Brownian Motion Problem_Random Walk

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    Brownian Motion Problem: Random Walk andBeyond

    Shama Sharma and Vishwamittar

    Shama Sharma is

    currently working as

    lecturer at DAV College,

    Punjab. She is working on

    some problems in

    nonequilibrium statistical

    mechanics.

    Vishwamittar is professor

    in physics at Panjab

    University, Chandigarh

    and his present research

    activities are in

    nonequilibrium statistical

    mechanics. He has written

    articles on teaching of

    physics, history and

    philosophy of physics.

    Keywords

    Brownian motion, Langevins

    theory, random walk, stochas-

    tic processes, non-equilib rium

    statistical mechanics.

    A brief account of developments in the experi-

    mental and theoretical investigations of Brown-

    ian motion is presented. Interestingly, Einstein

    who did not like God's game of playing dice for

    electrons in an atom himself put forward a theory

    of Brownian movement allowing God to play thedice. The vital role played by his random walk

    model in the evolution of non-equilibrium statis-

    tical mechanics and multitude of its applications

    is highlighted. Also included are the basics of

    Langevin's theory for Brownian motion.

    Introduction

    Brownian motion is the temperature-dependent perpet-

    ual, irregular motion of the particles (of linear dimen-

    sion of the order of 106m) immersed in a uid, causedby their continuous bombardment by the surrounding

    molecules of much smaller size (Figure 1). This eectwas rst reported by the Dutch physician, chemist andengineer Jan Ingenhousz (1785), when he found thatne powder of charcoal oating on alcohol surface ex-

    hibited a highly random motion. However, it got thename Brownian motion after Scottish botanist RobertBrown, who in 1828-29 published the results of his ex-tensive studies on the incessant random movement of

    tiny particles like pollen grains, dust and soot suspendedin a uid (Box 1). To begin with when experimentswere performed with pollen immersed in water, it was

    thought that ubiquitous irregular motion was due to thelife of these grains. But this idea was soon discarded asthe observations remained unchanged even when pollenwas subjected to various killing treatments, liquids other

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    Box 1. Observing the Brownian Motion

    One can observe Brownian movement by looking through an optical microscope with magnification 103

    104 at a well illuminated sample of some colloidal solution (say milk drops put into water) or smoke

    particles in air. Alternately, we can mount a small mirror (area 1 or 2 mm2) on a fine torsion fiber capable

    of rotation about a vertical axis (as in suspension type galvanometer) in a chamber having air pressure of

    about 102 torr and note the movement of the spot of light reflected from the mirror. The trace of the light

    spot is manifestation of angular Brownian motion of the mirror.

    It may be pointed out that movement of dust particles in the air as seen in a beam of light through a window

    is not an example of Brownian motion as these particles are too large and the random collisions with air

    molecules are neither much imbalanced nor strong enough to cause Brownian movement.

    Figure 1. Brownian motion

    of a fine particle immersed

    in a fluid.

    than water were used and ne particles of glass, petri-ed wood, minerals, sand, etc were immersed in variousliquids. Furthermore, possible causes like vibrations ofbuilding or the laboratory table, convection currents inthe uid, coagulation of particles, capillary forces, in-ternal circulation due to uneven evaporation, currentsproduced by illuminating light, etc were considered butwere found to be untenable.

    An early realization of the consequences of the stud-ies on Brownian motion was that it imposes limit onthe precision of measurements by small instruments asthese are under the inuence of random impacts of thesurrounding air.

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    1These are collected in the book

    Alber t Einstein : Investigations

    on the theory of Brownian

    Movementedited with notes by

    R Furth (Dover Publications,

    New York,1956).

    2 Review article entitled Brown-

    ian Movement and Molecular

    Reality based on his work has

    been transla ted into English by

    F Soddy and pub lished by Tay-

    lor & Francis,London in 1910.

    In 1863, Wienerattributed Brownian

    motion to molecular

    movement of the

    liquid.

    experiments.

    In 1863, Wiener attributed Brownian motion to mole-cular movement of the liquid and this viewpoint wassupported by Delsaux (1877-80) and Gouy (1888-95).On the basis of a series of experiments Gouy convinc-ingly ruled out the exterior factors as causes of Brown-ian motion and argued in favour of contribution of thesurrounding uid. He also discussed the connection be-tween Brownian motion and Carnot's principle and there-by brought out the statistical nature of the laws of ther-modynamics. Such ideas put Brownian motion at theheart of the then prevalent controversial views about

    philosophy of science. Then, in 1900 Bachelier obtaineda diusion equation for random processes and thus, atheory of Brownian motion in his PhD thesis on stockmarket uctuation. Unfortunately, this work was notrecognized by the scientic community, including hissupervisor Poincare, because it was in the eld of eco-nomics and it did not involve any of the relevant physicalaspects.

