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Electron-LO-Phonon Quantum Kinetics in quantum Dots

K. Král, Z. Khás

To cite this version:

K. Král, Z. Khás. Electron-LO-Phonon Quantum Kinetics in quantum Dots. Journal de Physique I,

EDP Sciences, 1997, 7 (11), pp.1431-1443. �10.1051/jp1:1997139�. �jpa-00247461�

(2)

Electron-LO-Phonon Quantum Kinetics in Quantum Dots

K. Kr61

(*)

and Z. Khfis

Institute of

Physics, Academy

of Sciences of Czech

Republic,

Na Slovance 2, 180 40

Prague

8, Czech

Republic

(Received

10 March 1997, revised 20

May 1997, accepted

15

July 1997)

PACS.72. Electronic transport in condensed matter PACS.73.40.-c Electronic transport in interface structures

PACS.72.10.-d

Theory

of electronic transport;

scattering

mechanisms

Abstract. Quantum kinetic equations are solved numerically for the process of the relax-

ation of an excited electronic system in a cubic quantum dot in a

GaAs/ALGaI-~As

structure with the

electron-LO-phonon

interaction included and with the carrier-carrier interaction ne-

glected.

The

theory

is

developed

within the equation of motion method for the reduced

density

matrices. It is shown that near the low electron and hole

density

limit a

relatively

broad inter- val of the dot lateral size may exist in which the relaxation of the electrons may develop at a

picosecond

time scale.

1. Introduction

Recently,

the

improvement

in the

technology

has led to a further reduction of the dimensional-

ity

of the seIniconductor structures

having,

besides the fundaInental

significance,

a

large iInpact

on the

expectation

of

applications

in

signal processing.

There is a

large

interest in understand-

ing

the

physical properties

of the heterostructures in which the electronic wave functions are

confined in three diInensions

(quantuIn dots).

These seIniconductor structures are

proInissing

due to the discrete electronic

density

of

states,

which makes their candidates for

high efficiency

lasers

ill.

The

perforInance

of the semiconductor lasers is

expected

to be

seriously

affected

by

the process of the relaxation of the excited electrons to the

ground

state, which is

supposed

to be critical in

quantum

dots

having

lateral dimensions less than 50 nm

[2-5j.

In

particular,

earlier theoretical estimates show that unless the

separation

of the electronic energy levels is close to the energy of the

Longitudinal Optical (LO) phonon

at the center of the Brillouin zone

(ltuJo),

the radiative

efficiency

of the

quantuIn

dot would be weak [3j at least in the

approxiInation

at which other interaction of electrons than the Fl0hlich

coupling

to the

polar optical phonons

are

neglected. Although

these conclusions appear to be

supported by

soIne

experiInents [6-8],

a luminescence was

reported [9-llj

in

samples,

in which the effect of the

phonon

bottleneck

on the luminescence should be noticeable.

Recently, photoluminescence

measurements have been

reported

in GaAs

quantum

dots hav-

ing

lateral dimension of about 450nm

[12j.

The

scattering

of electrons with the acoustic

(*)

Author for correspondence

(e-mail: kraltlfzu.cz)

@

Les

#ditions

de

Physique

1997

(3)

phonons

was found too slow to

explain

the small value of the relaxation time

(not larger

than

10ps)

observed.

Any strong

threshold behaviour in the

photoluIninescence spectra, expected

to occur on the basis of the reference

[3],

when the excitation energy scans

through

the

optical

phonon

energy

hula,

was

reported

to be absent in the

experimental

data.

The

high

value of the electronic

cooling rate,

obtained in the Born

approximation

[3] under the condition of the near-resonance between the electronic energy level

separation

and the

optical phonon

energy

hwo, brings

about a

question

about the role of the electron energy collision

broadening

in the effect under consideration. The electronic relaxation in quantum dots was studied

recently

in

coInprehensive

papers

[13,14].

The authors took into account the

electron-energy

collision

broadening

in a self-consistent Inanner and included into consideration the electron-hole electrostatic

coupling. They

find that in

dependence

on the

density

of

injected

carriers the electronic relaxation time can reach hundreds of

picoseconds

in a broad range of the dot size and carrier densities. This rather

rapid

electronic relaxation is found to be influenced in a fundamental manner

by

the

rapid

relaxation of the hole

subsystem having

rather

high density

of states.

The electronic relaxation channel due to the Fl0hlich

coupling

to the LO

phonons

is usu-

ally

the most intensive way of the energy relaxation in

polar

semiconductors and even in the

quantum

dots leads to an intensive relaxation

[3],

at least in the Born

approximation

to the

scattering rate, though

under some rather restrictive conditions

imposed

on the relation be-

tween the electronic

energy-level spacing

and the

optical phonon

energy. With the collision

broadening

included

[13,14]

it

might

offer a window of reasonable width in the electronic energy

scale,

or in the scale of the dot

size,

in which the electronic relaxation

might

be intensive under suitable circumstances. Besides the collision

broadening,

indicated

by

the Born

approximation

value of the relaxation rate, the

rapid

electronic relaxation may have some additional quantum effects. As such the

electron-LO-phonon

relaxation channel alone deserves a more detailed

attention.

