||
+ | |||
+ | \frac{\partial ^ {2} }{\partial v ^ {2} } | ||
+ | |||
+ | \rho _ {t} ( v). | ||
+ | $$ | ||
− | 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 | + | 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 | ||
− | + | $$ | |
+ | dv ( t) = - \gamma u ( t) dt + D dw ( t), | ||
+ | $$ | ||
− | where | + | 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 |
Langevin equation. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Langevin_equation&oldid=16399