    Eventually, Einstein in a number of research publica-

    tions beginning in 1905 put forward an acceptable modelfor Brownian motion1 . His approach is known as `ran-dom walk' or `drunkards walk' formalism and uses the

    uctuations in molecular collisions as the cause of Brown-ian movement. His work was followed by an almost sim-ilar expression for the time dependence of displacementof the Brownian particle by Smoluchowski in 1906, who

    started with a probability function for describing themotion of the particle. In 1908, Langevin gave a phe-nomenological theory of Brownian motion and obtained

    essentially the same formulae for displacement of theparticle. Their results were experimentally veri ed byPerrin (1908 and onwards)2 using precise measurementson sedimentation in colloidal suspensions to determine

    the Avogadro's number. Later on, more accurate val-ues of this constant and that of Boltzmann constant kwere found out by many workers by performing similar

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    The correctness ofthe random walk

    model and

    Langevins theory

    made a very strong

    case in favour of

    molecular kinetic

    model of matter.

    The techniquesdeveloped for the

    theory of Brownian

    motion form

    cornerstones for

    investigating a variety

    of phenomena.

    The correctness of the random walk model and Lange-vin's theory made a very strong case in favour of mole-cular kinetic model of matter and unleashed a wave of

    activity for a systematic development of dynamical the-ory of Brownian motion by Fokker, Planck, Uhlenbeck,Ornstein and several other scientists. As such, during

    the last 100 years, concerted eorts by a galaxy of physi-cists, mathematicians, chemists, etc have not only pro-vided a proper mathematical foundation to the physical

    theory but have also led to extensive diverse applicationsof the techniques developed.

    The two basic ingredients of Einstein's theory were: (i)the movement of the Brownian particle is a consequenceof continuous impacts of the randomly moving surround-ing molecules of the uid (the `noise'); (ii) these impactscan be described only probabilistically so that time evo-lution of the particle under observation is also proba-bilistic in nature. Phenomena of this type are referred toas stochastic processes in mathematics and these are es-sentially non-equilibrium or irreversible processes. Thus,Einstein's theory laid the foundation of stochastic mod-eling of natural phenomena and formed the basis ofdevelopment of non-equilibrium statistical mechanics,wherein generally, the Brownian particle is replaced bya collective property of a macroscopic system. Con-sequently, the techniques developed for the theory ofBrownian motion form cornerstones for investigating avariety of phenomena (in dierent branches of scienceand engineering) that have their origin in the eect ofnumerous unpredictable and may be unobservable eventswhose individual contribution to the observed feature is

    negligible, but collective impact is observed in the formof rather rapidly varying stochastic forces and dampingeect (see Box2).

    The main mathematical aspect of the early theories ofBrownian motion was the `central limit theorem', whicham- ounted to the assumption that for a suciently large

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    Box 2. Brownian Motors

    One of the topics of current research activity employing these techniques is referred to as Brownian motors.

    This phrase is used for the systems rectifying the inescapable thermal noise to produce unidirectional

    current of particles in the presence of asymmetric potentials. Their study is relevant for understanding the

    physical aspects involved in the movement of motor proteins, the design and construction of efficient

    microscopic motors, development of separation techniques for particles of micro- and nano-size, possible

    directed transport of quantum entities like electrons or spin degrees of freedom in quantum dot arrays,

    molecular wires and nano-materials; and to the fundamental problems of thermodynamics and statistical

    mechanics such as basing the second law of thermodynamics on statistical reasoning and depriving the

    Maxwell demon type devices of their mystique and the trade-off between entropy and information.

    3 This result will be obtained in

    the next section of this article;

    see equation (8).