The purpose of this work is to

analyze

the

electron-LO-phonon

relaxation channel in a

greater

detail

going beyond

the

approach

of papers

[13,14].

For this purpose the other energy relaxation channels are

neglected

here

together

with the

coupling

of electrons to the holes in the valence band states. A

simple

model of a cubic quantum dot with

only

two

lowest-energy

states is considered. In difference to the Monte Carlo

approach

of references

[13,14]

the present

theory

is

developed

in the frame of the

quantum transport equations [15,16] using

the reduced-

density

matrix formalism. This

approach

Inakes it

possible

to treat

siInultaneously

the effect of the electron energy collision

broadening

and the effect of coherent

exchange

of energy between the electron and

phonon subsysteIns.

In Section 2 the

quantuIn

kinetic

equations, giving

the

electronic relaxation in

quantuIn dot,

are forInulated within the second Born

approximation (see

Ref.

[17]), including

the self-consistent collision

broadening

contribution to the electron

energies.

The results of the nuInerical solution of the kinetic

equations,

for the case of a

quantuIn dot with

only

two electron energy

levels,

and a

single

electron in the

quantuIn dot,

are

presented

in Section 3.

2. Kinetic

Equations

2,I. HAMILTONIAN. A

siInple

case of the

quantuIn

dot will be

assuIned, naInely,

the GaAs

quantuIn

dot eInbedded in the

A[Gai-~As crystal,

in which the

single-electron

states are

represented by

their

energies

and wavefunctions. The Inodel electronic

potential

of the

quantuIn

dot and the

corresponding

electronic wavefunctions and

energies

will be

specified

in a later section. The effect of the holes in the valence band states and the electrostatic

coupling

aInong

electrons will be

neglected.

In this

respect

the model used

corresponds

to the liInit of low

(4)

density

of electrons and holes in the

saInple

with

quantuIn

dots. The

following

process will be considered here: at the tiIne t

= 0 the electronic

subsysteIn

is

prepared

at a state described

by

the

single-electron

distribution function. The electronic

systeIn

relaxes at t >

0, interacting only

with the

LO-phonons.

which are

kept

at

equilibriuIn

with the ambient lattice

throughout

the process. The effects connected with the finite duration of the

optical

excitation

pulse

and

the coherent

effects,

which may be induced

by

the effect of the

pulse

in the electron-hole

system

in the course of the excitation process

[15,16],

are thus

neglected

here.

The

unperturbed

electronic states, localized within the

dot,

form the orthonormal set

(in jr )

of orbital wave

functions,

with the

corresponding energies En. Neglecting

the effect of con- fined and interface

optical phonons,

the

system

of the

unperturbed

lattice vibrations will be

approximated by

the

LO-phonon

modes of bulk GaAs

crystal interacting

with the electrons via the Fl0hlich

coupling [18].

The electronic

screening

of this

coupling

will be

neglected.

The

Hamiltonian of the whole

system

then is:

H

=

£ Enc(~cn,~

+

£ ltuJqb(bq

+

£ £ £ Aq4l(n,

m,

q) (bq b+~) c(~cm,~, (l)

n,«

'

q m,n q «

'

where the three terms on the rhs of

(I)

are,

respectively,

the Hamiltonian of free

electrons,

the Hamiltonian of free LO

phonons

with the energy

ltuJq

and the Fr6hlich

coupling.

In

(I)

cn,~

and

bq

are,

respectively,

the annihilation

operators

of the electron in the n-th orbital

state,

with

spin

a, and the annihilation operator of the

LO-phonon

with the momentum q. The

quantity 4l(n,

m,

q)

is the forIn-factor of the

quantuIn dot,

defined as

4l(n,

m,

q)

=

d~r ~fi((r)e~~~~fim(r), (2)

having

the

property

4~~ln,

m,

qj

"

~jm,n, -qj. j3)

The

coupling

constant

Aq [18]

is

ie

~i ~-i

~q

"

~j 2eoV

~~° ° '

(4)

where q

=

)q),

-e is electronic

charge,

so is

perInittivity

of free space and ~c~ and ~co are

high frequency

and static dielectric constants, ltuJo is the

LO-phonon

energy at the r

point

of the

Brillouin zone. V is the voluIne of the

saInple.

2.2.

QUANTUM-KINETIC EQUATIONS.

The effect of the

nonequilibrium

of the

phonon

sys-

te1n will be

neglected

here.

Thus,

the basic

quantity.

for which the quantuIn kinetic

equations

will be

forInulated,

will be the

density fn,~

of electrons in the state

in, a),

defined as

fn,~

~

(c$ ~cn,~)

~

Ti(c( ~cn,~p), (5)

p

being

the statistical

operator

of the whole

systeIn, Trip)

= I.

Starting

with the

Heisenberg equation

for the tiIne evolution of the operator

c(~cn,~

and

using

the

property (3)

of the forIn

factor,

one finds '

j

=

-) L L lAqlRel4lln>1> q)llbq b±q)Ct,«Ci,«11.

16) At the

right

hand side of this

equation

the Inean values are found of the

product

of one

phonon-

and two

electron-particle

operators. This

equation

is a

beginning

of an infinite series

(5)

of

equations.

