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Quantum Brownian motion in a periodic potential: a pedestrian approach

C. Aslangul, N. Pottier, D. Saint-James

To cite this version:

C. Aslangul, N. Pottier, D. Saint-James. Quantum Brownian motion in a periodic po- tential: a pedestrian approach. Journal de Physique, 1987, 48 (7), pp.1093-1110.

�10.1051/jphys:019870048070109300�. �jpa-00210531�

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Quantum Brownian motion in a periodic potential: a pedestrian approach

C. Aslangul (1,*), N. Pottier (1) and D. Saint-James (2,**)

(1) Groupe de Physique des Solides de l’Ecole Normale Supérieure (+), Université Paris VII, 2, place Jussieu, 75251 Paris Cedex 05, France

(2) Laboratoire de Physique Statistique, Collège de France, 3,

rue

d’Ulm, 75005 Paris, France

(Requ le 26 janvier 1987, accepté le 6

mars

1987)

Résumé.

2014

La dynamique d’une particule quantique couplée à

un

environnement de manière ohmique et

se

déplaçant dans

un

potentiel périodique est étudiée au moyen d’un développement direct de perturbations de l’équation du mouvement par rapport à l’amplitude des ondulations du potentiel. Ainsi,

en

faisant uniquement appel à la mécanique quantique élémentaire, nous calculons la mobilité de cette particule Brownienne dans les deux cas d’une force extérieure finie et constante et d’une petite force appliquée harmonique. La mobilité

statique est reliée à la mobilité d’une particule

sur

un réseau décrit en liaisons fortes par une transformation de dualité établie antérieurement. De plus, un calcul de réponse linéaire en présence d’une petite force appliquée harmonique montre que la particule

se

comporte comme une particule libre équivalente

avec un

coefficient de frottement modifié (dépendant de la fréquence), et, en conséquence, avec

un

spectre de bruit modifié, ces

deux quantités étant reliées par le théorème de fluctuation-dissipation.

Abstract.

2014

The dynamics of

a

quantum particle coupled to an environment in an ohmic way and moving in

a

periodic potential is examined by means of a direct perturbation expansion of the equation of motion with respect to the amplitude of the potential (corrugation strength). Thus, by using only elementary quantum mechanics, we calculate the mobility of this Brownian particle in both cases of

a

finite and constant external force and of

a

small applied harmonic force. The static mobility is found to be related to that of

a

particle in a tight-binding lattice by

a

duality transformation previously demonstrated. Besides, it is shown by

a

linear

response calculation in the presence of

a

small applied harmonic force that the particle behaves like

an

equivalent free particle with a modified (frequency-dependent) friction coefficient, and, consequently,

a

modified noise spectrum, both being related by the fluctuation-dissipation theorem.

Classification

z

Physics Abstracts 05.30

-

05.40

1. Introduction.

In the present paper, we would like to investigate, using only elementary quantum mechanics, the mo-

tion in a periodic potential of a particle in the

presence of ohmic dissipation, that is of a particle

described by a Langevin equation with a constant

friction coefficient or, which amounts to the same, with white noise in the classical (high-temperature)

limit. For such a Brownian particle, the Heisenberg representation of the coordinate q (t ) obeys the equation of motion

In equation (1), q denotes the friction coefficient,

V (q ) is the periodic potential ; F s (t) is a systematic (not random) applied external force and Fr (t ) is a

random force with known spectral properties.

As is well known, this equation of motion can be

obtained by properly coupling the particle to a bath

of an infinite number of degrees of freedom, the coupling to the environment providing both the

friction term and the fluctuating force. A very simple

model which has been extensively studied in the last past years is the Caldeira-Leggett model [1], in

which the coordinate q of the particle is linearly coupled to an infinite set of harmonic oscillators.

The Hamiltonian of the total system (particle plus bath) is given by

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:019870048070109300

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For such a linear coupling, one obtains an equation

of motion for q (t ) which in general differs from equation (1) since it contains a retarded friction

term. The microscopic expressions for both the

friction term and the fluctuating force can be ob-

tained [2] : the fluctuating force is a linear combi- nation of the creation and annihilation operators of the boson bath and the friction coefficient is linked to the spectral density of the fluctuating force by the fluctuation-dissipation theorem. Following [1], one

then goes to a continuous representation for the bath

modes and sets the simple prescription about the

bath density of modes p (w ) and the coupling

constant G «(JJ ) of the particle to the bath :

where Ie (CJJ / CJJ e) is some cut-off function such that

Ie (0) = 1 and decreasing on a frequency range of order wc (ohmic dissipation model). By rejecting

CJJ e to infinity, it is possible to derive an equation of

motion of type (1), in which the friction term is

instantaneous.

