Optically injected laser system: Characterization of chaos, bifurcation, and control

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    Optically injected laser system: Characterization of chaos bifurcation and

    control

    Santo Banerjee, Papri Saha, and A. Roy Chowdhury 

    Citation: Chaos 14, 347 (2004); doi: 10.1063/1.1755179 

    View online: http://dx.doi.org/10.1063/1.1755179 

    View Table of Contents: http://chaos.aip.org/resource/1/CHAOEH/v14/i2 

    Published by the American Institute of Physics. 

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    Optically injected laser system: Characterization of chaos, bifurcation,and controla…

    Santo Banerjee,b) Papri Saha,c) and A. Roy Chowdhuryd)

     High Energy Physics Division, Department of Physics, Jadavpur University, Kolkata—700032, India

    Received 17 December 2003; accepted 5 April 2004; published online 21 May 2004

    A single mode semiconductor laser subjected to optical injection, described by a set of three coupled

    nonlinear ordinary differential equations, exhibiting chaos is considered. By means of a recurrenceanalysis, quantification of the strange attractor is made. Analytical studies of the system using

    asymptotic averaging technique, derive certain conditions describing the prediction of 1→2

    bifurcation, which have subsequently been verified on numerical simulation. Furthermore, the locus

    of points on the parameter phase space representing Hopf bifurcation has been derived. The problem

    of control of chaos by a new procedure based on adaptive stabilization is also addressed. The results

    of such control are shown explicitly. Though this analysis deals with a very specific set of equations,

    the overall features that come out of the study remains valid for almost all laser systems. ©   2004

     American Institute of Physics.   DOI: 10.1063/1.1755179

    Different kinds of chaotic phenomena can be observed in

    an optically injected semiconductor laser system. We

    present here a different aspect of such laser model whose

    parameter space is analyzed through bifurcation dia-

    grams exhibiting period doubling route to chaos. Chao-

    ticity of the system is quantified through recurrence

    analysis which can identify hidden periodicity and distin-

    guish between a random signal and deterministic state.

    Transition points in bifurcation, obtained through nu-

    merical simulations, is verified with the analytical calcu-

    lations. A new type of control mechanism is constructed

    and applied, and the results are discussed in detail. The

    results may provide some new features in the study of 

    semiconductor lasers which has wide application in the

    field of signal processing and data transmission.

    I. INTRODUCTION

    Optically injected semiconductor lasers exhibit a variety

    of phenomena.1 Experimental and numerical research has re-

    vealed different kinds of chaotic properties.2– 8 Studies on

    single mode semiconductor laser show that they adopt a

    number of different routes to chaos,9 such as period dou-

    bling, torus break up and subsequently torus doubling route

    to chaos. Analysis of a laser with injected signal consists of 

    Adler’s phase equations10 which in bifurcation terms exhibits

    a saddle node infinite periodic bifurcation.

    11

    Numericalanalysis of the full three-dimensional equations produce

    Hopf bifurcations,12,13 period doubling cascades,3,14,15 and

    quasiperiodicity.12,16 Among the main features of laser in-

     jected with signal, accounted for by the averaged equations,

    there are saddle node bifurcations and relaxation oscillations

    which originate in a Hopf bifurcation. Hopf-saddle-node bi-

    furcation was discussed by Solari and Oppo.17

    Another recent analysis of the laser system18 supports

    the results based on the averaged equations of Ref. 17 ad-

    vanced in Ref. 19, namely, that the special reinjection present

    in the laser with injected signal together with the Hopf 

    saddle node type are responsible for the organization of bi-

    furcations. Zimmermann   et al.20 presented a consistent

    perturbation-approximation framework to the laser equations

    in order to incorporate larger degrees of complexity in the

    model. It was also established that the homoclinic bifurca-

    tions in such a model instead of involving the locking solu-

    tions, involves the undamped relaxation oscillations associ-

    ated with the Hopf bifurcations of the Hopf-saddle-nodebifurcation. The simplest invariant solutions of the equations

    were derived by the averaging procedure, as was the locus of 

    the Hopf-saddle-node bifurcation and the normal form com-

    putations were performed.

    In this paper we present a totally different aspect of the

    model analyzed by Krauskopf  et al.9 The chaoticity of the

    system is quantified through visual recurrence analysis21

    which was first described by Eckmann, Kamphorst, and

    Ruelle.22 This is a new graphical device for the qualitative

    assessment of time series and one can graphically detect hid-

    den patterns and structural changes in the data or see simi-

    larities in patterns across the time series under study. Then

    the identification of Hopf 23,24 and period-doubling25 bifurca-tion in the system of optically injected semiconductor laser

    through analytical calculations is taken up. The motivation

    was to verify that such transition points found through nu-

    merical simulations, indeed matched the analytical results

    obtained. We see that under certain parameter conditions,

    Hopf bifurcation exists in the given system. A curve is de-

    rived from analytical conditions such that each point on the

    curve represents a Hopf point. On the other hand, in a sepa-

    rate study the bifurcation of a period-1 orbit has been dem-

    onstrated, based upon the asymptotic averaging techniques.

    aThis work is dedicated to the memory of our beloved friend Mousumi

    Saha.bElectronic mail: [email protected] mail: [email protected] to whom correspondence should be addressed. Electronic mail:

    [email protected]

    CHAOS VOLUME 14, NUMBER 2 JUNE 2004

    3471054-1500/2004/14(2)/347/11/$22.00 © 2004 American Institute of Physics

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    We have verified analytically that the points of 1→2 bifur-

    cation on the bifurcation diagram actually satisfy the re-

    quired conditions. Along with these, the method of adaptive

    stabilization is implemented, which is different from the con-

    ventional control strategies such as the OGY method,26 ex-

    ternal harmonic forcing,27 adaptive and threshold control,28

    etc. This method has shown good results for the control of 

    chaos in Lorenz system.29

    The above analysis has been carried out on opticallyinjected laser system but such chaotic properties are also

    observable in other laser types.30–32 The results are almost

    valid for those systems and so the observations of these type

    of analysis is equally applicable to them.