As

usual,

the latter set of

equations

can be solved

approxiInately by factorizing

the mean values at the

right

hand sides in such a way that a closed set of

equations

for a restricted set of reduced

density

matrices is obtained. In the lowest

order,

a factorization of the

phonon-assisted

matrices

present

at the rhs of

equation (6)

can be

performed, resulting

in the

product

of the mean value

(bq)

and the mean value

(c(~ci,«). Assuming

the

diagonal approximation, namely, (cl ~ci,«)

~

6n,1(c$,~cn,~),

the

right (and

side of

equation (6) gives

zero. In this

approximatiin,

the nonzero value of the rhs of

equation (6)

would thus be

connected with the presence of coherent

phonons ((bq))

and

by

the

mixing

of the states n

and due to the

electron-LO-phonon coupling,

manifested

by

nonzero

quantities (c(~ci,«)

with n

~

l. We shall

neglect

these effects and

proceed

further to consider the

higher'order

equations.

The

coInplete equation

for the

phonon-assisted density

Inatrix

(bqc( ~cn,~)

reads:

~~~~~'"~~'"~ lt

~~ ~"

~ ~~°~~

~~~~~>""'"~

)lA~l4~li>'~>

~q) lfn,~(i fl,~)

+

"qlfn,~ fl,~)l

+) L lAql4~ln',m',-q)61C$,«Ci,«C$,,«,Cm,,«<I

w,~,,~,

+) £ lA~'l4~li'~"q')61b~q'b~~$,~°°'>"l

m',q'

£ jAq, j4l(n',

n,

q')6(b+~, bqc$,

ci

al

11

~, ~,

'" '

~

£ jAq, 4l(1, m', q') (bq, bqc$

~cm,

~)

h

, ,

' '

m ,q

+

~j )Aq, )4l(n',

n,

q') (bq, bqci

~

ci

al (7)

11

~, ~,

"

' '

The second terIn on rhs of this

equation

was obtained

by factorizing two-particle density

Inatrices into

products

of electronic and

phonon

distribution functions

fn,~

and uq =

(b(bq) (coInpare

with the

analogical

derivation in bulk

Inaterials,

Ref.

[16]).

The

neglection

of the

last five terIns in

(7)

would represent the second Born

(28) approxiInation [17]

to the quantuIn

kinetic

equation

for

fn,~.

It is well known [17] that 28

approxiInation

is

unstable, giving solutions,

in which the electronic distribution function leaves the interval

(0,1)

in the course of the time evolution. The inclusion of the last five terms allows one to Inake the

present

level of

approxiInation

consistent. The three terIns

containing

the

syInbol ii...)

are the

two-particle

correlation functions defined as the difference between the

two-particle density

Inatrix and the factorized forIn of the latter. For

instance,

61b+q,bqc$,,«Ci,«I

=

16+~,bqc(,,~ci,«1- 6-q,,q61,n,uqfi,« 18)

and

61C$,«Ci,«c$~,«~Cm~,«~) =

ic$,«ci,«c$~,«,cm~.«,) 6n,m~61,n~6«,«~fn,«li fi,«).

19)

The last two terIns in

equation (7)

contain the reduced

density

Inatrices which

give

zero con-

tribution in the factorized form.

They

do not contribute to the second term on rhs of

equation

(7).

This is due to the zero values attributed to the terms

(bqbq,).

(6)

It is well known that the above mentioned

instability

of 28

approximation

can be removed upon

introducing iInaginary coInponents

to the electronic

energies

in the

equation (7),

or the collision

broadening

of the

single-electron

energy levels

[16].

The Train

steps

of the derivation

are

following.

The

equations

of1notion can be written down for the five

two-particle

correlation functions of

equation (7).

These

equations

express the tiIne derivatives of the

two-particle

correlation functions in terms of mean values of

products

of five

particle operators.

The latter

five-particle

operator mean values can be factorized to the

products

of the

phonon-assisted density

matrix

(bqc$ ~ci,«)

and

single-particle

distribution functions. The

equations

for the five

correlation

functioni present

in

equation (7)

can be solved under the adiabatic and Markov

approximation [15].

The details of the derivation are

given

in the

appendix. Substituting

the result into

(7),

the

equation

for the

phonon-assisted density

matrix

(bqc$~ci,«),

with the

energy

broadening

of the electronic

energies included,

reads: '

~~~~~>""'"~ h l~ ~" ~

~~~'"

~

~"'"~

~

~~~

~~~~~>""'"~

+) lAq jail'll'~q)lfn,~li fl,~)

+

"q(fn,~ fl,~)l' lio)

In this

equation

the

damping

factor

r~,~

was determined in the second order

approximation

to the

electron-phonon coupling

and in adiabatic and Markov

approximation (see appendix).

It

reads

r~>"

~

)LlAql~l@(~>3,qll~

q>3

~

llf3>"

+

"~q)61E~ E3

+

h~-q)

+

l~

+ "q

f3.")61Ei EJ h~q)I' l~~)

The

singularity

ofthe

density

of states ofthe

quantum

dot leads to the

necessity

to calculate the

damping rate,

or the collision

broadening,in

a self-consistent manner

[13,14].