In the absence of any potential, or in a quadratic potential, the solution of equation (1) is fairly simple, since this equation is linear with respect to

the particle coordinate. One can either calculate the time evolution of average quantities, such as the

average particle position, and thus obtain the

mobility, or calculate correlation functions, which yield for instance the expression of the diffusion coefficient. The properties of a damped quantum free particle and of a damped quantum harmonic oscillator have been investigated in detail along

these lines by several authors [2-6].

However, for other types of potentials, non-

linearities arise so that a solution of equation (1) can only be obtained by approximate methods ; this is

the case of the periodic potential of the form

studied first by M. P. A. Fisher and W. Zwerger [7],

and later on by W. Zwerger [8]. Actually, the

calculations performed in references [7] and [8]

primarily concern a tight-binding lattice. Indeed, as

was shown by A. Schmid [9] and by M. P. A. Fisher

and W. Zwerger [7], there exists a duality transform-

ation between the periodic potential (4) and an appropriate tight-binding model, the hopping inte- gral being proportional to V. This duality transform-

ation yields a relation between the mobilities of the

particle in both situations.

Besides, a direct calculation of the mobility of the particle in a periodic potential of the form (4) has

been recently proposed by U. Eckem and F. Pelzer

[10]. They use field-theoretical methods based on

the Keldysh formalism and they determine the generating functional for real-time finite-tempera-

ture correlation functions ; the mobility of the par- ticle is expressed in terms of a self-energy, which

itself is calculated through a perturbation expansion

with respect to the potential strength. An expression

for the frequency-dependent particle mobility in the

linear response range is thus obtained.

Actually, since the quantum statistical properties

of a free particle in the presence of ohmic dissipation

are well known [2, 3], one is led to think that for

some

«

weak » potentials, the effect of the potential

on the particle may be treated as a perturbation

around its free Brownian motion. The potential (4)

can easily be handled in this way and the clue to a solution of this problem lies in the following fact :

since the fluctuating force Fr (t ) acting on the quantum Brownian particle is a linear combination of the boson bath creation and annihilation operators, all the statistical properties of not only

the free particle position operator qo (t ) but equally

of sin { Qo (t ) } can be known (where we have

defined the dimensionless position operator Qo (t )

=

(2 7T fa) qo (t )). Indeed, in the following we

show that the average value and the correlation functions of sin { Qo (t )} can be expressed simply in

terms of the corresponding quantities for qo (t ) itself.

This property is the quantum analog of the following

well-known property of classical random processes : if Fr (t ) is a Gaussian fluctuating force, qo (t ) is also a

Gaussian random process, and the statistical proper- ties of exp {i Qo (t )} can be calculated in terms of the first two cumulants [11, 12]. However, in the quan-

tum case, the calculations are made a little more

difficult since the position operators at different

times do not commute [13]. In the present paper, we take advantage of the Gaussian-like property of the

boson variables to calculate by a direct simple perturbation expansion of equation (1) with V (q ) as given by equation (4) all the statistical properties of

the particle position and velocity at the lowest non-

zero order with respect to the corrugation strength.

If we assume that the particle and the bath have been in thermal equilibrium in the infinite past, by

this extremely straightforward and transparent ap-

proach we recover the results of the field-theoretical method developed in reference [10]. Our calcula- tions can be achieved either for a finite external force (non-linear situation), or in a linear response limit.

The paper is organized as follows : in section 2, we outline the principle of the perturbation expansion

of the equation of motion.

In section 3, we restrict the study to the case of a

finite and constant external force Fs; the static non-

linear mobility of the particle in the presence of ohmic dissipation in a periodic potential is calculated

and is shown to be related, as expected, to the

(4)

mobility in a tight-binding lattice [7, 8,14] by the duality transformation [7, 9].