    II. FORMULATION

    The set of equations governing a single mode semicon-

    ductor laser subjected to optical injection is given by

     E ˙ 12 1i  i  E ,   2.1

     ˙2  12    E 21 ,   2.2

    where   E   is the complex electric field,      is the population

    inversion,    is the injected field strength,    the detuning of 

    the electric field from the solitary laser frequency,      is the

    linewidth enhancement factor,     is the cavity lifetime, and 

    is the damping rate. Substituting  E  x 1ix 2  and    x 3  and

    performing simple algebraic steps, Eqs. 2.1–2.2 are trans-

    formed to three ordinary differential equations as

     ẋ 1  x1 x 3

     

    2 x 2 x 3  x2 ,   2.3

     ẋ 2  x 1

     

    2  x 1 x 3

     x2 x 3

    2   ,   2.4

     ẋ 32 x3 12  x3  x12 x 2

    21 .   2.5

    Equations  2.3–2.5  show that   0,0,0   is not a fixed point.

    Considering  , the analytical fixed point is obtained as

     x 12  p

     p2 2   p 2 ,

     x 22    p2 

     p 2 2   p 2 ,   2.6

     x3

     p ,

    where  p  is a real number satisfying the condition

     p 2  21 4 p  2 2 4 2 2 0.

    Assuming,    2 2 /   ( 4 )   another analytical fixed

    point arises as

     x 1 

     

     x 20,   2.7

     x 32 

       .

    The system of equations under study are thus analyzed for its

    dynamical behavior around the existing fixed points under

    the effect of the parameters for its chaotic and periodic prop-

    erties. Exploring through the parameter regime, Hopf bifur-

    cation, intermittent transition to chaos and periodic doubling

    routes were observed. Two bifurcation diagrams have been

    depicted, which are part of the total bifurcation spectrum of 

    that particular parameter regime. Figures 1 and 2 demon-

    strate a gradual period doubling and these are specially im-

    portant to visualize the point of 1→2 bifurcation. These

    points are later used in Sec. IV for analytical verification of 

    the 1→2 bifurcation. The points are indicated in the figures

    by an arrow. In the figures, windows in between the chaotic

    regions is also seen. On comparing, it is also seen that the

    chaoticity is denser in the first than the second. This also

    points out to the separation of the neighboring points in

    phase space. For Fig. 1, the parameter     is varied and thevalues of the other parameters are

     2.0,    0.015,   0.035,    0.62,   2.8

    whereas for Fig. 2,    is varied and the other values are

     2.5,    0.015,   0.05,    0.2.   2.9

    Other than these, torus bifurcations and intermittency were

    also found with the variation of the parameters      and    

    FIG. 1. Bifurcation diagram showing the variation of the variable x  with   .

    FIG. 2. Bifurcation diagram showing the variation of the variable  y  with   .

    348 Chaos, Vol. 14, No. 2, 2004 Banerjee, Saha, and Chowdhury

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    which is not depicted. Along with the analytic study of pe-

    riod doubling, the case of analytic detection of Hopf bifur-

    cation is also considered. Before proceeding to that, the

    quantification of the chaotic region is studied, which gives a

    visual understanding to the properties of the attractor.

    III. QUANTIFICATION OF THE ATTRACTOR THROUGHRECURRENCE ANALYSIS

    In the method of recurrence analysis, an attractor is re-

    constructed from a given time series of the nonlinear dy-

    namical system of equations. To expand a one-dimensionalsignal or time series into an  m-dimensional phase space one

    substitutes each observation in the original signal  X (t ) with

    vectors,

     y i  x i , x id , x i2d , . . . , x i m1 d ,

    where   i   is the time index,  m   is the embedding dimension,41

    and   d   is the time delay. As a result we have a series of 

    vectors,

    Y  y 1 , y 2 , y 3 , . . . , y N  m1 d .

    From this new reconstructed dynamical system, a recurrence

    plot can be used to show which vectors in the reconstructed

    space are close and far from each other. We calculate thedistance between all pairs of vectors and plot them. In the

    diagram ‘‘dark’’ points show large distances between vectors

    while ‘‘light’’ denote small distances. Since the distance of 

    the ith vector to the  jth vector is the same as that of  jth to  ith

    vector, recurrence plot is symmetric and the diagonal of the

    plot is a white line. The recurrence plot carried out with

    10 000 data points is shown in Fig. 3. The   x-axis and the

     y-axis represent the data points and so do not have any unit

    and each point on the plot represent their mutual distance.

    The time delay is estimated by the mutual information func-

    tion. The point where the average mutual information

    reaches its first minimum is considered as the optimal time

    delay. The embedding dimension is obtained from the false

    nearst neighbor method which was suggested by Kennel

    et al.42 The dimension for which the proportion of false near-

    est neighbors is minimum is chosen. The embedding dimen-

    sion and time delay obtained in our case are 3 and 7, respec-

    tively. On observing the plot we can see that there is no

    definite repeating pattern. Such irregular patterns represent

    chaoticity and cannot be seen in any periodic signals.