For this purpose, the formula

ill)

can be

generalized by substituting

the Lorentzian function with a finite width

instead of the

energy-conserving

delta function. Let us note that in references

[13,14]

the

energy-conserving

delta function is substituted

by

a Gaussian line. In the case of the

presently

used Lorentzian function one obtains self-consistent

equations

for the

damping

rate which can be shown to

correspond

to a self-consistent Tamm-Dancoff

[19] approximation

to the electronic

self-energy represented by

the

imaginary

part of the

latter,

taken in the

pole approximation.

Other differences between the Gaussian and Lorentzian version of the substitution of the delta function are not considered here. It is obtained that

C~

=

~~£jAqj~j4l(I,j,q)j~

' lt

q,J

x

j /~,~

+

v-~) ' ~~>"~~ )j"~

7r

(E~ Ej

+

ltuJ-q)

+

~(r~,~

+

rj,~)

~

+(l

+ uq

fj,~)

~

~~~'"

~

~l'"~ j. (12)

~r

lE~ Ej

hU~q)~ + m

lrz,«

+

rj,«)~

The latter forInula allows one to calculate

self-consistently

the

damping

rates

r~,~

for all

I,

solving iteratively

the set of

equations (12),

at a

given

state of the

system

of the

quantum well,

given by

the

single-particle

distribution functions.

(7)

The

equations (6, 10, 12)

form

together

a closed set of

equations

for the

quantum-kinetic

determination of the time

development

of the electronic distribution

function,

the

phonon-

assisted distribution functions and the self-consistent collision

broadening

of electronic

energies, ltr~,~,

or the

damping

factor

r~,~.

This set of

equations

will be solved

numerically

in Section 3.

2.3. SEMICLASSICAL APPROXIMATION. As it is well known

[16],

the semiclassical

approxi-

mation can be obtained

by solving formally

the

equation (10)

with

applying

the adiabatic and Markov

approximation.

In the

present

case these

steps

lead to the Boltzmann

equation

for

In,~

with the collision

broadening:

~

l'~

"

-'f($~~fn,« +'i($~ Ii fn,«), (13)

where

~/1[l~~ =

LLLlAql~l4~ln,1,qjj~

+>- q I#n

rn,~

+

Ti,«

(I fi,«) "+q

~ ~

~

~~~~

x

~~ ~~

~ /~~~~~j2 +

((rn,«

+

Fi,«)~

and

~li',f

=

LLLlAql~l4~ln,1,q)l~

+>~ q I#n

~

(Ei En

+

lt~j$~~)(rn,~

+

ri~«)~ ~'~ ~~~

~ ~ ~~~~

As it was shown earlier

[17]

for the case of the

quantum-kinetic equations

in the bulk electron-

phonon system,

the sum ~y($~~ +

~y(# gives

the

daInping

factor of the energy level

En,

'fn,a ~'fn,a

~

~n,a. (16)

The latter forInula is

easily

verified for the

present

case

too, coInparing

the

equations (14, 15)

with the forInula

(12).

The

equations (13-16) provide

the relation between the collision broad-

ening

and the relaxation rate

given by

the Boltzlnann

equation. Taking

the liInits of

Tn,~

and

ri,« going

to zero at the

right

hand side of

equations (14, 15),

the Boltzlnann

equation (13)

is obtained with the collision

integral

taken into account in Born

approxiInation,

as it was used in the reference

[3],

when

estiInating

the

efficiency

of the

electron-LO-phonon scattering

channel in the lowest order.

In the

special

case of

fn,~

=

l,

with all the other states

eInpty,

y~,$~ is zero. The

daInping

factor

rn,~, given by

the

equation (16),

then

gives

the initial

It

=

0)

relaxation rate,

naInely, rn,~

=

id fn,~ /dtj.

The

equation (13)

can be used in seIniclassical calculations of the electronic

relaxation in

quantuIn

dots with electron energy collision

broadening

included.

3. Numerical Evaluations

For the purpose

of1nini1nizing

the

coInputer

deInands several

approximations

are Trade. The

quantuIn

dot is

supposed

to have the

shape

of a cube with the GaAs material inside. The electronic

potential

is

supposed

to be infinite outside the dot.

Therefore,

the

energies

of an electron are

~2fi2

~n

"