In section 4, we consider the case of a small harmonic applied force F s (t) and we derive the frequency-dependent mobility and diffusion coef- ficients. The results obtained can be given a very

simple physical interpretation : in the presence of a

periodic potential, the particle behaves like an equivalent free particle (with possibly a mass renor-

malization) subjected to a modified (frequency-de- pendent) friction coefficient, and, consequently, to a

modified noise spectrum, both being related by the fluctuation-dissipation theorem.

2. The perturbation expansion.

2.1 THE MODEL. - With the potential V (q ) as given by formula (4), equation (1) reads :

where a is the period of the potential and V is an

energy characterizing the amplitude of its variations

(corrugation strength). We shall see in the sequel

that the motion of the particle obeying equation (5)

can be handled as a perturbation around the Brow-

nian motion of the same particle subjected to the

same friction and to the same noise, but in the

absence of potential, provided that V remains much

smaller than an energy of the order of 1í’Y, with

y = 11 / M. Note that, since y-’ represents the relaxation time of the free Brownian particle, this

condition on the amplitude V of the potential also

means that the time scale associated with V must remain much larger than the relaxation time of the free Brownian particle.

2.2 SUMMARY OF THE FREE PARTICLE RESULTS.

-

For a free particle with ohmic dissipation, the equation of motion reads simply :

Let us recall that since in equation (6), the friction

term is instantaneous, the free particle results have

to be used in the infinitely short memory time limit

(WC --+ 00).

To specify the statement of the problem com- pletely, it is necessary to give some information about the initial preparation of the system (particle plus bath). We shall assume, as in our study of the quantum Brownian motion of a free particle [2], that

the particle has been put in contact with the bath

-

itself in thermal equilibrium at temperature T - at a time to

= -

oo so that at any finite time the system

(particle plus bath) has reached a thermal equilib-

rium state. This is also the hypothesis made by U.

Eckem and F. Pelzer in [10]. This hypothesis

eliminates transient phenomena and the average

over the particle initial velocity is automatically

built-in in the calculations. Thus, only the average

over the bath variables will have to be carried out in the following. Moreover, this choice of the initial time insures that all the correlation functions will

depend only on the time differences. The fluctuating

force Fr (t ) corresponds to a stationary random

process. In terms of the boson bath creation and annihilation operators, its microscopic expression is

(see Eq. (2) for the definition of the coupling

constants Gn). The average value of Fr (t ) is equal to

zero. In the ohmic dissipation model (3) with

wc

-

oo, the spectral density of the random force is

[2] : 1

Note that, owing to the quantum character of the bath operators, the operators Fr (t ) and Fr(O) do not

commute.

Before proceeding to the perturbation expansion

of the equation of motion (5), let us briefly recall

some properties of the trajectory qo(t) of the free

Brownian particle. Clearly, qo (t ) is the sum of a systematic part, which we shall denote as qOs(t), and

of a random part qor (t ). Whereas the systematic part

depends on the applied force and corresponds to the

average particle trajectory, the fluctuating part is only a function of the bath operators. Namely, one gets

and, similarly

QOr(t) is equal to zero on average, and its quadratic

mean value is given by :

with the function A2(t) as defined by

(5)

Note the appearance of the dimensionless parameter

a

which is a measure of the dissipation strength in

the periodic potential

The spectral density associated with QOr(t) is :

At this point it is important to emphasize that the position operators at different times do not com-

mute. By using the formula

.

(see for instance Ref. [2]), one readily shows that

where the function A1 (t ) is given by

Note that, since to has been rejected to - oo,

equation (16) depends only on the difference t - t’.

2.3 PERTURBATION EXPANSION.

-

Let us write the

particle coordinate under the form

with successive terms of increasing order in V.

Clearly, qo (t ) obeys equation (6) while that the first- order correction q 1 (t) satisfies

Equation (19) is analogous to the free Brownian

motion equation (6), the quantity

now playing the role of the force.

Equation (19) can formally be integrated, yielding

In order to calculate the corresponding first-order correction to the particle mobility, one has to

evaluate (S (t )) , or (exp{:tiQo(t)}). The free

particle position qo (t ) is the sum of two commuting quantities, the systematic part qos (t ) and the fluctuat-

ing part qor(t). Clearly

Since qor (t ) is a linear combination of the bath

operators, it is easily seen that

or, since (Qor(t»

=

0,

The r.h.s. of the above equation is real, and one simply gets :

In other words, the average first-order force felt by

the particle is equal to zero, so that there is no first- order correction to the mobility. This is coherent with the fact that the sign of V cannot play any role in the expression of mobility. (Note that the integral

in the exponent diverges, as a consequence of the ohmic dissipation law).

