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Clas Blomberg - Physics of life-Elsevier Science (2007)

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226 Part V. Stochastic dynamics

All information about such a process lies in the averages X(t) and the autocorrelation functions

X(t 1 ) X(t 2 ). This makes the process relatively easy to handle even if the process is not

Markovian.

If one requires that the process is Gaussian, Markovian and also has a stationary

distribution, then there is only one possibility. With one variable, its relevant probability

functions are:

1

Pxt ( , ) e

(( xx0 ) 2 / 2a)

Pxt ( , x1, tt)

2pa

1

( ) exp ⎛ 1

( xx x

gt

)

2

0 1e

2pa

1 e2gt

⎝⎜

2a

⎠⎟

(22.15)

x 0 is the average of X(t). All other probabilities are given from these. This process is called the

Ornstein–Uhlenbeck process. We will encounter this process in later example, in particular

concerning Brownian motion, Chapter 23. The velocity distribution of Brownian motion is

of this kind.

22D

Fokker–Planck equations

Transition from discrete steps to continuous equations

In the previous chapter, we considered discrete processes, characterised by certain discrete

states and probabilities of transitions between the states. The development of the probability

distribution of the respective states was described by the following type of equation, called

master equation.

dPn

() t

an ( 1) Pn1( t) bn ( 1) Pn1( t) [ an ( ) bn ( )] Pn( t)

dt

(22.16)

where P n (t) is the probability for being in state ‘n’ at time t; a(n) is the transition probability

rate for going one step downwards from state ‘n’ to state ‘n 1’, and b(n) is the transition

probability rate to go one step upwards from state ‘n’ to ‘n + 1’. The states may mean number

of particles of some kind (e.g. reacting substances) or certain positions.

These equations can be difficult to handle, and one may try other possibilities. If the state

numbers are large, it might be advantageous to go over to a continuous description, to treat

the state values as a continuous variable. A way to accomplish this is to use the first terms

in a Taylor expansion:

1

2

Fx ( 1) Fx ( ) F( x) F( x); Fx ( 1) Fx ( ) F( x) F( x)

1

2

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