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Many Partile Theory for the Luminesene,

Charaterization and Simulation of

Quantum Well Laser Strutures

M.F. Pereira Jr.,

InstitutodeFsia,UniversidadeFederaldaBahia,40210-340, SalvadorBABrazil

A. A.Bernussi, W. Carvalho Jr.,MarioT. Furtado,and A. L. Gobbi

LaboratoriodeOptoeletr^onia, LNLS,13083-970,Campinas,SP, Brazil

Reeivedon23April,2001

A photonGreen's funtion theoryis usedto inorporate Bethe-Salpeter-like many body

orre-tions in the the omputations of nonlinear optial spetra of semiondutor quantum well laser

materials. The numerial results presented reprodueseveral features found inthe experimental

haraterization oftheatualdevies.

Thesimulationofsemiondutorlasersisa

fasinat-ing hallengeto modernPhysis.[1℄They operatein a

highlyexitedregime,wheremany-partileeetsplay

adominantrule.[2℄ A previous approah for quantum

well lasers has suessfully desribed the ombination

of resonantavity, band struture and manybody

ef-fetsinatemperatureregimeandformaterialswherea

vertex-typeofapproximationstillsuessfullydesribes

the exited media.[3℄ There are howeverexperimental

onditions,speiallyatlowtemperatures,wherehigher

orderCoulomborretionsmustbedealtwith. Amore

general theory is thus required. [4, 5℄ In this paper

wepresentsolutionsofaBethe-Salpetertypeof

equa-tion forquantum wells within a photonGreen's

fun-tionsapproahapableofhandlingtheresonantavity

mirosopially, as well as quantum onnement and

band strutureeets. Themirosopiapproah

on-sistently desribesPauli-bloking,thesreening ofthe

Coulombinteration,Coulombenhanementofthe

po-larizationfuntion,andbandgap shrinkage.

The many-body approah used here is based on

Keldysh Green's funtions for arriers (G), photons

(D),and plasmons (W)to desribetheoupled

light-exited semiondutor system. [3, 4, 6, 7℄ Here, we

just outline the method with words and a few

repre-sentative equations. The Keldysh Green's funtion's

time evolution is desribed byDyson equations,

har-aterizedbyfreepropagatorsG 1

o ,D

1

o ,W

1

o

,and

self-energies,,P,andp,beingthearrierself-energy,the

transverse,andthelongitudinalpolarizationfuntions,

respetively. Detailed band-struture and

quantum-Hamiltonian, are inluded in the free-arrier

propaga-torG 1

o

, andserveastheinputforthesolutionofour

many-bodyproblem. Eahoftheselfenergieshanges

thebareintodressedpropagatorsin aspeiway.

ThetransversepolarizationP desribestheoptial

responseofthesystem,andanbewrittenasasumof

anRPAtermandaCoulomb-orrelationontribution,

expressed by thesolutions of the(integro-dierenial)

Bethe-Salpeterequation,[4℄

P(1;1;2;2)=G(1;2)G(2;1)+G(1;3)G(4;1)P(3;4;2;2):

(1)

Inordertodesribelightemission,werefertothe

quan-tum mehanial Poynting vetor. If we neglet

reso-nantavityeets,thePLspetrumisgivenessentially

by the arrier reombination spetrum, desribed by

P <

(!). If wewish to desribe the avity, the photon

Green's funtion presented here handles the problem

in rst priniples. The polarization funtion satises

the Kubo Martin Shwinger (KMS) sum rule. [2, 4℄

So,oneImPrisomputed,thearrierreombination

spetrais immediately obtained, ( is the total,

ele-tron+hole,hemialpotential),

P <

(!)=

2iImfP r

(!)g

1 exp((~! ))

: (2)

Fig. 1 ompares the measured (symbols)

photolumi-nesene (P.L.) with the numerial solutions of Eqs.

(2)

Figure1. Photoluminesenespetraofa30nmInGaAsP

quantumwell at 300K. Thesymbols depit experimental

results, while the solid and dashed urves are omputed,

respetivelywithandwithoutinhomogeneousbroadening.

Figure 2. Evolutionof theabsorptionspetra(solid)from

thelinearregime(topurve)tothegainregion,asthe

exi-tationarrierdensityisinreasedthemedium. Thedashed

urveistheP.L.omputedforalowarrierdensityandthe

symbolsare experimentaldata. All numerial parameters

are equal to those of Fig.1 for a 30 nm InGaAsP

quan-tumwellat300K.(a)and(b)areomputed,respetively,

withoutandwithinhomogeneousbroadening.