One must therefore study the second-order correc-

tions. The equation of motion at second-order is

where the notation sin {Qo (t) + Q 1 (t )} (1) means

that only first-order terms must be retained in the

development of this quantity. This development has

to be achieved with some caution, owing to the fact

that the operators qo (t ) and q1(t) do not commute.

By properly differentiating the exponential operators

[15-17], one obtains

The detailed derivation of this operator identity is explained in appendix A.

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It is now necessary to compute the series of commutators involved in equation (27). This calculation is carried out in appendix B. As a result, one finds that the second-order equation of motion is :

where the functions 1 (t" - t ) and X2 (t " - t ) are

power series of the function A1 (t" - t ) :

In order to obtain the evolution of the second order correction to the average particle position q2 (t », it remains to calculate the correlation functions

and

where, as indicated above, the averages have to be carried out over the bath variables.

Two types of terms are a priori involved in this calculation, that is either terms of the type

in which the two exponentials have arguments of the

same sign, or terms of the type

with different signs of the arguments. The com-

mutator of the position operators at different times

being a c-number (see Eq. (16)), one has, according

to the Glauber formula

Note that only the first factor in equation (30) has to

be averaged. Proceeding in analogy with the calcu-

lation done to obtain formula (24), one can easily be

convinced that the terms with arguments of the same sign involve a divergent integral in the argument of

an exponential, and thus give a null contribution to the correlation functions. The only non-zero con-

tributions come from the terms with arguments of different signs, or, following a terminology used in

references [7-10], from the « neutral charge con- figurations

».

As a result, one gets :

so that:

Finally, by taking into account the developments (29) the equation of motion (28) can be averaged

into

To proceed further in the calculation, one has to specify the detailed time-dependence of the applied

external force FS (t ). In section 3 we shall first examine the case of a constant external force, not necessarily small ; then, in section 4, we shall study

the linear response to a small applied harmonic

force.

3. Finite constant external force.

In this section, we discuss in detail the behaviour of the mobility when the applied external force FS (t )

=

F is time-independent. No hypothesis will

be made about its intensity.

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3.1 CALCULATION OF THE MOBILITY.

-

We have

(see Eq. (9)) : 1

Inserting this result in formula (32), it appears that,

in the presence of a constant external force, the correlation functions

and

depend only on the time difference t" - t ; this is a consequence of the choice of the initial time to

= -

oo. This means that at any finite time a

stationary regime is obtained ; this is even more evidently displayed in the following.

Indeed, by using the explicit form (17) of the

function A1 (t ), the equation of motion (33) is easily

rewritten as :

The r.h.s. of the above equation being a constant,

the time-independent particle velocity is equal to

The corresponding static non-linear mobility A in the periodic potential is thus :

where

denotes the free particle mobility and E

=

Fa is the

energy drop over one period of the potential. Note

that in formula (37), the correction to the free

particle mobility JL 0 involves the ratio V / liy, which

indeed plays the role of an expansion parameter in the problem. This will be discussed more thoroughly

later.

3.2 DUALITY RELATION WITH THE MOBILITY IN A TIGHT-BINDING LATTICE.

-

The result of (37) for

the particle mobility in the periodic potential (4),

calculated to second order with respect to the

corrugation strength, involves an integral which is

identical to the mobility of a particle on a tight- binding lattice, at the same temperature and with the

same friction coefficient q [7, 14], provided that an appropriate correspondence between the other par- ameters of both models is taken into account. This is in accordance with a general theorem of A. Schmid [9] and of M. P. A. Fisher and W.

Zwerger [7], who have established that there exists a

duality transformation between the periodic poten- tial (4) and an appropriate tight-binding model, the hopping integral being proportional to V. In its most general form the duality relation [7, 9] reads (with

the appropriate parameters)

As ’a matter of fact, either in the tight-binding

lattice [14], or, as above, in the periodic potential (see formula (37)), we have shown that the particle mobility can be obtained by a very simple and direct perturbative treatment of the equations of motion.