l~nin2n3 @

~~~ ~

7l(

~ 7l(~

(~~)

(8)

while the

corresponding

orbital wave functions are:

~bn>n~n~

ir) 11)

~/~

sin

i~i~ (xi iii

sin

i~i~

x~ i)i

sin

i~i~

x~ iii

,

i18)

where r

=

(xi,

x2,

x3)

is the electron coordinate and m is the effective mass. The indices n~, I =

1, 2, 3,.

, are

positive integers.

The

composed

index

(ni,

n2,

n3)

now

plays

the role of the index n in the

equation (I). Eiii

is the electron

ground

state energy. The first electronic

excited state is

degenerate, E211

"

E121

"

Ei12.

The kinetic

equations

will be solved

taking

into the consideration

only

two orbital

states,

(I, I, I)

and

(2,1,1),

out of the whole space of

possible

orbital states of an electron in the

dot, assuIning

that this restriction does not cause any serious error in the Train conclusions of this work. We assuIne that there is a

single

electron with

spin

a in the dot. At the initial

tiIne oft

= 0 the

population f211«

of the orbital state

(2,1,1),

with the

spin

a, is assuIned to be

I,

while the electronic

population

in the lowest energy orbital state

(I, I, I)

with

spin

a,

fill«,

is taken to be zero. At t > 0 the electrons are

being

transferred to the

ground

state

by

the relaxation process. The

optical-phonon systeIn

is assumed to be

constantly

at

equilibrium

at the temperature of the ambient

lattice, TL

"

10K, ignoring

in this way the

effect of hot

phonons.

The distribution function uq is

given by

the Bose-Einstein distribution function.

Consistently

with the

assumption

of

TL"

10K of the ambient

lattice,

the processes of the transfer of the electron from the

ground

state to the orbital states

(1, 2,1)

and

(I,1, 2),

in the process of

absorption

of an

optical phonon,

will be

ignored.

Therefore we assuIne

f211«

+

fill«

" I in the course of the relaxation. In the

following

we

keep

the index a in

fn~n~n~~,

to

keep

record of the

fact,

that

fn~n~n~~

e

(0,1).

The

dispersion hwq

of the LO

phonon

is assuIned

isotropic, given by

the forInula

h~°q

"

Fo

+ AF cos

l~~

~B '

(~~)

approxiInating

the Brillouin zone

by

the

sphere

in the q-space, with the radius

qB " 1.09 x

10~°1n-~

We take

Fo

" 5.219 x

10~~~

J and AF

= 5.79 x

lo-~~ J,

to

approximate

the well-known

dispersion dependence

of the

LO-phonons [20].

The Inaterial

paraIneters

of

GaAs are taken over froIn reference

[21].

The

probleIn

under consideration

requires

that the

daInping

factors

r~,~

be deterInined froIn the self-consistent

equations (12),

rather than froIn the first-order

expression (11).

The

iInpor-

tance of the

higher

orders of the

perturbation expansion

of

r~,~

in powers of the electron-LO-

phonon coupling,

can be

clearly

seen in the process of the iterative solution of the self-consistent

equations (12). Therefore,

the nuInerical results

presented

in this paper are

coInputed

with the self-consistent solution for the

daInping

factor

r~,~

included.

The seIniclassical relaxation rate d

f211«/dt, given by

the

equation (13), coInputed

at the initial instant of the

tiIne,

t =

0,

is

presented

in the

Figure

I. This rate is

displayed

as a

function of the lateral size d. The Inaximuln of the rate is found at about d

= 21.7nm. At

this distance the electronic

energy-level separation E211 El

ii

equals

the zone-center value of the

LO-phonon

energy

hwo.

The value of the relaxation rate is of the order of 10~~

s~~

in the

range of d from about 20nm to about 23nm. This range of d

corresponds approxiInately

to the energy range froIn 32 to 411neV of the

energy-level separation E211 El

ii

(see Fig. I).

Let

us reInark at this

point,

that the

scattering

rate calculation

[13,14],

based on a self-consistent determination of the

electron-energy

collision

broadening

and the electron-hole

scattering

gave the relaxation times of the order of hundreds of

picoseconds

in a broad range of the dot

size,

(9)

_

0

v~

~

41 mev 36 mev 32 mev

~ Q~

li

~ 5

_8

li

~

Q~

0C

§0

21 22 23

Lateral size

(nm)

Fig,

I. Relaxation rate

-df211«/dt,

as a function of the lateral size d, computed from the semi-

classical equation

(13),

at the state with f211«

= 1 and

fill«

= 0, with the

damping

factor determined from the self-consistent equation. The lattice temperature TL is lo K. The values of the

energy-level

separation E211

Eiii, corresponding

to three selected values of the lateral size

(given by

the

arrows),

are presented in the

graph.

which differs from the

present

result. This difference is ascribed to the

neglection

of the electron-hole

coupling [13,14]

in the

present

model of the dot. The

shape

of the relaxation rate d

f211«/dt (Fig. 1),

which extends over a rather wide range of

d,

is in a

partial agreement

with the

experimental

observation on the

photoluminescence

in

quantum

dots

[12]. Namely,

in reference

[12]

an absence is

reported

of any threshold behaviour of the

photoluIninescence

response, when the energy of the

exciting photon

scans

through

the

optical phonon

energy

ltwo.

Such a threshold behaviour can be

expected

on the

grounds

of the earlier theoretical

estiInates

[3],

which gave a very

sharp dependence

of the electronic relaxation rate on the electron energy level

separation.

It has to be realized

however,that

a

coInparison

ofthe

present

result with the

experiIneni [12]

should be Trade with care, because in the

experiInent

[12] the nuInber of electrons per

single

dot Tray be

larger

than I and the processes of the

exchange

of energy between electron and

holes1nay play

a role as

pointed

out in

[13,14].

The present result should rather be

coInpared

with data

corresponding

to the low electronic and hole

density

liInit.

The

quantuIn

kinetic

equations (6, 10),

with the

equation (12)

for

r~,~,

were solved

by Runge-Kuttalnethod

of the nuInerical solution of a set of differential

equations.

The tiIne

step

was 0.25fs. This way of

solving

the

equations

was rather

deInanding

on Inelnory and CPU time. The nuInerical solution of the quantum kinetic

equations

is

presented

in

Figure

2. In this

figure,

the electronic

population f21la

is

displayed

as a function of tiIne t and the

quantuIn

dot lateral size d. In the interval of the lateral size d froIn about 20 nIn to about 23 nm the electronic

population

decreases

monotonously

with time. This range of d agrees with the range, inside which the semiclassical relaxation rate d

f211«/dt,

of

Figure I,

is nonzero. In this semiclassical

region

of d in

Figure 2,

the characteristic time of the relaxation

corresponds

to the semiclassical values of the relaxation rate of

Figure

I. Let us

note,

that at the very small

times,

under about 30

fs,

the relaxation rate in the semiclassical range of d is rather

weak,

which can be

regarded

as a manifestation of the

energy-nonconservation

effect due to the time

inhomogeneity

at t = 0 in the

presently

considered

"thought" experiment,

in which the

system

is excited at t = 0

by

an excitation

pulse

with the

infinitely

short duration. The solution of the

quantum

kinetic

equations

can be

expected

to agree in the semiclassical

region

with the numerical results based

(10)

8~

~

l~

I

~

t

Fig.

2. Time evolution of the

population

f211«, as a function of the lateral size d and time t,

in the cubic quantum dot with two energy levels taken into account,

computed

from the quantum kinetic equations. TL

= 10K. The oscillations of the

population

at

large

and small d demonstrate the reversible transfer of energy between the electronic and

phonon

subsystems.

.oo

c

o a

= m

~ o.95

if

f

~ m

d =19 nm

o.90~