    Contrary to the above one can also make a nonparamet-ric time series prediction without any assumption about the

    functional form of the process that generated the observable

    time series. The methodology behind this is that to predict a

    point   x(n1), we determine the last known state of the

    system as represented by vector

     X  x n , x nd , x n2d , . . . , x n m1 d  ,

    where   d   and   m   have their usual meanings. Then the time

    series is searched to find   k   similar states that have occurred

    in the past, where ‘‘similarity’’ is determined by evaluating

    the distance between vector  X   and its neighbor vector  X    in

    the   d -dimensional state space. If the observable signal wasgenerated by some deterministic map

     M  x n , x nd , x n2d , . . . , x n m1 d 

     x n1 ,

    then the map can be recovered from the data by looking at its

    behavior in the neighborhood of  X . We find the approxima-

    tion of   M   by fitting a polynomial which maps   k   nearest

    neighbors of similar states of   X   onto their next immediate

    values. Now using this map   x(n1) is predicted. So with

    the assumption that  M   is fairly smooth around  X   if a state

     X  x

    n , x

    nd , x

    n2d , . . . , x

    n m1 d 

    in the neighborhood of   X   resulted in the observation   x(n

    1) in the past, then the point  x(n1) which we want to

    predict must be somewhere near  x(n1).

    Normally the data set is divided into two parts. The first

    part is used for model fitting and the second part for model

    validation. In our case we have a total of 7530 data points

    out of which the first 3367 are utilized for model fitting and

    the rest are for model validation.

    The embedding dimension has to be chosen properly be-

    cause a low embedding dimension would not reveal the un-

    derlying system properties uniquely and a high embedding

    dimension would lead to increased computation time, ampli-fication of noise, and deteriotion in the quality of predictions.

    The time delay determines the time separation of the com-

    ponents in the reconstructed vector of the system state is to

    be chosen properly. If time delay is set to a low value, then

    the corresponding vector components may be too redundant

    and a high time delay can led to corresponding vector com-

    ponents too independent. Embedding dimension and time de-

    lay was estimated as 3 and 7, respectively.

    Other than these, a kernel have also been chosen which

    is essentially a weighting function used to assign the contri-

    bution of each neighbor to the prediction of the kernel re-

    gression and locally weighted linear predictors.

    FIG. 3. Recurrence plot for the chaotic regime with 10 000 data points.

    349Chaos, Vol. 14, No. 2, 2004 Chaos, uncertainty, control

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    To weigh the contribution of each of the k  nearest neigh-

    bor to the resulting prediction we have,   k (Epanechnikov)

    0.75*(1distance/ h)2.   h   is the bandwidth of the neigh-

    borhood formed by  k  neighbors which is simply the distancefrom the reference state. The predictor was the nearest neigh-

    bor basis and ‘‘one-step-ahead’’ forecast was used. The dis-

    tance was measured by correlation, the root mean square

    error0.0083 and the normalized error0.0006. The varia-

    tion of the predicted and the actual model with time is shown

    in Fig. 4, where we can see that actual values and the pre-

    dicted values almost overlap each other and is only differen-

    tiable at the end of the curve. The time represents the inte-

    gration step of the Runge–Kutta–Fehlberg method which

    was considered to be 0.01.

    IV. PREDICTION OF 1\2 BIFURCATION THROUGHASYMPTOTIC AVERAGING TECHNIQUES

    In Sec. II we have explored the various parameter re-

    gions where the system shows period doubling before attain-

    ing chaos. In this process the system undergoes subsequent

    bifurcations and those are depicted in the bifurcation dia-

    grams. It is possible to predict those points of period dou-

    bling through partly analytical and partly numerical methods.

    In the other sense it is possible to verify that those points

    where bifurcation occur actually satisfy the required analyti-

    cal conditions. This can be done by the asymptotic averaging

    technique which is briefly discussed. The differential equa-

    tion modelled by the formdX 

    dt  F  X ,   4.1

    where   F ( X ) F 1( X ) F 2( X ) F 3( X )T  and   X  X 1 X 2 X 3

    can be partitioned according to

     X  X  1  X  2 ,   F  X F  X  1 G X 1 , X  2 ,

    4.2dX  1

    dt   F  X  1 ,

    dX  2

    dt   G X  1  t , X 2 .   4.3

    Equation  4.2   is for the period-1 orbit and Eq.   4.3   is for

    the period-2 orbit, since  X (1 )( t ) is the period one solution

    of period  T 2  /  , in the region  X (2 )0. In the parameter

    space where   X (2 ) is born   X (1 ) loses its stability. Basically,

    this technique of asymptotic averaging requires transforma-

    tion of Eq.   4.1   in a form that supports the averaging pro-

    cedure. The system coordinates ( X 1 , X 2 , X 3) are transformed

    to the dynamical coordinate ( x , y , z) such that the system of 

    Eq. 4.1  can be expressed as a single third order differentialequation according to

     X i X i x, y , z   i1,2,3,   4.4

    dx

    dt  y ,

    dy

    dt  z , and

    dz

    dt W  x , y , z .   4.5

    These transformations are treated as they are extensively

    used to construct embeddings of scalar experimental data

    into multidimensional phase spaces. If the system of Eqs.