Similar results are obtained for the periodic potential

in reference [10] by using the Keldysh method ; however, the formalism used in this paper is rather

complicated. Although the integral in (37) can be directly calculated, we shall take advantage of the correspondence (39) to use the results for the

mobility in a tight-binding lattice already obtained

for instance in references [7] and [14].

First, let us briefly recall what are the correspon- dence rules between the two models : while the temperature and the friction coefficient are the

same in both problems, the other parameters are related in a non-trivial manner. VTB

=

V /2 is the tight-binding hopping integral ; the dimensionless

dissipation strength and the lattice spacing in the tight-binding lattice are given by « TB = 1 / a and

aTB

=

a/« respectively. Moreover, the term corre- sponding to the product p «(ù ) 1 G «(ù ) 12 in the tight-

binding model is not simply given by IíTJ (ù / 7T as in

the periodic potential but is of the form

where

in other words, a Lorentzian cut-off is automatically

built-in in the tight-binding model, with the cut-off

frequency

ClJ

cTB

=

y

=

’T1 / M, which is not present in

the periodic potential.

Thus the form of the functions A1 (t ) and A2 (t ),

involved in equation (37), and defined by equations (17) and (12) respectively is a priori imposed by the equation of motion of the particle and should in principle be used in order to calculate J.L TB’ However,

we have shown in reference [14] that the mobility in

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the tight-binding lattice is in fact largely independent

of the precise form of the cut-off function provided

that one assumes that both the hopping integral VTB and the energy drop I £ I TB = a I F TB are much

smaller than hw cTB’ In terms of the parameters of the

periodic potential, it means that, if one assumes that

both V and

are much smaller than hy, the results will be largely independent of the precise form of the cut-off function. We shall take advantage of this property to

use at sufficiently low temperatures a different cut- off function (namely an exponential one,

fcTB (- / y )

=

exp (-

w

/ y ), for which the analytic

calculation has been performed in [14]). Thus,

instead of using the expressions (17) and (12) for the

functions Al (t ) and A2 (t ), we shall write :

and, for kB T « hy,

Let us now examine the physical meaning of the

two conditions required for deriving results indepen-

dent of the precise form of the cut-off function.

First, the ratio Vlhy clearly plays the role of the

expansion parameter in the problem ; indeed we

have supposed that the particle trajectory does not

much move away from the free Brownian particle trajectory. This evidently implies that the time scale associated with V must remain much larger than the

relaxation time M/q

=

y -1 of the free Brownian

particle. Similarly, the second condition I E I « a 9y

can be rewritten as

which means that the characteristic acceleration time of the particle by the applied force must equally

remain much larger than the relaxation time y -1 of

the free Brownian particle. Note that the two conditions V 9y and I e I

a

9y , which insure the

irrelevance (except for numerical factors) of the specific form of the cut-off function fcTB’

I

must be

satisfied in our perturbative approach. However,

f cTB is by construction a Lorentzian and, in the framework of a more refined calculation, the equiva-

lence between two different cut-off functions is not evident [8].

3.3 RESULTS FOR THE MOBILITY. - At this stage, it would be sufficient to refer to [7] and [14] which

treat the tight-binding lattice. Here we shall however

quote the main results for completeness and we postpone the physical discussion of the results as

well as of their validity to the subsequent paragraphs.

3.3.1 Low temperatures (kB T 9y ).

-

In this case

we use the exponential cut-off function ; the func-

tions A1 (t ) and A2(t) are given by equations (40)

and (41). The computation is then straightforward

and yields the

E

and T-dependent mobility tt ( E, T).

For the sake of simplicity, we shall only give here the

results corresponding to the two limits T -+ 0 and

e -+

0, although the full expression can be written

down without difficulty (see for instance Eq. (33) in

Ref. [14]).

(i) Zero-temperature limit

One obtains :

In this formula, it appears that, apart from the negligible exponential factor exp {- I e I / a fry} - 1,

the mobility depends only on the parameter

a result which has been demonstrated by W. Zwerger [8] by using scaling arguments. From now on, we shall drop the exponential factor in equation (43).

Note that, for

a >

1, the correction to 110 goes to

infinity when s - 0, so that the linear mobility does

not exist at zero temperature. This point is to be

discussed later on.