~~~ loco

Time

Ifs)

Fig.

3. Time evolution of the

population f211«,

for the selected value of the quantum dot lateral size d. The numerical data show that the

population oscillates,

due to the reversible transfer of energy between electrons and phonons, between the lower limit

fm (dotted line)

and I. The

averaged

value of the population is

fa (dashed line).

on the semiclassical formula

(13).

In the semiclassical range of the lattice size the solution

presented

in

Figure

2

supports

the above

given interpretation

of the absence of a threshold in the

photoluminescence experimental

data

[12].

It has to be noted

again,

the numerical results

should be better

compared

with

experiments performed

near the low carrier

density

limit.

In the range of d above about 23nm and below about 20nm in

Figure 2,

the electronic

population

is not constant and

equal

to

I,

as it would be

expected

on the

grounds

of the semiclassical

approach,

but it oscillates with time between I and

fm, fm being

a number between zero and one. This time

dependence

of

f211«

is

displayed

in1nore detail in

Figure

3 for a selected value of d. F1o1n

Figure

2 it is observed that the

Inagnitude

of

fm increases,

approaching

the value of I, when either d increases above about

23nm,

or d decreases below

(11)

about 20 nm.

Similarly,

the

frequency

of the oscillations increases with

increasing

the

separation

of d from the semiclassical range of d values. In other

words,

the

frequency

of the oscillation of

f211« along

the time axis increases with the difference between the electronic

energy-level

separation E211 Eiii

and the energy of the LO

phonons.

Let us denote the

region

of d

values,

which are outside the semiclassical

region,

as the

quantum region

of d. The

inspection

of the numerical data

shows,

that the electronic

population, averaged

in time over one

period

of the

oscillation,

is about

la

=

(I

+

fm)/2,

with

fm depending

on d in the way

given

above. It is essential to see,

that,

the electronic

population, averaged

over one

period,

is lower than I in the

quantum region.

The more the lateral size d

approaches

the semiclassical range of the dot

size,

the

stronger

the decrease of the average

population

is. The numerical calculation shows that in the

vicinity

of the lateral size of about 20nm or about 23nm a transition

region

appears

to occur, in which the collision

broadening

is still nonzero, but small

enough

for the reversible oscillations to

prevail.

The oscillations deInonstrate the

exchange

of energy between the electronic and vibrational

subsysteIns.

This

exchange

is reversible and is an

iInplication

of the

fact,

that the states of the whole

systeIn,

at which the electronic

subsystem

is in the excited

state,

are not

eigenstates

of the whole

systeIn. Relying fully

on the

plausibility

of the

approxiInation

to the

quantuIn

kinetic

equations, accepted

in this

work,

one should

expect

the oscillations of the electronic

population

to be

observable, providing

the initial state of the

electron-phonon systeIn

of the dot is realized.

It should be

expected,

that the behaviour of

f211«,

deInonstrated in the

quantuIn region

of

d,

is influenced

by

the

quantuIn

effect of the energy nonconservation due to the time in-

homogeneity,

in the scenario considered. In a real

experiment,

the manifestation of the time

inhomogeneity

would be

different,

in

dependence

on the process of excitation of the electronic

systeIn. Nevertheless,

in the case of

exciting

the electronic

systeIn

in

quantuIn

dots with

help

of a femtosecond laser

pulse,

the conditions of the

experiment

would be close to the scenario under consideration.