    4.1   were to be linearized around a fixed point, choosing

     X i x   for any   i, one obtains  W g1 xg 2 yg 3 z , where   g 1 1 2 3 ,   g 2 ( 1 2 2 3 3 1), and   g 3 1 2

     3   with    1 ,    2 , and    3   as eigenvalues of the secularequations. In the environment of period one orbit,  W  appears

    as the sum of linear and a quadratic form. The fundamental

    procedure described in Ref. 33 consists of writing each of the

    dynamical variables   x,   y,   z   in the form   x x 1 x2 ,   y y 1 y 2 , and so on, where x 1 ,  y 1 ,... stands for the period 1 and

     x2 ,   y 2   those for period 2. For our system we set   X

    ( X ,Y , Z ),

     X ˙  XZ 

     

    2 Y Z  Y ,

    Y ˙  X  

    2

     X Z Y Z 

    2

      ,   4.6

     Z ˙2 Z  12  Z  X 2Y 21 .

    The transformation of the system to a single third order dif-

    ferential equation is done by choosing   x Z  which leads to

    the following exact but complicated result:

    dx

    dt  y ,

    dy

    dt  z ,

    dz

    dt W ,   4.7

    where

    W  x , y , z 2 z y2 2 12  x  y 24  

     xy

     xz

    1

    2  x 4  yz

    4  xz4  y 2 4 2 y 2 y2 x 12  x 2

    4  y  x 12  x   x 1

    2  x 2   12  x ,   4.8

    where    and    are given by

    1

    2   12  x 2 x 2 xy2  x 2 x  z2 y

    12  x 2 y   y2 x 12  x 2,

    1 y2 x 12  x 1 X 21/2.

    FIG. 4. Variation of the actual   bold line AV   and predicted   thin line

    PV  values of the model with time.

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    We now assume that the parameter      is very small, so that

    we approximate Eq.  4.8  by

    W  x , y , z g 1 xg2 yg3 zhq11 x2q 12 x yq 13 xz

    q22 y2q 23 y zq 33 z

    2,   4.9

    where

    h2 22  ,   g1 4  4 24  ,

    g 2  1,   g 32 ,

    q 118  2  2

     

    4  2 4  

    0.5,

    q 122  4 44  

    2  2  

     

       ,

    q 134 1

    2 0.5,   q 234 

     4 ,

    q 33 

    4 .

    The above transformation yields the following equations:

    dz 1

    dt   g1 x 1g2 y 1g3 z 1hQ x1 , y 1 , z1

    equation for period one orbit   4.10

    so that  x 2   evolves according to

    dz 2

    dt   F 1 t  x 2F 2 t  y 2F 3 t  z2Q x2 , y 2 , z 2

    4.11

    and

    F 1 t g 12q11 x1 t q 12 y 1 t q 13 z 1 t ,

    F 2 t g 22q22 y 1 t q 12 x 1 t q 23 z 1 t 

    equation for period two orbit,

    F 3 t g 32q33 z1 t q 13 x1 t q 23 y 1 t .

    To proceed further we assume a simplest form of period one

    orbit without any higher harmonics which when used in Eq.

    4.10  yields the following conditions:

    q 12q13 D 02

    2q11g 2q 13g3q 12 D 0 g 1g2g 304.12

    and

     D 12

    2 g1 D 0q 11 D 02h

    q11 2 q 22q13

    4.13

    with

     2 g 2q12 D 0, where   x1 t  D 0 D 1 cos t .4.14

    A similar analysis is also performed for the period 2 case and

    with the following substitutions:

     x2u cos t 2 v sin t 

    2  ,   4.15

     y 2 

    2 u sin t 

    2   

    2  v cos t 

    2  ,   4.16

     z2  2u

     

    2

    d v

    dt  cos t 

    2  

    2v

     

    2

    du

    dt  sin t 

    2  .

    4.17u  and   v  are determined by the inverse transformations.34 An

    elaborate computation leads to the following two differential

    equations for  u  and   v:

    d 2u

    dt 2 A 11 t 

    du

    dt   A 12 t 

    d v

    dt   A 13 t u A 14 t v

    U  u,v , . . . , t ,   4.18

    d 2v

    dt 2 A21 t 

    du

    dt   A 22 t 

    d v

    dt   A 23 t u A24 t v

    V  u ,v, . . . , t .   4.19

    The strategic point of the asymptotic averaging technique is

    to approximate the solutions of these two equations by the

    corresponding ones of the averaged differential equations

    written as

    d 2 x

    dt 2

    1

    T  

    0

    F  dxdt 

     , x,t  dt .   4.20Here   x(u,v) with   T 4  /  . Hence the next stage is to

    introduce the following second transformation from (u,v) to

    new coordinates ( y , z) defined by generating functions  1 ,

     2

      as

    u y 1 y , z , d ydt  ,dz

    dt  , t  ,

    4.21

    v z 2 y , z , dydt   ,dz

    dt  , t  .

    The quadratic terms with nonzero averaging values are now

    critical for the onset of period 1→2 bifurcation. The details

    calculations leads to a secular equation which controls the

    stability of the period 2 equation as

     A4 4 A 3 

    3 A2 

    2 A 1  A 00,   4.22

    where A4 1 f 11 1 f 22 f 12 f 21 ,

     A3 d 11d 22 d 11 f 22d 22 f 11d 12 f 21d 21 f 12,

     A2 d 11d 22d 12d 21 e11  e 22   e 11   f 22e 22   f 11

    e21   f 12e 12   f 21,

     A1 d 11e 22  d 22e 11   d 12e 21  d 21e12   ,

     A0e 11   e22  e12  e21   .