    The main

    mathematical aspect

    of the early theories

    of Brownian motion

    was the central limittheorem, which

    states that the

    distribution function

    for random walk is

    quite close to a

    Gaussian.

    number of steps, the distribution function for randomwalk is quite close to a Gaussian. However, since thetrajectory of a Brownian particle is random, it growsonly as square root of time3 and, therefore, one cannotdene its derivative at a point. To handle this problem,N Wiener (1923) put forward a measure theory whichformed the basis of the so-called stable distributions orLevy distributions. As a follow-up of these and to givea rm footing to the theory of Brownian motion, Ito

    (1944), developed stochastic calculus and an alternativeto Brownian motion { the Geometrical Brownian mo-tion. This, in turn, led to extensive modeling for thenancial market, where the balance of supply and de-mand introduces a random character in the macroscopicprice evolution. Here the logarithm of the asset price isgoverned by the rules for Brownian motion. These as-pects have enlarged the scope of applicability of theoret-ical methods far beyond Einstein's random walks. Theseconcepts have been fruitfully exploited in a multitude of

    phenomena in not only physics, chemistry and biologybut also physiology, economics, sociology and politics.

    The Random Walk Model for Brownian Motion

    While tottering along, a drunkard is not sure of his steps;these may be forward or backward or in any other di-rection. Besides, each step is independent of the one

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    taken. Thus, his motion is so irregular that nothingcan be predicted about the next step. All one can talkabout is the probability of his covering a specic distance

    in given time. Such a problem was originally solvedby Markov and therefore, such processes are known asMarkov processes. Einstein adopted this approach to

    obtain the probability of the Brownian particle coveringa particular distance in time t. The randomness of thedrunkard's walk has given this treatment the name `ran-

    dom walk model' and in the case of a Brownian particle,the steps of the walk are caused by molecular collisions.

    To simplify the derivation, we consider the problem inone-dimension along x-axis, taking the position of theparticle to be 0 at t = 0 and x(t) at time t and makethe following assumptions.

    1. Each molecular impact on the particle under obser-vation takes place after the same interval 0(10

    8s) sothat the number of collisions in time t is n = t=0 (ofthe order of 108).

    2. Each collision makes the Brownian particle jump bythe same distance which turns out, we will see, to beabout 1nm, for a particle of radius 1m in a uid withthe viscosity of water, at room temperature along eitherpositive or negative direction with equal probability and is much smaller than the displacement x(t) which weresolve through the microscope only on the scale of am of the particle.

    3. Successive jumps of the particle are independent of

    each other.

    4. At time t, the particle has net positive displacementx(t) (it could be equally well taken as negative) so thatout of n jumps, m(= x(t)=, of the order of 103) extra

    jumps have taken place in positive direction. Since nand m are quite large, these are taken as integers.

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    In view of the four assumptions above, the total numberof positive and negative jumps, respectively, is (n+m)=2

    and (n m)=2. Since the probability that n indepen-dent jumps, each with probability 1/2, have a particu-lar sequence is (1=2)n, the probability of having m extrapositive jumps is given by

    Pn(m) = (1=2)(1=2)nfn!=[(n + m)=2]![(nm)=2]!g;

    (1)

    where the factor (1/2) comes from normalization m

    Pn(m) = 1. While writing this expression, we have notused any restriction on n and m except that both areintegers. So it holds good even for small n and m. Notethat both n and m are either even or odd. As an il-lustration, if we consider 8 jumps, then the probabilities

    for m = 0; 2;4 and 8 are 35/256, 7/64, 7/128 and 1/512,respectively.

    For large n we can use the approximation n! = (2n)1=2

    (n=e)n, so that for large n and m, equation(1) nally

    becomes

    Pn(m) = (1=2n)1=2exp(m2=2n): (2)

    Substituting m = x= and n = t=0, this yields theprobability for the particle to be found in the interval xto x + dx at time t as

    P(x)dx = (1=4Dt)1=2exp(x2=4Dt)dx; (3)

    with D = 2=20 . It may be mentioned that taking m tobe large mathematically means that is innitesimally

    small for a nite value of x. This aspect has enabledus to switch over from discrete step random walk to a

    continuous variable x in the above expression.

    In order to understand the physical signicance of thesymbol D, recall that if the linear number density ofsuspended particles in a uid is N(x; t) and their con-

    centration is dierent in dierent regions, diusion takes

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    The proportionality of

    root mean square

    displacement of theBrownian particle to

    the square root of

    time is a typical

    consequence of the

    random nature of the

    process.

    place. This is governed by the diusion equationD0(@

    2N(x; t)=@x2) = @N(x; t)=@t; (4)

    where D0 is the diusion coecient. Equation (4) hasone of the solutions as

    N(x; t) = (Ntot=pf4D0tg)exp(x

    2=4D0t): (5)

    Here,

    Ntot

    =Z1

    1N(x;t)dx (6)

    is the total number of particles along the x-axis. Ob-viously, N(x; t)=Ntot corresponds to P(x) if we identify

    D as D0 , i.e, 2=20 as diusion coecient. In other

    words, P(x) is a solution of the diusion equation mean-ing thereby that the random walk problem is intimatelyrelated with the phenomenon of diusion. In fact, the

    random walk model is a microscopic phenomenon of dif-fusion.

