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    Circuit model for traveling wave semiconductor laser

    ampliersWeiyou Chen *, Aijun Wang, Yejin Zhang, Caixia Liu, Shiyong Liu

    Department of Electronic Engineering, Jilin University, Changchun 130023, People's Republic of China

    Received 2 December 1999

    Abstract

    A circuit model of a traveling wave semiconductor laser amplier is presented for the circuit level simulation of

    single device or Optoelectronics Integrated Circuit (OEIC) included ampliers. To verify the model, the simulated

    results are compared with the experimental results. 2000 Elsevier Science Ltd. All rights reserved.

    Keywords: Traveling wave amplier; Circuit model; Computer-aided analysis

    1. Introduction

    A semiconductor laser is capable of amplifying lin-

    early coherent light, below the threshold. Linear semi-conductor laser ampliers (SLA) are of two types: one is

    the traveling wave (TW) amplier [1,2], and the other is

    the FabryPerot (FP) amplier. The principle of

    TW-SLA and FP-SLA is identical, i.e. intrinsic stimu-

    lated light amplication. The dierence is reectivity of

    facets. FP-SLA is of a higher reectivity; light propa-

    gates reciprocally in cavities, resulting in resonance

    amplication. TW-SLA is of a lower reectivity; the

    incident light is amplied in a single pass. TW-SLA is of

    greater interest than FP-SLA. This article mainly studies

    the circuit model of TW-SLA.

    2. Model description

    Traveling wave-semiconductor laser amplier oper-

    ates in a multi-longitudinal mode, so it is necessary to

    construct a circuit model by means of multi-longitudinal

    mode rate equations. However, it is very complex to do

    so, because the mode number is an uncertainty and a

    large value. In our previous works [3], we adopted the

    assumption [3] that the emission spectra of the amplier,

    as a function of wave-length is of Gausss shape. This

    assumption is also used in this article. For the conve-

    nience of derivation, we suppose that the output of theamplier is the linear superimposition of amplied

    spontaneous emission and signal so that the spontane-

    ous emission and signal can be processed separately.

    2.1. Signal propagation behavior in a cavity

    Fig. 1(a) schematically shows the propagation be-

    havior of signal in a cavity. Here, we assume that the

    incident light is illuminated on the left facet. The signal

    photon density distributions are shown schematically in

    Fig. 1(b), sf stands for the propagation in +z, and sb

    stands for the propagation in)

    z. Under the assumptionof uniform gain along the cavity, sf and sb can be written

    as

    sf sf0 expgmzY 1

    sb sbL exp gmL zY 2

    where, gm is the average net gain,

    gm CgnY ki aintY 3

    C is the optical connement factor, aint is the cavity

    absorption coecient, ki is the signal light wavelength, g

    is the gain function. Because TW-SLA operates under

    Solid-State Electronics 44 (2000) 10091012

    *Corresponding author.

    0038-1101/00/$ - see front matter 2000 Elsevier Science Ltd. All rights reserved.

    PII: S 0 0 3 8 - 1 1 0 1 ( 0 0 ) 0 0 0 1 5 - 0

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    a threshold, gain saturation eect can be neglected, gas a

    function of carrier density and wavelength can be rep-

    resented as

    gnY k g0n ntrf1 2k kp2aDk2ggY 4

    where, g0 is the gain constant, n is the carrier density in

    an active region, ntr is the transparency carrier density,

    Dkg is the FWHM of this function, kp is the center

    wavelength.

    At the left and right facets, the boundary conditions

    are

    sf0 sin RLsb0Y 5a

    sbL RRsfLY 5b

    where, sf0 and sb0 are the forward and backward prop-

    agation photon densities at the left facet, respectively,

    whereas sfL and sbL are the photon density at the right

    facet. RL and RR are the re ectivity of left and right

    facets. sin is the incident photon density at left the facet,

    as a function of incident light power can be expressed as

    sin giPin

    hmWDcHY 6

    where, Pin is the incident light power, gi is the incident

    eciency, hm is the signal photon energy, W and D are

    the width and thickness of the cavity. cH is the light speed

    in the medium.

