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Hole Transport Charateristis in Pure and Doped GaSb

L.G.O. Messias and E.Marega Jr.

Departamentode Fsiae Ci^eniadosMateriais,

IFSC/USP,CaixaPostal369,13560-970, S~aoCarlos,SP,Brazil

Reeivedon23April,2001

ThesteadystateholetransportpropertiesofGaSbwereinvestigatedbytheEnsembleMonteCarlo

method(EMC). Inourmodelwetakenintoaountheavyandlightholevalenebands,and the

followingsatteringmehanisms: inelastiaoustiphonon;polaroptialphonon;nonpolaroptial;

ionizedimpurity.Thetheoretialalulationsareomparedwithavailableexperimentalresultsfor

theGaSbholemobilityshowngoodagreementwithtemperaturesfrom90K upto300K.

I Introdution

Amongthe III-V binarysemiondutors, Gallium

An-timonide (GaSb) has attrated onsiderable attention

over the last several years. Many of its interesting

properties are diretlyassoiated withits verylow

ef-fetive eletron mass and high mobilities[1℄.

Conse-quently,itisanimportantandidateinhighspeed

ap-pliations in transistors and other devies. The

rela-tivelylowbandgapofGaSblendsitselfwelltomid/far

rangeIRdetetorsandsoures. Fromthedeviepoint

of view, GaSbbased strutures haveshown

potential-ityfor appliations in laser diodes with lowthreshold

[2℄, photodetetors[5℄, superlatties with tailored

opti-alandtransportharateristis[6℄, heterojuntions[3℄

andresonanttunneling devies[4℄.

UndopedGaSbisalwaysp-type,ausedbythe

pres-eneofanunusuallylargenativeaeptorbakground.

Duttaet. al.[1 ℄haveshownthat theondutivityarise

from adoubly ionizable nativedefet. At higher

tem-peratures the mobility depends basially on the

on-entrationofnativedefets,whiharerelatedwiththe

growthonditions. Inthisregime,signiant

ontribu-tionsfromaousti,non-polaroptial,andpolaroptial

phononsatteringareobserved,inagreementwiththe

Monte Carlosimulation. Thelargenegativeresistane

in n-GaSb are drastially aeted by the inrease of

the density of defets, indiated by the dereasing of

thearriersmobility.

Fromthetheoretialpointofview,afewworkwere

reported in theliterature relatedto p-GaSb transport

properties. Inareentwork[7℄,theresultsobtainedfor

theholemobilityareindisagreementwiththeavailable

experimental results[1℄. The ionized impurity

meha-nism was notinluded in the alulationsand it may

p-GaSb.

In this work we investigate the steady state hole

transport properties using Ensemble Monte Carlo

method (EMC) in p-GaSb. The transport properties

suhas: holedriftveloity,averageenergyand

mobil-ity were studied and ompared with available

experi-mental results. OurresultsfortheGaSbholemobility

showngoodagreementwithtemperaturesfrom90Kup

to300K.

II The model

The Ensemble Monte Carlo method is desribed

else-where [8℄, so we fous our attention in the prinipal

featuresofourmodel. Intheaseoftheholetransport

the analyti band struture is alulated from Warp

model [8℄. The nonparaboli valene bands were

in-luded and the warping parameters A, B, and C are

xedonstantforGaSb. Indespite,theotherswarping

onstantsvaluesanbefoundintheliterature. Nintuze

ando-workers[11℄studiedtheinueneofthese

param-eters, on theholetransport properties. Theveloities

obtained,usingthreesetsofparametersagreewith

ex-perimentin therangeof 12%-15%. Forlow elds, the

agreementarelosertotheexperiment.

The sattering mehanisms inluded in our

model are: inelasti aoustial phonon (deformation

potential)[12℄; polar optial phonon[10℄; nonpolar

op-tial proess[13℄; ionized impurity (Cowell-Weiskopft

model)[14℄. Foraoustiinterations,wehoosethe

in-elastimodelbeausetheequipartition approximation

k

b

T >> ~!

a

isn't more valid for low temperatures.

Also, we inludedin ourmodel the interband

(2)

Theparametersused inouralulationsareshown

in table1.

Table1

Parameters Values

heavyholeeetivemass(300K) 0.22

lightholeeetivemass 0.05

jAj 11.80

jBj 8.06

jCj 11.71

AoustiDeformationPotential(eV) 3.0

OptialDeformationPotential(eV/m) 0.6x10 9

Density(g/m 3

) 5.613

phononenergy(meV) 32.90

optialphononenergy(meV) 32.90

Relativepermittivity(high) 14.44

Relativepermittivity(stati) 15.69

Inall alulationswetook in onsiderationthe

ef-fetof thetemperatureonthe gapand eetivemass.

The eet of the temperature was not onsidered for

thewarpingparameters.

III Results

In Fig. 1 we ompare the experimental results[1℄ for

theholemobilitytemperaturedependene withthe

re-sultsobtainedbytheEMC.Ourresultstverywellthe

experimentalresultsdownto90K.Thedisrepanyfor

lowtemperatureouldbeexplainedduetodependene

of thevalene band parameterswith thetemperature,

notinluded in ourmodel due totheabsene of

theo-retialandexperimentaldatareportedintheliterature.

However,theresultsarein qualitativeagreementwith

theexperimentalresults.