    A look at (3) shows that the probability function de-scribing the position of the particle at time t is Gaussianwith dispersion 2Dt (Figure 2) implying spread of thepeak width as square root of t. Furthermore, mean val-ues ofx(t) and x2(t) turn out to be

    hx(t)i = 0 and hx2(t)i = 2Dt: (7)

    Since hx(t)i = 0, the physical quantity of interest ishx2(t)i. So what one measures experimentally is theroot mean s quare displacement of the Brownian particlegiven by

    xrms = hx2(t)i1=2 = (2Dt)1=2: (8)

    The proportionality of root mean square displacementof the Brownian particle to the square root of time is atypical consequence of the random nature of the process

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    0

    0.2

    0.4

    0.6

    0.8

    1

    1.2

    -5

    -4.7

    -4.4

    -4.1

    -3.8

    -3.6

    -3.3 -

    3

    -2.7

    -2.4

    -2.1

    -1.8

    -1.5

    -1.2

    -0.9

    -0.7

    -0.4

    -0.1

    0.2

    2

    0.5

    1

    0.8

    1.0

    9

    1.3

    8

    1.6

    7

    1.9

    6

    2.2

    5

    2.5

    4

    2.8

    3

    3.1

    2

    3.4

    1

    3.7

    3.9

    9

    4.2

    8

    4.5

    7

    4.8

    6

    Series1

    Series2

    Series3

    Figure 2. Plot of (4Dt)1/2

    P(x) (equation(3)) versus x

    for D= 5.221013m2s1andx varying from 5.0 mm to

    5.0 mm corresponding to t

    values 1s (the innermost

    curve), 2s (the middle

    curve), and 4s (the outer-

    most curve ).

    and is in contrast with the result of usual mechanicalpredictable and reversible motion where displacement

    varies as t. For three dimensional motion, the aboveexpression becomes

    hr2(t)i = hx2(t)i + hy2(t)i + hz2(t)i = 6Dt: (9)

    From equation (7), we have

    D = hx2(t)i=2t; (10)

    which connects the macroscopic quantity diusion con-stant D or D0 with the microscopic quantity the mean

    square displacement due to jumps. It gives us a di-rect relationship between the diusion process, which isirreversible, and Brownian movement that has its ori-

    gin in random collisions. In other words, irreversibilityhas something to do with the random uctuating forcesacting on the Brownian particle due to impacts of themolecules of the surrounding uid.

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    4 One such well-investigated

    topic is that of quantum ran-

    dom wa lks a natural exten-

    sion of classical random walks.

    Though the ma in emphasis in

    these studies has been on

    bring ing out the differences in

    their behaviour as compared

    to the classical analogs, it is

    believed that this knowledge

    will be helpful in developing

    algorithms that can be run on a

    quantum computer as and

    when it is practically realized.

    The successful use of the concept of random walk in thetheory of Brownian motion encouraged physicists to ex-ploit it in dierent elds involving stochastic processes.4

    Langevin's Theory of Brownian Motion

    The intimate relationship between irreversibility and ran-domness of collisions of the uid molecules with the

    Brownian particle (mentioned above) prompted Langevin(1908) to put forward a more logical theory of Brown-ian movement. However, before proceeding further, we

    digress to consider the motion of a hockey ball of massM being hit quickly by dierent players. Its motion isgoverned by two factors. The frictional force fd betweenthe surface of ball and the ground tends to slow it down,while the impact of the hit with the stick by a player in-

    creases its velocity. The eect of the latter, of course, isquite random as its magnitude as well as direction de-pend upon the impulse of the hit. Since a hit lasts for

    only a very short t ime, we represent the magnitude fj ofcorresponding force at time tj by a Dirac delta function( Box3 ) of strength Cj

    fj(t) = Cj(t tj); (11)

    and write the equation of motion pertaining to this forceas

    Mjdv=dtj = fj : (12)