    This equation determines the conditions for stability of the

    period two orbit evolving from period one orbit, parallel to

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    the secular equation which determines the conditions for

    evolution to a dynamical orbit evolving from instability of a

    fixed point. The first analytic condition for the onset of pe-

    riod one to period two bifurcation is A 00, where one of the

    roots of the eigenvalue Eq.  4.22  passes through a zero. For

    the development of the period two orbit there must exist one

    real negative root and a pair of conjugate complex roots with

    a negative real part. As the period two develops, it is stable

    as long as all roots are negative or have negative real parts.When any real part becomes positive, the period two orbit

    itself becomes unstable. The calculation of that parameter

    point at which the period two orbit becomes unstable re-

    quires explicit inclusion of the nonlinear terms which is suf-

    ficient to establish the necessary analytic condition  A 00 for

    the onset of period two. The control parameter    or    at the

    1→2 bifurcation point is denoted by   *   or    *   so that   A k *

     Ak ( *) or  A k * A k ( *) and

     A 4* 3 A 3* 

    2 A 2*  A1*0.

    The necessary and sufficient condition that all eigenvalues

    have negative real parts and therefore the bifurcation is

    stable when   A 2* A3* A 1* A 4* . 35 The quantities    0( y 0 , z0)determines the amplitude and phase of the period two orbit

    where  0  is the fixed point of the averaged equation. The two

    conditions for the onset of 1→2 bifurcation are

     A 0 0 0 and

    4.23 0  A 2 0 A 3 0  A 1 0 A 4 0 0

    in the limit   0→0.

    As   0→0 grows there are now four roots to Eq.  4.22.

    The extent of the period two orbit is determined by that value

     0  such that one or more of the roots acquires a positive real

    part, at which point the period two orbit becomes unstable.25

    The coefficients and terms used in this section are explicitlygiven in the Appendix.

    Figures 1 and 2 are the bifurcation diagrams in the two

    parameter regimes of    and   , respectively. In the first one it

    is observed that the period 1→2 bifurcation occurs at the

    point where   0.4325, whereas in the latter it occurs at a

    point where   0.4202. These points along with their cor-

    responding other parameter values were used to calculate

    numerically the coefficients   A1( 0),   A 2( 0),   A 3( 0), and

     A 4( 0). Substituting all these values in Eq. 4.23, it is found

    that   A 00 and   ( 0)0 for both the cases thus satisfying

    our numerical results.

    V. ALGEBRAIC DETECTION OF HOPF BIFURCATION

    The  n-dimensional system of ordinary differential equa-

    tion defined by

     ẋ f  x, ,

    where   x x(t )Rn and   f :   U →Rn is a   C 2-smooth function

    defined on a subset  U Rn which depends upon a vector of 

    parameters,    Rk . The equilibrium point of the system is

     xRn such that   f ( x , )0. As the parameters are varied,

    equilibrium points can undergo bifurcation. There are two

    types of elementary bifurcations that occur in one parameter

    families of systems—saddle nodes and Hopf bifurcations.

    The necessary condition is that the Jacobian evaluated at an

    equilibrium point possesses a simple zero eigenvalue in case

    of former and a pair of pure imaginary eigenvalues in case of 

    latter. For the case of saddle-node bifurcation one can obtain

    the bifurcation locus by augmenting the equation   f ( x, )

    0 with a procedure to calculate equilibrium points where

    the Jacobian has numerical rank ( n1). An inflated system

    for the detection of saddle nodes has been previously done

    using det( D x f ) as the augmenting equation.36

    Here we exam-ine a procedure for locating Hopf bifurcations. For this we

    seek explicit criteria that specify whether a ( nn) matrix

    with coefficients that may depend upon parameters has a pair

    of pure imaginary eigenvalues. For this purpose the desired

    necessary conditions are to be developed.

    Let   J  be the Jacobian matrix for   f   and its characteristic

    polynomial be given by

     p C 0C 1¯C n1n1 n.

     p  has a nonzero root pair  ,  if and only if    is a com-

    mon root of the two equations   p() p() and   p()

     p(). Making the substitution   z2 and rearranging,

    we construct two new polynomials. If  n  is even, then

    r e z C 0C 2 zC 4 z2¯C n2 z

    n2  /2 z n /2,

    5.1r 0 z C 1C 3 zC 5 z

    2¯C n1 z

    n2  /2,

    while for odd  n

    r e z C 0C 2 zC 4 z2¯C n3 z

    n3  /2 z n1  /2,

    5.2r 0 z C 1C 3 zC 5 z

    2¯C n2 z

    n3  /2 z n1  /2.

    Then p  has a nonzero root pair  ,  if there exists a  z  that

    satisfies

    r e z

    r 0 z 0.The two polynomials have a common root if they have a

    common factor. Since the degree of  r 0  is less than or equal to

    r e , we use the Euclidean algorithm.

    We construct a sequence of polynomials,

    P0r e ,   P 1r 0 , P 2 , P 3 , . . . , P k  ,

    such that   P i1   is the remainder of the division of   P i1   by

    P i  . Thus the degrees of  P i   are strictly decreasing and there

    are polynomials  Q i ,   i1,2,...,k   such that

    P i1Q i P iP i1 .

    The Sylvester matrix can be constructed from the coeffi-

    cients of the polynomials. The determinant  RS det(S ) is a

    polynomial in the coefficients of   p   referred to as the

    Sylvester resultant of  r e   and  r 0  share a common root.

    For   i0, 1 let   S i  denote the matrix obtained from  S  by

    deleting the rows 1 and  n /2 and the columns 1 and   i2 for

    even   n. The relationship between the characteristic polyno-

    mial and its corresponding matrices   S ,   S 0 ,   S i   leads to the

    results.