    From Eqs. (1) and (2), we can get

    sfL sf0 expgmLY 7a

    sb0 sbL exp gmLY 7b

    where L is the cavity length.

    Solving the equation set of Eqs. (5) and (7),

    sf0

    sin

    1 RLRR exp2gmL X 8

    The average signal photon density is

    ss 1

    L

    L0

    sf sbdz

    sin1 RR expgmL exp gmL 1

    gmL1 RRRL exp2gmLX

    9

    The signal output powers from the left and right facets

    are

    PoutL hmWDcH1 RLRRsf0 exp 2gmLY 10a

    PoutR hmWDcH1 RRsf0 exp gmLX 10b

    2.2. Model derivation

    According to Eqs. (10a) and (10b), if gm is known, it

    is easy to get the signal output. However, it is very dif-

    cult to get gm, because gm is determined with the carrier

    density, and the carrier density is relative to spontaneous

    emission recombination, nonradiative recombination,

    and stimulated emission recombination. Therefore, we

    must solve the carrier and photon rate equations. Due tocontinuous spectrum operation of TW-SLA, we adopt

    multi-longitudinal mode rate equations,

    dn

    dt

    Ij

    Q Rnn Rrn

    I0

    CcHgnY ksk dk

    CcHgnY kissY 11

    dsk

    dt CcHgnY ksk

    sk

    sph bspkRrnY 12

    where Ij is the injection current, Q qVact, q is theelectron charge, Vact WDL. Rn(n) and Rr(n) are thenonradiative and radiative recombination rates, respec-

    tively [3].

    According to the assumption of the Gaussian func-

    tion of spontaneous emission spectra, the spontaneous

    emission photon density as a function of wavelength can

    be expressed as [3]

    sk sp expf4 ln2k kp2aDkp

    2gY 13

    where s(k) is the total photon density inside and outside

    the active region per unit wavelength, dening as the

    total photon number inside and outside the active region

    divided by active region volume. This is equivalent to

    compressing the photon outside the active region into

    Fig. 1. (a) Schematic propagation of the signal, and (b) sche-

    matic of the photon density distribution.

    1010 W. Chen et al. / Solid-State Electronics 44 (2000) 10091012

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    the active region, but those photons are not capable of

    stimulating. sp is the peak value, Dkp is the FWHM.

    The processing method of Eqs. (11) and (12) is sim-

    ilar to that in Ref. [3].

    The output powers of the spontaneous emission from

    the left facet and the right facet per unit wavelength are

    pLk hc2WDRL 1 ln RLRR

    2ngk1 RL RLaRR

    p1 RR

    skY 14a

    pRk hc2WDRR 1 lnRRRL

    2ngk1 RR RRaRL

    p1 RL

    skX 14b

    From integralI

    0pkdk, the total output power can be

    obtained. In general, if Dkp ( kp, then the k in de-nominator of Eq. (14) can be replaced by kp. The total

    output powers are

    PL hc2WDRL 1 ln RLRR

    2ngkp1 RL RLaRR

    p1 RR

    stotY 15a

    PR hc2WDRR 1 ln RRRL

    2ngkp1 RR RRaRL

    p1 RL

    stotX 15b

    Based on Eqs. (10)(12) and (15), we construct the

    TW-SLA circuit model as shown in Fig. 2, where

    Isti QCcHgnY kiss. The other meaning of the elements

    in this circuit model is similar as in Ref. [3].

    There are seven ends in this model, the two ends re-

    lated to Ve

    correspond to real electrical ends, the upper

    one is for anode, the lower one is for cathode. The other

    ve ends are virtual. The end marked with Pin is for the

    power input; the input light source must be regarded as

    the voltage source. The four ends placed at the lower

    right are for signal output and spontaneous emission

    output from the left and the right facets.