    To nd the eect of the hit in changing the velocity,we substitute (11) into (12), integrate on both the sideswith respect to time over a small time interval aroundtj and use the property of delta function to get

    Mjvj j = Cj: (13)

    Here, vj is the change in velocity brought about by

    the hit at time t = tj. Now, the hits applied by dierentplayers can be in any direction, the total force exerted

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    Box 3. The Dirac Delta Function

    Many times we come across problems in which the sources or causes of the observed effects are nearly

    localized or almost instantaneous. Some such examples are : point charges and dipoles in electrostatics;

    impulsive forces in dynamics and acoustics; peaked voltages or currents in switching processes; nuclear

    interactions, etc. To handle such situations, we use what is known as Dirac delta function. It represents an

    infinitely sharply peaked function given, for one-dimensional case, by

    =

    =

    0

    0

    0

    0)(

    xx

    xxxx

    but such that its integral over the whole range is normalized to unity :

    =

    .1)(0

    dxxx

    Its most important property is that for a continuous function f(x)

    =

    ).()()(00

    xfdxxxxf

    Thus, (x x0) acts as a sieve that selects from all possible values off(x) its value at the pointx

    0, where

    the function is peaked. Accordingly, the above result is sometimes called sifting property of function.

    on the ball in a nite time interval will be obtained by

    summing up the above expression over a sequence of hitsmade taking into account the directions of the hits. Thisforce can be written as

    fr(t) = jCjj(t tj); (14)

    where j is unit vector in the direction of hit at timet = tj . The subscript r in (14) has been used to indicate

    the randomness of the force vector. Thus, the total forceacting on the ball at any time t will be fd + fr and itsequation of motion will read

    Mdv=dt = fd + fr: (15)

    Furthermore, if a very large number of hits are appliedquickly over a long time interval as compared to theimpact time, all possible directions j will occur com-pletely randomly with equal probability. Accordingly,

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    Figure 3. A large Brownian

    particle surrounded by ran-

    domly moving relatively

    smaller molecules of the

    fluid.

    average value of fr will be zero, i.e.,

    hfr(t)i = 0:

    Reverting to the Langevin's theory, we consider Brown-ian particle in place of the hockey ball in the above illus-tration and make the following simplifying assumptions.

    1. The Brownian particle experiences a time-dependentforce f(t) only due to molecular impacts from the sur-rounding particles (Figure3) and there is no other exter-nal force ( such as gravitational, Coulombic, etc.) actingon it.

    2. The force f(t) is made up of two parts: fd and fr(t).

    The former is an averaged out, systematic or steadyforce due to frictional or viscous drag of the uid, whilethe latter is a highly uctuating force or noise arising

    from the irregular continuous bombardment by the uidmolecules. The equation of motion of the particle isgiven by (15).

    3. The steady force fd is governed by the Stokes formula(Box 4) so that

    fd = v: (16)

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    Box 4. Stokes Formula

    Following Stokes we assume that a perfectly rigid body (say, a sphere) with completely smooth surface and

    linear dimension l is moving through an incompressible, viscous fluid ( viscosity, density ) having an

    infinite extent in such a manner that there is no slip between the body and the layers of the fluid in its

    contact, with such a speed v that the motion is streamlined and the Reynolds number R ( = vl/) is very

    small (strictly speaking vanishingly small), then the viscous drag force fdon the body is proportional to

    velocity v,i.e. fd

    = v; and the constant depends on the geometry of the body. For example, it is 6a

    for a sphere of radiusa and is 16a for a plane circular disc of radiusa moving perpendicular to its plane.

    Here, is viscous drag coecient and

    1== jvj=jfdj (17)

    is mobility of the Brownian particle. The drag coecient

    depends upon viscosity of the uid, geometry as wellas size of the Brownian particle. For a spherical particleof radius a,

    = 6a: (18)

    4. The coecient of viscous drag is a constant, havingthe same value in all parts of the uid and at all times.

    5. The random force fr(t) is independent of v(t) andvaries extremely fast as compared to it so that over a

    long time interval (much larger than the characteristicrelaxation time ), the average offr(t) vanishes (as elab-orated above for a hockey ball), i.e.,

    hfr(t)i = 0: (19)

    This essentially amounts to saying that the collisionsare completely independent of each other or are uncor-

    related.