    Theorem 1:  Let  S  be the Sylvester matrix for the poly-

    nomials r e  and  r 0 . Then the jacobian matrix  J  has precisely

    one pair of pure imaginary eigenvalues if 

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    RS 0 and det S 0•det S 1 0.

    If   RS 0 or det(S 0)•det(S 1)0, then   p() has no purely

    imaginary roots.

    Theorem 2:  Let   1 ,   2 , . . . , n  be the roots of the poly-

    nomials   p() and let   S (s i j) be the (n1)(n1)

    Sylvester matrix of the associated pair ( r e , r 0). If 

    m n1  /2

    2   n

    2 ,then

    RS 1 m

    1i jn i j .

    Theorem 3:   For (r e) and ( r 0) defined as above, let

    r 0(C r e)C   if  n  is even and  r e(C r 0)C   if  n  is odd. If RC   is

    used to denote det(C ), then RC RS  .

    To develop a third criterion, we consider the Bezout re-

    sultant. For   n   even the two polynomials specified by Eq.

    5.1  we define the brackets

    i, j det   C 2i   C 2 jC 2i1   C 2 j1 ,   5.3where 0i ,   jn /2 and we take   C n1,   C n10. The Be-

    zout matrix   B  corresponding to the polynomial pair ( r e , r 0)

    is an   n /2-dimensional square symmetric matrix with entries

    constructed as sum of bracket products in the coefficients  C ias follows:

    For 1i jn /2 set

    k minmax 0,i j n21 ,5.4

    k maxi1.

    Then,

     B i j  k k min

    k max

    i jk 1,k  B  ji  .   5.5

    The only modification required is the definition for the case

    of   n-odd is that   C n  has the value prescribed by the charac-

    teristic polynomial   p   and   C n1   is taken to be unity. The

    Sylvester and the Bezout matrix are connected by a relation 37

    which leads to the following theorem:

    Theorem 4:  For the Bezout matrix corresponding to the

    polynomial pair (r e ,r 0) let R B  denote det( B). Then we have

    R B1 nRS  .   5.6

    The coefficients of the linear remainder term from the Eu-

    clidean algorithm can be expressed as determinants of certain

    Bezout submatrices, in analogy to the submatrices defined

    for the Sylvester form. We consider the two submatrices,  B ifor  i0 and 1, obtained by deleting the first column and the

    ith row of  B. We now state another theorem:

    Theorem 5:  Let  B  be the Bezout matrix for the polyno-

    mials r e  and r 0 . Then J  has precisely one pair of pure imagi-

    nary eigenvalues if 

    R B0 and det B 0•det B 1 0.

    If   R B0 or det( B0)•det( B1)0, then   p() has no purely

    imaginary roots.

    For our system  2.3–2.5   if we choose the fixed point

    2.7, the corresponding eigenvalue equation becomes

    3 2  2 2 2

     

       2  2 2

     2 

     2

     2

    2 2

     2 

      0.Therefore Eq.   5.2  can be written as

     p C 0C 1C 223,

    r e zC 0C 2 z ,

    r 0 zC 1 z,

    where  z 2 and

    C 0 2 2  2 

       ,   C 1  2

     2 ,

    C 2 2  2 2

     2 

       .The Sylvester matrix  S  and the two relevant submatrices,  S 0and  S 1 , are given by

    S  C 0   C 2C 1   1

      ,

    Now by Theorem 1,  p  has a pair of purely imaginary roots if 

     Rsdet(S )C 0C 1C 2   vanishes and the product   S 0S 1C 10.

    The Bezout matrix associated with (r e , r 0) is just a

    single element given by

    FIG. 5. Locus of the points satisfying the Hopf bifurcation condition in the

     ,   phase space.

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     B 1,0det C 2   C 01   C 1

    C 2C 1C 0 1 3 C 0C 1C 2 R s .

    The Bezout subresultant condition provided by the expres-

    sion, det( B0)det( B1)C 1   is necessarily positive when  p  has a

    pair of imaginary conjugate roots. In our case   C 1( 2 2 /  2)( 2 /  2)) is always positive. Therefore   C 0C 1C 20 is the only condition for a pair of purely imagi-

    nary conjugate roots. Figures 5 and 6 represents the curve of 

    Hopf bifurcation for     versus      and     versus    , respec-

    tively. Each point on the two curves represents a Hopf bifur-

    cation point. Tables I and II provide the eigenvalues for some

    points of Figs. 5 and 6, respectively.

    Thus we have a method of computing the singularity

    condition necessary to establish that the Jacobian of the dy-

    namical system   2.3–2.5  has a pair of purely imaginary

    eigenvalues, which is the condition for the Hopf bifurcation.

    VI. CONTROL OF CHAOS BY ADAPTIVESTABILIZATION

    In this section the task of controlling chaos is consid-

    ered. The aspect of controlling chaos in a semiconductor

    laser system is important due to its possible applications in

    synchronization, communication, and data transfer. Different

    control techniques have been developed so far,38,39 most of 

    which require the system parameters to be known exactly.

    This requirement makes the practical application of such

    control procedures difficult. So we have discussed a new

    control strategy using invariant manifold theory which can

    deal with systems where the parameter values are unknown.

    This makes the procedure feasible to experimental setup. The

    essential requirement is that the steady or equilibrium state

    of the system is to be known and so this procedure is imple-

    mentable to fixed points and not to periodic solutions. The

    amplitude of perturbation given to the dynamical system in

    the form of three control inputs is determined by the method

    itself.