IntheFig. 2,weshowthedriftveloityasa

fun-tion of the eletri eld at 300K and 77K. For these

data weanonludedthat theionizedimpurity

sat-tering is more pronounedat 77K.However, when we

observetheinuene oftheimpurityonentrationon

the transport, the qualitative resultsremain thesame

for bothtemperatures. Also,isobservedthat at 300K

thedriftveloityislinearwiththeeletrield (F)up

to 8 kV/m, sothe relationfor thehole driftveloity

v

h

= F is still valid in this range. This is a diret

onsequenethatthedissipativeeetsstilldon'twork

upto 7kV/m. Thesimilareetshasbeenfoundfor

GaAs [13℄ at room temperature. On the other hand,

at 77K theGaSb showsa dierentbehavior,the drift

veloityremainlinerupto1.5kV/matNi=0and3

kV/matNi=2.72x10 17

m 3

,butstartlatertoshow

thesublinearbehavior. Thisbehavioranbeexplained

due to the fat that the dominant part of the

popu-lation of holesis sattered to emit optial phonons in

with energy. On the other side, at 300K, the

domi-nantpartof thepopulationof holesis shiftedtowards

higherenergies with respet to other ase. The

emis-sion of optial phonons in this range of energy, is no

moreinreasingbuttendstosaturateandforveryhigh

energiesderease[13℄.

10

100

1000

M

ob

ility (c

m

2

/(V

.s

))

Temperature (K)

Experimental

EMC

Figure1. Dependeneof the hole mobility with the

tem-perature.WeonsiderNi=2.72x10 17

m 3

forholedoping

andaompensationof5.2x10 15

m 3

.

0

1

2

3

4

5

6

7

8

0,0

0,5

1,0

1,5

2,0

D

rift V

elo

ci

ty ( 1

0

7

c

m

/s

)

Electric Field (kV/cm)

T = 300 K N

i

= 2.72x10

17

cm

-3

T = 77 K N

i

= 2.72x10

17

cm

-3

T = 300 K N

i

= 0 cm

-3

T = 77 K N

i

= 0 cm

-3

Figure2.Holedriftveloityasafuntionofexternaleletri

eldfortwodierenttemperaturesanddopinglevels.

(3)

oftheapplied eletrield. Theresultsshownthat at

300Kthesystemismoredependentofthethermal

en-ergythanat77K.Inthisalulation,weobservedthat

light holes start to heat up at elds for whih heavy

holesare still lose to the thermal energy. It is

inter-esting tonote thatat 77Kasharptransition fromthe

thermalenergytotheheatedenergymakethearriers

unable to releasefor the lattie the inreasing energy

aquiredbyeletrield [18℄.

0

1

2

3

4

5

6

7

8

0

1

2

3

4

5

6

7

8

T = 300 K

T = 77 K

(

ε

/

ε

0

)

Electric Field (kV/cm)

Figure3.Ratiobetweentheholemeanenergyandthe

ther-malenergyasafuntionoftheexternaleletrieldinpure

p-GaSb.

IV Summary

Fromthepresentedstudyweshownresultsforthehole

transport in GaSb. Our results for the temperature

dependene of the mobility math with experimental

resultsabove90K. Thestudy realizedby Damayanthi

and o-workers[7℄ do notsupport the available

exper-imental results. Aboutthis disrepany, we speulate

that there are two possibleexplanations: i) the eet

oftheband struturethatmakewarpmodel

unappro-priatedforlowtemperaturesandlowelds;ii)The

pa-rametersA, Band C slight hange with temperature.

We expeted that a better understanding of the hole

transport to this material anbe improved when

ad-elds and the inuene ofthe temperature onvalene

band.

Aknowledgments

This work was supported byCNPq (Conselho

Na-ional de Desenvolvimento Cient

io e Tenologio

-Brasil).

Referenes

[1℄ P.S.Dutta,V.Prasad, andH.L. Bhat,Journal Appl.

Phys.80,2847(1996).

[2℄ Y. Horikoshi, Semiondutors and Semimetals, V. 22,

PartC,93,(AademiPress, NewYork,1985).

[3℄ A.G.Milnes,A.Y.Polyakov,Sol.StateEletr.36,803

(1993).

[4℄ H. Kitabayashi, T. Waho, and M. Yamamoto, Appl.

Phys.Lett.71,512(1997).

[5℄ J.Johnson,JournalAppl.Phys.80,1116(1996).

[6℄ L.Esaki,J.CrystalGrowth52,227(1981)

[7℄ P.Damayanthi,R.P.Joshi,andJ.A.MAdoo,Journal

Appl.Phys.88,817(2000).

[8℄ K.Tomizawa,NumerialSimulationofSubmiron

Semi-ondutor Devies, (Arthe House, Boston-London,

1993).

[9℄ J. Singh, Physis of Semiondutors and their

Het-erostrutures,(MGraw-Hill,London,1993).

[10℄ C. Jaoboni, P. Lugli, The Monte Carlo Method for

Semiondutor Devie Simulations, (Springer-Verlag,

Wien-NewYork,1989).

[11℄ N.Nintuze,M.A.Osmani,Semiond.Si.Tehnol.10,

11(1995).

[12℄ S.Bosi, C.Jaoboni, and L. Reggiani, Journal Phys.

C:SolidStatePhys.12,1525(1979).

[13℄ M.Costato,C.Jaoboni,andL.Reggiani,Phys.Stat.

Sol.b52,461(1972).

[14℄ P. J.Briggs,A. B.Walker, andD. C.Herbert,

Semi-ond.Si.Teh.13,692(1998).

[15℄ G.Dresselhaus, Phys.Rev.100,580(1955).

[16℄ J. Kolodziejzak, S. Zukotynski, and H. Stramska,

Phys.Stat.Sol.14,471(1966).

[17℄ J.Robert,B.Pistoulet,D. Barjon, andA. Raymond,

J.phys.Chem.Solids34,2221(1973).

Imagem

Figure 2. Hole drift veloity as a funtion of external eletri
Figure 3. Ratio between the hole mean energy and the ther-

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