    Substituting (16) into (15), we get

    M(dv=dt) = v + fr(t); (20)

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    where fr(t) satises the condition given in (19).This isthe celebrated Langevin equation for a free Brownianparticle. fr(t) is usually referred to as `stochastic force';(20) is the stochastic equation of motion and is the basic

    equation used for describing a stochastic process. Thesolution to (20) reads

    v(t) = v(0)exp(t=) + exp(t=)

    Zt0

    exp(u=)A(u)du;

    (21)

    and gives us the drift velocity of the Brownian particle.Here,

    = M= (22)

    is the relaxation time of the particle and

    A(t) = fr (t)=M (23)

    is the stochastic force per unit mass of the Brownianparticle and is generally called `Langevin force'.

    It may be mentioned that the rst term in (21) is thedamping term and it tries to exponentially reduce thevalue of v(t) to make it essentially dead. On the otherhand, the second term involving Langevin force or noisecreates a tendency for v(t) to spread out over a contin-ually increasing range of values due to integration and,thus, keeping it alive. Consequently, the observed valueof drift velocity at any time t is an outcome of these twoopposing tendencies.

    From (19) and (23), it is clear that hA(t)i = 0 so thatthe average value of drift velocity in (21) becomes

    hv(t)i = v(0)exp(t=): (24)

    Obviously, average drift velocity of the Brownian parti-cle decays exponentially with a characteristic time tillit becomes zero. This is a typical result for dissipative

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    5 For details of this step see

    Statistical Mechanics by R K

    Pathria listed at the end.

    or irreversible processes. But, this is physically not ac-ceptable as ultimately the particle must be in thermalequilibrium with its surroundings at ambient tempera-ture and, therefore, cannot b e at rest. So we considerhv2(t)i = hv(t):v(t)i. Substituting for v(t) from (21)and using the fact that hA(t)i = 0, we have

    hv2(t)i = v2(0)exp(2t=) + exp(2t=)

    Zt

    0Z

    t

    0

    exp(u1 + u2)=)K(u2 u1)du1du2; (25)

    where

    K(u2 u1) = hA(u1):A(u2)i: (26)

    It is called autocorrelation function for the Langevin

    force A(u) and involves u2 u1 to emphasize the factthat for Brownian motion it depends upon the time in-terval u2 u1 rather than actual values of u1 and u2.We assume that K(u2 u1) is an even function of its

    argument and is signicant only for u2 almost equal tou1. Using these ideas when the double integral in (25)is evaluated, we get5

    hv2(t)i = v2(0) + [v2(1) v2(0)][1 exp(2t=)]:(27)

    Here, hv2(1)i is the mean square velocity of the Brown-

    ian particle for innitely large value of t and is expectedto be the value corresponding to the situation when thesystem is in equilibrium at temperature T. Thus, from

    equipartition theorem(1=2)Mv2(1) = (3=2)kT: (28)

    As a special case ifv2(0) equals the equipartition value3kT=M, then hv2(t)i = v2(0) = 3kT=M implying thatif the system has attained statistical equilibrium then itwould continue to be so throughout.

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    The Einstein relation

    gives a relationship

    between the diffusion

    coefficient and

    mobility of the particle

    and hence the

    viscosity of the fluid.

    Thus, viscosity of a

    medium is a

    consequence offluctuating forces

    arising from their

    continuous and

    random motion and is

    an irreversible

    phenomenon.

    It may be noted that multiplying (20) with r(t)=M,where r(t) is the instantaneous position of the Brownianparticle, we nally get

    d2hr2i=dt2 + (1=)(dhr2i=dt) = 2hv2(t)i; (29)

    here hv2(t)i is given by (27). This second order dier-ential equation, on being solved, gives

    hr2(t)i = v2(0)2f1 exp(t=)g2 (3kT=M)2

    f1 exp(t=)gf1 exp(t=)g + (6kT=M)t: (30)

    For t very small as compared to it yields

    hr2(t)i = v2(0)t2; (31)

    so that root mean square displacement rrms = hr2(t)i1=2

    is proportional to t as for a reversible process. On theother hand, for t , we get

    hr2(t)i = (6kT=m)t = (6kT=)t (32)

    implying that

    rrms(t) = (6kT=)1=2t1=2 : (33)

    Expression (32) becomes identical to (9) if we take

    D = kT=; (34)

    which in view of (18) reads

    D = kT=6a (35)

    for a spherical Brownian particle. Equation (34) is usu-ally known as `Einstein relation'. Obviously, it gives arelationship between the diusion coecient and mobil-ity of the particle and hence the viscosity of the uid.Thus, viscosity of a medium is a consequence of uctu-

    ating forces arising from their continuous and randommotion and is an irreversible phenomenon.