Further experimental investigations (not shown)

suggest a sizable Stokes shift between P.L. and

pho-tourrent measurements (P.C.). Although the

resolu-tion of the P.C. is not high enough at the moment

for nal onlusions, a Stokes shift an be desribed

by the theory, as shown in Fig. 2. The

inhomoge-neousbroadeningissimulatedherebymeansofa

Gaus-sian distribution of thefundamental band gap,as

de-pitedinFig.2. fortheomputednonlinearabsorption

spetra obtainedfrom dierentarrier densities, from

(!) =(2! p

(1)) ImP r

(!), for the QW of Fig.

1. NotetheinreaseofStokesshiftbetweenabsorption

and emissionin theinhomogeneouslybroadenedurve

(b) in omparison with (a). Possible explanations for

quaternary alloy (InGaAsP), reduing the band gap,

and inreasing the Stokes shift between emission and

absorption. (ii) Non- mixing of the quaternary alloy

in the well and barrier regions, givingrise to gap

en-ergymodulation, broadeningtheemissionpeak. Both

eetsarestronglydependentonthegrowth

tempera-ture,andatthattemperature,thewellmaterialwould

be outof thenon- mixing region. However,bothwell

and barrier ould be ordered at that temperature. A

more detailed experimental analysis is foreseen for a

ompleteomparisonwithexperiments.

Theabsorption spetrahereontainsonlytherst

fewtransitions. A diret omparison with thefull

ex-perimentalphotourrentspetrum,requiresallallowed

transitions(notshown). Thetransitionsdepitedplay

themajorroleinthegainspetra,sinethehigher

sub-bandsarenotappreiably populated.

Fig. 3 depits the inreasing Stokes shift with

inho-mogeneousbroadeningahievedhere,byinreasingthe

broadeningoftheGaussiandistribution.

Figure3. LinearAbsorptionpeak(triangles)andPeak

Lu-minesene(irles)asafuntionofinhomogeneous

broad-ening,desribedbythewidthoftheGaussiandistributions

broadening.

In summary, regardlessof the eetive

dimension-alityofthesystemthemirosopimehanismsgiving

rise to optial gain, the semiondutor must be

on-sistently treated as both resonator and gainmedium.

Highdensity(e.g. Vertex)approximations,maybe

mis-leading,speially forsystems with largeexiton

bind-ingenergy,andareavoidedhere,bymeansofaphoton

Green's funtion theory for quantum well laser

spe-trathat allowstheonsistentinlusionofbeyondRPA

orretions in the polarization funtion by means of

Bethe-Salpeter-Equation-likeorretions. The

numer-ial odes used here inlude a simplifying ansatz for

thenon-interating polarizationbubbleused asinput

for the full numerial solution of the Bethe- Salpeter

equationdiagramthatinludesCoulomb-Many-Body

orretions. The algorithm avoids a Kramers-

Kro-nig integration in the loop and allows the redution

of a omplex to a real matrix in the numerial

ma-trixinversionomputation that inreasesthe speed of

(3)

re-physial eetsand makeastarting pointfor

simulat-ing the operation of semiondutor lasers, ampliers,

and otherhot-semiondutor-avityoptoeletroni

de-vies,andtheurrentnumerialresultssuessfully

re-produeseveraloperationalharateristisofthelasers

developedat Funda~aoCPQd-LNLS.

Aknowledgments

Researh supported by Conselho Naional de

Pesquisas,CNPqofBrazil.

Referenes

[1℄ P. Zory, Quantum Well Lasers, Aademi Press, San

Diego,1993.

[2℄ R. Zimmermann, Many-Partile Theory of Highly

Ex-ited Semiondutors, "Teubner Texte zur Physik",

Leipzig(1987).

[3℄ M.F.PereiraJr.andK.Henneberger,Phys.Rev.B53,

16485(1996).

[4℄ M.F.PereiraJr.andK.Henneberger,Phys.Rev.B58,

2064 (1998).

[5℄ P.Mihler,M.Vehse,J.Gutowski,M.Behringer,andD.

Hommel,M. F.PereiraJr.,andK.Henneberger,Phys.

Rev.B58,2055(1998).

[6℄ K. Henneberger and S.W.Koh, Phys.Rev.Lett. 76,

1820 (1996).

[7℄ K. Henneberger and H. Haug, Phys.Rev. B 38, 9759

Imagem

Figure 1. Photoluminesene spetra of a 30 nm I nGaAsP

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