The effect of the decrease of the electronic

population f211«

in the

quantuIn region

at short

tiInes,

as it contributes to the overall status of the

systeIn resulting

froIn the decrease of the electronic

population

in the whole range of

d,

is therefore

coInplelnentary

to the seIniclassi- cal relaxation of

Figure

I. In contrast to the Born

approxiInation

result of reference

[3],

the

d-dependence

of the electronic relaxation is then

relatively

broad,

including,

besides the semi- classical

region,

the

quantum region

as well. The electronic relaxation of

Figure

2 thus does not contain any

strong

threshold feature to be observed in

photoluIninescence experiInents.

With

taking

into consideration the quantuIn

region

of the decrease of

f211«,

the range of

d,

at which a finite aInount of the electronic

population

is relaxed at a

given

instant of

tiIne,

is therefore broader than it results froIn the seIniclassical

approach only.

In the

quantum region

of d, the average of the

population fill«

of the electronic

ground

state has thus a nonzero

value at t > 0. This fact should have an

iInpact

on the processes, not included in the

present

paper, like the luminescence connected with transitions froIn the electronic

ground

state to the valence band states.

The results

presented

are based on the

analysis

of the dot with two electron energy levels

only. Quantitatively,

these results can be Inodified to an extent when

considering

not

only

an

exciting optical pulse

of a finite

width,

but also

quantum

dots with a

large

nuInber of electron energy levels and many electrons.

As it has been mentioned

already

in the Section

2.2,

the numerical solution of the quan- tum kinetic

equations,

similar to those considered

above,

can

display

an

unphysical

property of

f~ii~ leaving

the interval

(0,1),

in the case, when the

damping

factors

r~,~

are

approxi-

mated

by

zero. This effect was

analyzed recently

in a

quantum

dot

system [17].

It was found

(12)

that the effect is the

property

of the

approxiInation,

rather than a nuInerical

inaccuracy.

It has been

shown,

that the

unphysical

behaviour of the electronic distribution function can be

reInoved,

if the

electron-energy

collision

broadening

is introduced

[16].

As

expected,

the nu- 1nerical solution for

f211«,

of the

quantuIn

kinetic

equations (6, 10),

with

(12),

in both the

seIniclassical and

quantuIn regions,

is found within the interval

(0, 1).

Let us reInark that the nuInerical results are

coInputed

for the

quantuIn

dot with

infinitely deep potential

well.

Taking

into account a Inore realistic

shape

of the

confining potential

Tray

influence the

quantitative

results to an extent.

4.

Summary

The hot electron relaxation was studied in

polar

semiconductor

quantum

dots in the approx- imation of two electronic energy levels

coupled by

the interaction of electrons with

only

LO

phonons.

The relaxation was studied within the method of

equations

of motion for the reduced

density matrices, applying

the

approximations

used

recently

in studies of the femtosecond

phe-

nomena in bulk materials. The

emphasis

was

put

on

quantitative

estimates of the effects

given

by

the semiclassical and

quantum

kinetic

equations.

The solution of the

quantum

kinetic

equations displays

two main

regions

of the quantum dot size

(or

electronic

energy) according

to the behaviour of the electronic relaxation. In the interval

from about 20nm to about 23 nm of the lateral size of the cubic dot the electronic relaxation time is found at the

picosecond

time scale and the electronic

population

decreases

monotonously

as it would be

expected

when

using

the irreversible semiclassical

approximation

to the process of relaxation with the electron energy collision

broadening

included. In the

quantum region

of the lateral size above about 23nm and below about 20nm the relaxation process appears to be reversible in the

present model,

with the excited-state electronic

population oscillating

around an average value of the

population.

The electronic

population

starts to oscillate around this average value at

early

times which appear to be not

larger

than the relaxation time in the semiclassical

region.

The numerical results appear to indicate the presence of narrow

transition

regions

between the two main

regions,

in which the

damping

factors are nonzero but small

enough

to lead to a non-monotonous decrease of the electronic

population.

Both the

quantum

and the transition

regions might

contribute to the relaxation from the excited

electronic level in cases when the electron has a finite lifetime in the

ground

state.

Although

the range of the electron

energy-level separation,

at which the relaxation is irre- versible and is at the

picosecond

time

scale,

is

only

about a

one-quarter

of the

optical phonon

energy, it

corresponds

to a rather broad interval of the lateral dot size. The width of this dot size interval may be

interesting

from the

point

of view of the current

technology

of

quantum

dots.

According

to the

present results,

the values of the electronic energy level

separations,

at which the electronic relaxation is very

fast,

are not restricted to a very narrow

vicinity

of

the zone center LO

phonon

energy, as indicated

by

the Born

approximation. Providing

that

quantum

dots

having

the size of tens of nanometers are

prepared

with the

energy-level

sep-

aration

being

within the energy window

given

in

Figure I,

the relaxation time of the

polar

semiconductor

quantum

dot laser structures can be at the

picosecond

time scale even at low

injection

levels of electronic

density.