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    6 This derivation is given, e.g.,

    in ar ticle 1.6 in Nonequilibrium

    Statistical Mechanics b y R

    Zwanzig (Oxford University

    Press, Oxford, 2001).

    7 See R Zwanzig, J. Stat. Phys.,

    Vol.9, p.215, 1973.

    At this stage it is in order to mention one of the ex-perimental observations by Perrin and Chaudesaigues.They studied the mean square displacement of gambogeparticles of radius 0.212 m in a medium with viscos-

    ity 0.0012 Nm2s and maintained at a temperature of186 K. The values found along the x-axis at times 30,60, 90 and 120 seconds, respectively, were 45, 86.5, 140,195 1012m2 . These give the mean value of squared

    displacement for 30 seconds as 48:75 1012m2. Now,from (7) and (35), we have

    hx2

    (t)i = (kTt=3a); (36)

    which on substituting the above listed values yields k =1:36 1023JK1 . Clearly, it is quite close to the ac-cepted value of the Boltzmann constant except that thedeviation is reasonably large.

    It may be mentioned that the Langevin equation (equa-tion (20)) was based on the assumptions enumerated inthe beginning of this section. However, in a real systembeing used for the observation of Brownian motion, some

    external force fext(t) may be present; the viscous dragforce fd may be a function of higher powers of velocityor some other function of v(t); the drag coecient maynot be a constant and rather may depend upon v, t oreven position. In such a case this equation is modiedto a general form

    M(dv=dt) = (v;x ; t)F(v) + fr(t) + fext(t): (37)

    It is worthwhile to point out that the Langevin equa-tions can also be obtained by assuming the Brownian

    particle to be interacting bilinearly with a large num-ber of harmonic oscillators constituting a heat bath6 .This approach yields explicit expressions for the dragforce fd as well as the stochastic force or noise fr(t) and,thus, provides better insight into their mechanism but

    still does not make the theory very rigorous7 . The lattertask is achieved by using the so called master equation

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    Address for Correspondence

    Shama Sharma

    Department of PhysicsDAV College

    Bathinda 151 01

    Punjab, India

    Vishwamittar

    Department of Physics

    Panjab University

    Chandigarh 160 014, India.

    Email:[email protected];

    [email protected]

    8 See H Risken, The Fokker

    Planck Equation: Methods of So-

    lut ion and Appl icat ions,

    Springer, 1996.

    Suggested Reading

    [1] E S R Gopal,Statistical Mechanics and Properties of Matter, Macmillan

    India, Delhi, 1976.

    [2] W Paul and J Baschnagel,Stochastic Processes from Physics to Finance,

    Springer- Verlag, Berlin, 1999.

    [3] R K Pathria,Statistical Mechanics, Butterworth-Heinemann, Oxford,

    2001.

    [4] J Klafter, M F Shlesinger and G Zumofen, Beyond Brownian Motion,

    Physics Today, Vol. 49, No. 2, pp .33-39, 1996.

    [5] A R Bulsara and L Gammaitoni, Tuning in to noise,Physics Today, Vol.

    49, No. 3, pp. 39-45, 1996.

    [6] M D Haw, Colloidal Suspensions, Brownian Motion, Molecular reality:

    a Short History,J. Phys.: Condens. Matter , Vol. 14, pp .7769-79, 2002.

    [7] R D Astumian and P Hanggi, Brownian Motors,Physics Today, Vol. 55,

    No. 11,pp.33-39, 2002.

    [8] D Ruelle, Conversations on Nonequilibrium Physics with an

    Extraterrestial,Physics Today, Vol. 57, No. 5, pp.48-53, 2004.

    for the time rate of variation of probability distributionfunction and its simplied version { the Fokker{Planckequation.8 However, we do not propose to go into thesedetails here.

    Sir Isaac Newton had a theory of how to get the

    best outcomes in a courtroom. He suggested to

    lawyers that they should drag their arguments

    into the late afternoon hours. The English judges

    of his day would never abandon their 4 oclock

    tea time, and therefore would always bring

    down their hammer and enter a hasty, positive

    decision so they could retire to their chambers

    for a cup of Earl Grey.

    This tactic used by the British lawyers is still

    recalled as Newtons Law of Gavel Tea in

    legal circles.