(ii) Finite temperature : linear limit

At finite temperature, a linear mobility can be

defined and reads

3.3.2 High temperatures (kB T > hy ).

-

In this

case we use the Lorentzian cut-off function. The functions At (t) and A2 (t) are now taken as given by equations (17) and (12). The s-dependence of the mobility is negligible in this temperature range [14].

In order to obtain a classical result, we follow the procedure of references [7] and [8]. We replace the

factor sin {At (t)} in equation (37) by its argument

and we approximate the function A2 (t) by

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Two different types of behaviour are observed, according to the value of the parameter

introduced by M. P. A. Fisher and W. Zwerger [7]

(w o

=

(2 w la) J V / M denotes the small classical oscillation frequency around one of the potential minima).

When the parameter K is much smaller than 1,

A2 (t) - Ky t, and one can replace sin f A, (t)) by its

argument provided that kB T > 9y. One obtains

When K is much higher than 1, A2 (t) - Ky 2 t2/2

and one can replace sin fA,(t)l by its argument

provided that kB T > Eo

=

4 7T 2 IP / Ma2. Eo is the

localization energy in a well of the potential and plays an important role in the problem, as we shall

see in the subsequent discussion. One obtains

Note that (47) and (48) are classical results, in

accordance with references [7] and [8]. This is the

reason why we used the classical parameter WO instead of (1/h) .JVEo.

3.4 DISCUSSION OF THE VALIDITY OF THE CALCU- LATION.

-

Let us now discuss the conditions of

validity of this perturbation expansion. As indicated above, the ratios V /9y and 1 8 1 /a hy must be small.

A necessary condition for the validity of the pertur- bation treatment is that the mobility in the periodic potential does not much differ from the free particle mobility. Since the result of the calculation takes the form of (39), it will be valid only as long as

,"TB (with the convenient parameters) remains much smaller than go.

3.4.1 Low temperatures (kB T 9y ).

(i) Zero-temperature limit

By looking at the appropriate expression (43) of

the mobility, one obtains the validity condition

For all

a

1, this condition is automatically fulfilled

since in our treatment both factors in equation (49)

have to be much smaller than 1, whereas for

« >

1, it implies that the applied force should be

high enough so that the energy drop over one period

satisfies

1

(As indicated above, the linear mobility stricto sensu

cannot be defined in this case).

This can be physically understood as follows : when a

>

1, the mobility in the tight-binding lattice (where aTB 1) increases when the applied force F

decreases while the mobility in the periodic potential

decreases. The system thus exhibits a tendency

towards localization. Note however that a completely

localized state would be meaningless in our perturba-

tive approach. In other words, formula (50) states

that the applied force has to be strong enough to prevent the particle from localizing.

(ii) Finite temperature : linear limit

At finite temperatures, a linear mobility can be

defined (Eq. (44)) and we will restrict the discussion

to this case. The validity condition reads :

For all

«

1, this condition is automatically fulfilled since both factors in equation (51) are small, whereas,

for a

>

1, it implies that the temperature should be high enough so that

This can be physically understood as follows : when

a >

1, the mobility in the tight-binding lattice

(where a TB 1) increases when the temperature

decreases while the mobility in the periodic potential

decreases. Formula (52) simply states that, in order

to obtain a sufficiently high mobility, the tempera-

ture has to be high enough to prevent the particle

from localizing

3.4.2 High temperatures (kB T > 1í’Y).

-

In the high-temperature range kB T >> hy, two different expressions for the mobility are obtained according

to the value of the parameter K as defined by equation (46).

When K 1, the validity condition is automati-

cally fulfilled as soon as the ratio V /9y is a small

parameter.

When K > 1, the quantity (VlkB T)312 (wo/y )

must remain much lower than 1. One must then have

which is not a very restrictive condition since

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To conclude this discussion, let us make some

comments about the physical meaning of the condi- tion V 1í’Y. It may seem at first sight that this

condition does not involve the period of the potential

or the localization energy Eo in a well of the

potential. However, it is interesting to rewrite the above condition in terms of

a.