    To stabilize the system we introduce three control inputs

    in the system  2.3–2.5  as follows:

    dx 1

    dt     x1 x 3

     

    2 x 2 x 3  x2u 1 ,   6.1

    dx 2

    dt  

      x 1

     

    2  x1 x3

    1

    2 x 2 x3

    u 2 ,   6.2

    dx 3

    dt   2 x3 12  x3  x1

    2 x 2

    21 u 3 .   6.3

    Now we consider the fixed point   2.6   of the system. To

    avoid the numerical complications we choose   0.7. There-

    fore the fixed point  2.6  becomes

    a a 1 ,a 2 ,a 3T  6.4

     a 1

    1.4 p

     p 2 2   p 2

    a 21.4   p2 

     p 2 2   p 2

    a 3 p  .   6.5

    The three manifolds given below are selected as invariant

    manifolds:

     M 1 xR3 x 1a 10,   6.6

     M 2 xR3 x 2a 20,   6.7

     M 3 xR3 x 3a 30.   6.8

    Therefore the system is also stable on the intersection of 

    these manifolds, M c M 1 M 2 M 3

     xR3 x 1a 10, x2a 20, x 3a30.   6.9

    Our motivation is to design a control which drives the sys-

    tem trajectories along these three manifolds to the set  M c .

    Then by Lasalle’s invariant set principle40 we can con-

    clude that   x   will converge to the equilibrium   a  asymptoti-

    cally, where   a   is the only stable equilibrium of the set   M c .

    To design such a stabilizing controller we construct a

    Lyapunov function as follows:

    V  x 12 

    T  x T   x ,   6.10

    FIG. 6. Locus of the points satisfying the Hopf bifurcation condition in the

     ,    phase space.

    TABLE I.    1.0.

            Eigenvalues obtained

    0.2 0.19183 0.10870 0.2, 5.81090.9798i

    0.25 0.23386 0.14286 0.25, 5.961080.96824i

    0.31 0.27862 0.19188 0.31, 2.3031080.95073i

    0.44 0.34444 0.35901 0.44, 1.078081080.89799i

    0.56 0.341921 0.75107 0.56, 5.5321090.82840i

    TABLE II.    1.5.

        Eigenvalues obtained

    3.0 0.35355 0.5 0.5, 2.42881070.86602i

    4.0 0.31792 0.26087 0.375, 2.1231060.92702i

    5.2 0.26337 0.17303 0.28846, 2.3031080.95073i

    6.3 0.22419 0.13427 0.23810, 2.81060.97124i

    7.9 0.18290 0.10231 0.18987, 1.14241070.98181i

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    where    T ( x)  1( x)  2( x)  3( x) x 1a 1 x 2a 2 x 3a3 ,   T R

    33 is a positively definite matrix. Now we

    want the following differential equations holds so that the

    controller can be designed

    T  ˙  x   x 0.   6.11

    Therefore the time derivative of  V ( x) becomes

    V ˙  x  T  x   x .   6.12

    This implies that  V ˙ ( x)0 for all   x M c  , meaning the sys-

    tem trajectory can be driven to   M c   asymptotically. To find

    such a controller, the system Eqs.  2.3–2.5  into Eq. 6.11

    gives

    u u 1u2u3   0.7 x1 x 3

     

    2 x 2 x3  x 2

      x 1 

    2 x1 x 3

    1

    2 x 2 x3

    2 x 3 12  x 3 x 12 x 2

    21

    T 1 x 1a 1 x 2a 2

     x 3a 3 .   6.13

    If the parameters   ,   ,    are unknown, the controller  6.13

    should be able to realize the stabilization. However the con-

    troller 6.13   is not implementable because parameters   ,   ,

      are assumed to be unknown. This problem cannot be

    solved via the conventional adaptive control theory, because

    the basic assumption of the adaptive control is that the equi-

    librium is fixed and unknown. Here we shall develop a tai-

    lored adaptive control for our system in the following. Be-

    cause the parameters    ,    ,     are unknown, we use themodified three invariant manifolds   M 1 ,   M 2 ,   M 3  which are

    defined, respectively, as    ˆ 1( x) x 1â 1 ,    ˆ 

    2( x) x2â 2 ,

     ˆ 3( x) x3â 3 , where   â 1 ,   â 2 ,   â 3  are given by

    â 11.4 p̂ 

     p̂ 2 2 ˆ  ˆ  p̂ 2 ,   6.14

    â 21.4  ˆ  p̂ 2 

     p̂ 2 2 ˆ  ˆ  p̂ 2 ,   6.15

    â 3 p̂ ,   6.16

    where  p  is real satisfies the relation

     p̂ 2  ˆ  21 4 p̂  ˆ   ˆ 0.98̂4 ˆ  20.490.   6.17

    For a adaptive control design we construct the following

    parameter-estimate-dependence Lyapunov function:

    V  x, ˆ  , ˆ  , ̂12 

    ˆ  T  x T  ˆ  x eT P1e,   6.18

    where   e  ˆ  with        T  and    ˆ   ˆ   ˆ   ̂ T ,    ˆ  T ( x)

     ˆ 1  ˆ 

    2  ˆ 

    3   and  PR33 is a positive definite matrix. Let

    us denote

     f  x   0.7 x1 x 3

    2

     x2 x 3

    2

     x12 x 2

    21

     ,

    F  x   x 2 x 3

    2  x2   0

     x 1 x3

    2 x 1   0

    0 0   2 x 3 x12 x 2

    21  ,

    and

    g x  1 0 0

    0 1 0

    0 0 1 .