Appendix

Let us write down the

equation

for the correlation function

6(b+~,bqc(, ~ci,«)

of

equation

ii)

and

demonstrate,

on this

example,

the

approximations applied. Using'the

definition

(8),

(13)

we obtain in a

straightforward

way

j6(b+~,bqc(,

~ci

al

"

(Ei

+

ltuJq En, ltuJ-q,)(b+~,bqc(,

~ci

al IA. I)

t ' i '

+

£ )Aq, j4l(ni,

ml,

-q') (bqc+,

ci

«c(

~ cm~ ~~

~

ni,mi,t

" '~ ~' ~ ~

i

~i

q(~ '~~" '~~~'~~'~"~l~~"~~q~~~CS~,«Cmi,«i

+

L iAq,, i#ml, n~,

q~~i

ibq,, b+~, bqcsi,«ci,«1

~,,,~,

+) L lAql4~lni,mi,-qllb+q,C$,,«Ci,«c$i,«icmi,«il

ni,mi,«i

+

L lAq,, la fl,

mi,

q"I16+q, b+q,, bqc$,,«Cmi,«I

q",mi

L lAq" la Ini, n', q")16+q, b+q,, bqc$i,«Ci,«1

~,,,~~

+

)6-q,,q61,n,v~ L L iAq,, iReiaii,

r,

q~~)iibq,, b+~,, )c[~cr«i I

q,, r#1

The reduced

density

matrices on the rhs of this

equation, containing

five

particle operators each,

can be factorized to the

products

of two mean

values,

one of which is of the

type (bqcf~cj,~

and the other is a

single-particle

distribution function. After

doing

the

factorization, seieral

terms

on the rhs of

equation (20)

are

found,

which have the form of a sum over

q",

of terms

containing expressions

like

(bq,,cf~cj,~).

These terms are eliminated on the

grounds

of the Random-

Phase-Approximation irgument (RPA) (compare

Ref.

[16]). Namely,

the latter mean values

are

regarded

as

changing rapidly

in

phase

in the Brillouin zone, over which the summation extends.

Solne of the

terIns,

which still reInain in

(20)

after the RPA reduction of this

equation,

are

found to be

proportional

to the

quantity (bqc$,~ci,«) only

upon

assuIning

that n'

= n in the

correlation function

(b+~,bqc(, ~ci,«).

Such terms contribute

only

to the term with n'

= n in

the sum over n' in the fifth

term

on the rhs of

equation iii. Realizing

that

according

to the

equation (6)

the electronic states with the orbital indexes n and I are

coupled

via emission or

absorption

of the

phonon,

the terms like

6(b+~,bqc$~ci,«)

are not

expected

to contribute on the basis of the energy conservation

argument

and

tiey

are therefore

neglected.

In the

approximation specified above,

it is obtained that

~~~~~q'~~~$,al>") j ~~

~

~~q ~'l' ~~-q') ~~~q'~qc~',a~l>")

+) lAq'l@l~>11'> ~q'll~

+ "-q'

fn',al lbq~t,a~l,al. jA.21

Let the letter t denote the time

dependence

of the

phonon-assisted density matrices, writing

(bqc$~ci,«)t.

In the zero-order

approximation (in Aq)

(bqc$,~ci,«)t-t~

=

(bqc$,«Cl>«)t ~~P~)~~~'~' ~~

~~

(14)

where

ER

"

Ei En

+

ltuJq. Taking

this

rapid part

of the

time-dependence

into account, the

equation (21)

can be

integrated formally. Applying

the adiabatic and Markov

approximation

[15] to the formal solution of

equation (21),

one obtains

6(b+~,bqc(,

~ci

al

"

ijAq, j4l(n, n', -q')(I

+ u-q,

fn, ~)(bqc(~ci al

,

(A.4)

' ' '

ER

ltuJ + is

where e

=

0+

and ltuJ =

Ei

+

ltuJq En, ltuJ-q,.

This

equation provides

the

self-energy

contribution to

equation iii.

In this paper the real part of the

self-energy, giving

the

polaron

shifts of the electronic

energies,

will be

neglected.

Analogically

the other correlation functions in

equation iii

are treated.

References

ill Cingolani

R. and Rinaldi

R.,

Rivista del Ntlovo Cimento 16

(1993)

1.

[2]

Benisty H., Sotomayor-TorrAs

C. M. and Weisbuch

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10945.

[3] Inoshita T. and Sakaki

H., Phys.

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Wang P., Sotomayor-Torrbs C., Benisty H.,

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Sotomayor-TorrAs C.,

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W.,

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G.,

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Lam Y. and

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Kuhn T, and Rossi

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Zimmermann R, and Wauer

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The galaxy bias model described above was used to correct the observed galaxy overdensity field, enabling measurement of the shape and amplitude of the power spectrum of L ∗

(c) Raman wavenumbers of the 1-LO peak as a function of the laser power for the 5.5-nm PbSe nanocrystal film and a bulk PbSe sample.. (d) Raman wavenumbers of the 1-LO phonon mode as

intermediate states. Quite generally in the large class of two-dimensional systems investigated in this and our previous [4, 11] articles the disorder induced

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