Indeed, 1í’Y ==

a Eo/2 7T, so that the condition V 9y transforms

into

For

a

1, this condition automatically insures that

V Eo, which means there are no bound states and

the mobility does not differ very much from the

mobility go of the free particle. On the contrary, for

a >

1, condition (53) does not insure automatically

that there are no bound states. In this case, condi- tions (50) on the applied force or (52) on the temperature mean that the applied force or the

temperature must be sufficiently high to extract the particle from the possible bound state, or, in other words, that the bound state becomes irrelevant. The

perturbation treatment around the free Brownian motion is then justified.

__

The inequality V « 9wo (= ,,IVEO) (equivalent

to V Eo) could have been used to define a

«

weakly corrugated potential » [10]. Note that the

periodic potential has then no bound states. The foregoing discussion shows that potentials of larger amplitudes can indeed be studied by a perturbational

treatment around the free Brownian motion ; this is

the case if

a >

1 and if the applied force or the

temperature are sufficiently high.

To conclude this discussion, we can say that the

validity domain of the method is in fact very large,

and only excludes, when a

>

1, a small region in the vicinity of T or F equal to zero.

3.5 DISCUSSION OF THE RESULTS.

-

The discussion of the behaviour of the mobility as a function of the temperature and of the applied external force will

not be undertaken here in detail, since this has already been achieved in references [7, 8] (periodic potential and tight-binding lattice) and [14] (tight- binding lattice).

Let us however make some comments about our

results.

3.5.1 Classical regime.

-

At high temperatures, that is when kB T > hy, a comparison with the

results of a standard classical Langevin equation is possible. Two different types of behaviour are observed, according to the value of the parameter K (Eq. (46)). We have by hypothesis V « 9y « kB T.

(i) Let us first study the case where the parameter K is much smaller than 1 ; this can occur only if wo/y JV /kB T, which means that the classical

oscillator at the bottom of a potential well is strongly

overdamped. The classical regime is a diffusive one, governed by a Smoluchowski equation [7, 8], and, at high temperatures, the mobility > tends towards the free particle mobility tLo as T-2 (see formula (47)).

(ii) If instead the parameter K is much larger than 1, the only requirement on w o/ y is that

which is not very restrictive. The mobility > then

tends towards the free particle mobility uo as

T-312 (see formula (48)).

3.5.2 Quantum regime.

-

Let us first concentrate

on the case kB hy. When this condition is fulfilled, the mobility is given by equation (44).

However, the A-dependence of this expression is

rather intricate, since

a -

llh. For a > 1, formula (44) gives

so that quantum effects are certainly important for

Note the singularity in h In A in formula (54), which

is not uncommon in that kind of problem.

As shown by W Zwerger [8], for kB T >> hy, and

in the overdamped limit (K 1), which implies

a > 1, the quantum corrections are in h2. Thus,

when one goes from high (kB T > 9y ) to low (kB TT hy ) temperatures, the quantum corrections in the overdamped limit cross over from a h2

behaviour to a h In h one. This is explained in more

detail in appendix C.

When quantum effects can be neglected, formula (54) reduces to the classical result (47). It is interesting to note that formulae (44) (and (54)

which is deduced from it) on the one hand, and the

classical result (47) on the other hand were derived by using two different cut-off functions.

Finally, let us compare our result (37) with that of

U. Eckern and F. Pelzer [10]. They have found a

correction to the friction coefficient, due to cor- rugation, and it is easily seen that, for low values of this correction, their result and our result are

identical. They show that, since they formally obtain

a correction to the friction coefficient

-

and not to the mobility

-

their result for the mobility is always finite, but they do not assign precise validity limits to

their calculation. In our approach, the validity

domains of the two calculations of the mobility in the

(11)

periodic potential and in the tight-binding lattice are

the same, provided one takes into account the one-

to-one correspondence between parameters indi- cated above. The validity domain of the present calculation of the mobility in the periodic potential is precisely delineated : the calculation is valid either for

a

1 (and then the corrugation of the potential

is necessarily weak), or for a

>

1, where potentials

of larger amplitudes can be studied provided only

that the vicinity of either T or F equal to zero is

excluded.

4. Linear response to a small applied harmonic

force.