    Then the time derivative of the Lyapunov function is given

    by

    V ˙  x, ˆ  , ˆ  , ̂ ˆ  T T   ˆ 

      x  f  x F  x  g x u

     ˆ  T T   ˆ 

      ˆ    ˆ ˙e T P1 ˆ ̇

     ˆ  T T   ˆ 

      x  f  x F  x  ˆ g x u

     ˆ  T T   ˆ 

      x  F  x e ˆ  T T 

      ˆ 

      ˆ    ˆ ˙e T P1 ˆ ̇.

    Let  u  consists of two parts, i.e.,  uueu c . Also let

      ˆ 

      x  f  x F  x  ˆ g x u eT 

    1 ˆ ,   6.19

     ˆ  T T   ˆ 

      x g x uc 

    ˆ  T T   ˆ 

      ˆ    ˆ ˙ ,   6.20

     ˆ  T T   ˆ 

      x F  x eeT P1 ˆ ̇.   6.21

    Then

    V ˙ ˆ  T  ˆ 0

    for all   x  such that    0, so the stability of the system state

    with respect to the invariant manifolds    ˆ 10,    ˆ 

    20, and

     ˆ 30 is realized. From   6.19–6.21  we obtain

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    u e u e1ue2ue3

      0.7 x1 x3 ˆ 

    2 x 2 x3 ˆ x 2

     ˆ x 1 ˆ 

    2 x 1 x3

    1

    2 x 2 x3

    2̂ x 3 12̂ x 3 x 12 x 2

    21

    T 1

     x 1â 1 x

    2

    â 2

     x 3â 3  6.22

    and

    u c u c1uc2uc3

        ˆ 1

      ˆ 

      ˆ 1

     ˆ 

      ˆ 1

     ̂

      ˆ 2

      ˆ 

      ˆ 2

     ˆ 

      ˆ 2

     ̂

      ˆ 3

      ˆ 

      ˆ 3

     ˆ 

      ˆ 3

     ̂

    P

      x 2 x32

     x 2   0

     x1 x3

    2 x1   0

    0 0   2 x 3 x 12 x2

    2

    T  x 1â

     1

     x2â 2 x3â 3

      6.23and the update law for parameter estimation

     ˆ ̇   ˆ ̇

     ˆ ˙

    ̂̇ P  ˆ 

      x F  x

     T 

    T  ˆ 

    P  x 2 x3

    2 x 2   0

     x1 x 3

    2 x1   0

    0 0   2 x 3 x 12 x2

    2

     x 1â 1 x2â 2

     x3â 3

     .   6.24

    For our system we consider the parameter values as   2.0,

     0.69,  0.005. Also constant matrices were set to be

    T  1 0 0

    0 1.43 0

    0 0 0.5 ,   P

     1 0 0

    0 1.05 0

    0 0 0.25 .

    The initial conditions were   x(0)(0.5,0.5,1.0)T  and

    ( ˆ 0 , ˆ  0 ,̂0)(2.5,0.7,0.01). Using Eqs.   5.22–5.23   and

    then integrating the system  6.1–6.3  along with  6.24  we

    get a controlled scenario from a chaotic state. The time evo-

    lution of the variables are shown in Fig. 7 which depicts their

    convergence to a steady state.

    VII. CONCLUSION

    Properties of single mode optically injected semiconduc-

    tor lasers are very much important from various experimen-

    tal points of view. In this paper, we have made a detailed

    simulation study of its chaotic aspects, the various mecha-

    nism of onset of chaos—period doubling bifurcation and

    Hopf bifurcation and have given a complete characterization

    of the attractor with an eye to the availability of a single time

    series from experimental data. Our results are checked in a

    dual way—both analytically and numerically. Finally a new

    method has been applied to ascertain the controlling property

    of the chaotic scenario. The construction of a control mecha-nism is nowadays a well researched and formulated topic.

    Already there exist a few authentic monographs on the sub-

     ject and all of them actually start from the ansatz of a suit-

    able Lyapunov function. The net effect and the conditions

    therein, for the influence on the phase space, are classified in

    stages. We have not attempted to deal with this ourselves, but

    refer to the literature.43

    ACKNOWLEDGMENTS

    One of the authors   P.S.   is grateful to the CSIR   Gov-

    ernment of India, for the senior research fellowship, and the

    work of A.R.C. is partially supported by a research project

    FIG. 7. Time variation of the system variables on the application of adaptive

    stabilization which shows convergence to a steady value.

    356 Chaos, Vol. 14, No. 2, 2004 Banerjee, Saha, and Chowdhury

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    12/12

    sponsored by the CSIR. The authors are also thankful to the

    anonymous reviewers for their valuable suggestions.

    APPENDIX: COEFFICIENTS  f ij  ,  d ij  ,  e ij 

     f 11C 0

    2

    2  ,    f 12

    C 03

    2  ,

     f 21

    C 03

    2  ,    f 22

    C 02

    2   ,

    d 11 k 23 k 11 C 0

    k 11m 1

      

    k 21m 2

       c 11 ,

    d 12 k 24 k 12 C 0

    k 12m 1

      

    k 22m 2

       c 12 ,

    d 21 k 13 k 21 C 0

    k 11m 3

      

    k 22m 4

       c 21 ,

    d 22 k 14 k 22 C 0

    k 12m 3

      

    k 22m 4

       c 22 ,

    e 11k 13C 0

    k 13

       m 1

    k 23

       m 2c 13 ,

    e 12k 14C 0

    k 14

       m 1

    k 24

       m 2c 14 ,

    e 21k 23C 0

    k 13

       m 3

    k 23

       m 4c 23 ,

    e 22k 24C 0

    k 14

       m 3

    k 24

       m 3c 24 .

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