    3. Simulation

    The above model is converted to the subcircuit of

    PSPICE; the simulation has been done by using

    PSPICE, with the circuit shown in Fig. 3. Most of the

    model parameters are mainly taken from Refs. [1,2,4], as

    shown in Table 1. The parameters not shown in Table 1

    are set to be zero.

    To verify the model, the simulated results have been

    compared with the experimental results given in Ref. [1],

    as shown in Fig. 4. The solid curves are the simulated

    results, the scatters are the experiment results. It can be

    seen that for a smaller biased current, simulated resultsagree well with the experimental results. For high cur-

    rent, the output power of the right facet is far away from

    the experimental result. This has resulted the gain sat-

    uration eect is not being included in this model.

    As examples, the other characteristics of the

    TW-SLA have been simulated (Figs. 5 and 6). Fig. 5

    shows the output power versus the incident power; it can

    be seen that when the incident power increases, the

    spontaneous emission output power decreases, the signal

    Table 1

    Model parameters

    Parameters

    (unit)

    Value Parameter

    (unit)

    Value

    An1 (s1) 2 108 Rs (X) 1

    An3 (cm6 s1) 5 1029 Vbi (V) 1.13

    Ar2 (cm3 s1) 1.4 1010 W (lm) 600

    Cp (pF) 10 Dkg (nm) 150

    Csc0 (pF) 10 Dks (nm) 150

    D (nm) 10 C 0.05

    ng 4.0 aint (cm1) 3

    G0 (cm3 s1) 1.9 106 bsp0

    (lm1)

    6 104

    L (lm) 1500 g 2

    ntr (cm3) 1.2 1018 gi 0.7

    nr 3.4 ki (lm) 0.9

    Rd (X) 1 1010 kp (lm) 0.86

    RL (RR) 0.0026Fig. 2. The circuit model of TW-SLA.

    Fig. 3. The circuit for simulation of TW-SLA.

    W. Chen et al. / Solid-State Electronics 44 (2000) 10091012 1011

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    output power from right facet increases, the signal out-

    put from left facet increases initially and then decreases.

    The amplication ratio (dened as the right facet signal

    output power/incident power) decreases with an increase

    in the incident power. This is because for a xed biased

    current, the increase in the incident power will result in

    the increase of the photon density, the decrease of the

    carrier density, and of the medium gain.

    Fig. 6 gives the output power versus reectivity. As

    shown in this gure, the output powers from the left and

    the right facets are close to each other, with increasing

    reectivity.

    4. Conclusion

    A circuit model of TW-SLA has been presented for

    the circuit level simulation of OEIC with this type of

    device. This model can be used to simulate the DC, AC

    and transient characteristics of single TW-SLA or

    OEIC.

    References

    [1] Goldberg L, Mehuys D, Hall DC. 3.3W CW diraction

    limited broad area semiconductor amplier. Electron Lett1992;28(12):10824.

    [2] Goldberg L, Mehuys D. 21W broad area near-diraction-

    limited semiconductor amplier. Appl Phys Lett 1992;

    61(6):6335.

    [3] Chen W, Liu S. Circuit model for multilongitudinal-mode

    semiconductor lasers. IEEE J Quant Electron 1996;32(12):

    212832.

    [4] Dai Z, Michalzik R, Unger P, Ebeling KJ. Numerical

    simulation of broad-area high-power semiconductor laser

    ampliers. IEEE J Quant Electron 1997;33(12):224053.

    Fig. 4. Signal output power versus biased current. The incidentpower is 500 m W ((d) right facet output, () left facet output).

    Fig. 5. The output power versus the incident power, under

    dierent biased currents. The dashed curves are for spontane-

    ous emission, the dotted curves are for signal output from the

    left facet, the solid curves are for the signal output from the

    right facet.

    Fig. 6. The output power versus the re ectivity: The solidcurves are for signal output from the right facet and the dashed

    curves are for signal output from the left facet.

    1012 W. Chen et al. / Solid-State Electronics 44 (2000) 10091012