We shall now assume that a small harmonic force F s (t)

=

F e"’ is applied to the system and we shall study the linear response. Let us recall that, for a

free particle, the frequency-dependent mobility, or complex admittance J.L 0 (Cl) [18], is defined by

with

4.1 CALCULATION OF THE MOBILITY.

-

We use the results of section 2, and in particular, the equation of

motion (33). We have (see Eq. (9))

At the lowest order in F, the correlation functions which are involved in equation (33), that is

and

reduce to (see formula (32))

By using the explicit form (17) of the function Al(t), the equation of motion (33) can be rewritten

as

This formula shows that a stationary regime is obtained, in which

The second-order correction Ag (,w’) to the free particle mobility reads

Note that, in the static limit w - 0, the same result is

recovered either from equation (60) or from equation (37) with F --+ 0.

One can equally write the mobility tk ( w ) in the

form :

where Aq (w ) is complex and frequency-dependent.

Formula (60) shows that, at second order with respect to V, Aq (w ) is given by

The real part d 1] , (ClJ) of Aq (w ) modifies the friction coefficient q of the particle whereas the imaginary part Aq " (w ) may be interpreted as a

mass renormalization term. Before giving any ex-

plicit results for Aq’ (w ) and Aq "(w ), let us remark

that equations (62) and (37) involve integrals of the

same type,

w

playing the role of (27T/a)(F/1]).

Therefore, if we assume that

w

is much smaller than y, the results will be largely independent of the particular form of the cut-off function ; this will

allow us to use for computational facilities at zero or low temperatures kB T h-y an exponential cut-off

function.

Formula (61) states in particular that, in the

presence of the periodic potential (4), the particle

behaves like an equivalent free Brownian particle

with a modified (frequency-dependent) friction coeffi-

cient and a mass renormalization term (possibly frequency-dependent). On account of the fluctuation- dissipation theorem, this implies that the random

force (and thus the noise which is its spectral density)

is modified by the presence of the potential.

We shall examine this point more thoroughly in

the following paragraph.

4.2 NOISE IN THE PRESENCE OF THE PERIODIC POTENTIAL.

-

Generally speaking, the second fluc-

tuation-dissipation theorem states that, in a dissipa-

(12)

tive system, the friction coefficient q is linked to the

spectral density of the random force Fr(t) by

This is the case of the free Brownian particle [2]. As

demonstrated above, in the presence of the periodic potential, the friction coefficient q is modified by the

addition of â17’ (Cù ), which in turn implies that the

noise is modified by the addition of the quantity

We know [7, 14] that this quantity can equally be expressed in the equivalent form

in which one recognizes (by using the Wiener- Khintchine theorem) the spectral density of the

random force

This result however, could have been derived in a

completely different way, by looking at the stochastic equation of motion

similar to equation (5), but in which the particle

evolves under the sole action of the random force

F, (t) due to the coupling with the bath. At the lowest perturbation order, the force term due to the potential is a stochastic term equal to

where the quantity F,(t) + F’(t) now plays the role

of the random force. This scheme will be consistent with the preceding one if it can be shown that the spectral density of the quantity F,(t) + F’(t) is actually equal to the sum of expressions (63) and (64) ; in other words, the two random forces Fr(t) and F’(t) must be uncorrelated.

The expression to be analysed is the correlation function

The random force F,(t) is a linear combination of the bath creation and annihilation operators (see Eq. (7)) ; by using the following property of boson operators (where 0 and qi are any complex quantities)

which states that these average values are both

proportional to the average value of

one proves that expression (69) is proportional to

the average value of exp { i QOr (t )}, that is actually equal to zero (see Eq. (24)). Therefore the random

forces F,(t) and F’(t) are, as expected, uncor-

related. At second order with respect to the corruga- tion strength, the noise in the system is thus the sum of expressions (63) and (64) (or (65)).

4.3 RESULTS FOR Aq’(W ) AND Aq " ( w ). - In this paragraph we only give the analytic results for

å’T1 ’ (CJJ) and The physical implications of

these results on the transport coefficients, as well as

the validity of the calculation, will be discussed in

the following paragraphs. As in the static case, we

shall successively examine the low and high tempera-

ture situations.

4.3.1 Low temperatures (kB T hy). - We use in

this case the exponential cut-off function ; the func-

tions Al(t) and A2(t) are given by equations (40)

and (41).

(i) Zero-temperature limit

The real part Aq’(w ) of Aq (w ) is equal to

Exactly as in formula (43), the exponential factor is

very close to 1 and will be dropped out in the sequel.

The imaginary part Aq " (w ) of Aq (w ) is given by

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