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    An Invariance Principle in the Theory

    of Stability

    JOSEPH P.LASALLE

    THE stabili ty theorems of Lyapunov have been among

    the oldest and strongest pi llars

    of

    control theory. The cen

    tenary

    of

    Lyapunov's celebrated 1892 memoir was recently

    marked with its English translation [17], while the 1907 French

    translation was reprinted in 1949 by Princeton University

    Press [16].

    Applications

    of

    Lyapunov stability concepts to control prob

    lems began to appear in Russia in the 1930s-1940s. Significant

    theoreticalresults from the 1950s were summarizedin the books

    by Chetayev [3], Lurie [15], Malkin [18], Letov [14], Zubov

    [22], and Krasovskii [7]. In the post-1957 Sputnik era, English

    translations of these books, and

    of

    other Russian works, further

    increasedthe interest already stimulated by Contributions to the

    Theory of Nonlinear Oscillations, a five volume series (1950,

    1952, 1956, 1958, and 1960) edited by Lefschetz, and published

    by Princeton University Press. The fourth volume contained a

    detailed and rigorous survey of Lyapunov stability theory by

    Antosiewicz [1]. The 1960 survey by Kalman and Bertram [6]

    was more accessible and had a stronger impact on engineering

    audiences, as did the books by Lefschetz [12], Lefschetz and

    LaSalle [13], and a paper by LaSalle [10]. This activity contin

    ued in the early 1960s when several volumes of Contributions

    to Differential Equations were published, including the impor

    tant results by Yoshizawa [20], whose 1966 book [21] presented

    a collection of advanced stability results. The status of stability

    theory in the pre-1965 per iod is summarized in the scholarly

    work by Hahn [4], which is the most comprehens ive source

    covering that period.

    Among the innovations from that period are the results which

    settle the issue of existence of Lyapunov functions. Particularly

    important among the results

    of

    this type are the converse theo

    rems of Massera [19], Krasovskii [14] and Kurzweil [8], which

    found applications in diverse areas of control theory. Radially

    unbounded Lyapunov functions were introduced in 1952 by

    Barbashin and Krasovskii [2] to guarantee stability in the large,

    that is, global stability. The same Barbashin-Krasovskii paper

    and the bookby Krasovskii [14] initiatedanother line of research

    which culminatedin this paper byLaSalle, and its extended 1968

    version [11].

    This line

    of

    research was aimed at extracting from Lyapunov's

    stability theorem more information about the asymptotic behav

    ior

    of

    the solutions

    x t)

    E IR

    n

    of

    x

    =

    f x t) , f O, t)

    =

    0 for all

    t

    (1)

    With a positive definite function Vex, t) , a theorem of Lya

    punov establishes asymptotic stability of the equilibrium x = 0,

    if V  x, t) is negative definite along the solutions

    x t)

    of (1). IfV

    is only nonpositive, the same theorem guarantees stability, but

    does not reveal whether

    x t)

    converges to zero or to a set in IR

    n

    .

    For autonomous systems,

    x

    =

    f x),

    a theorem ofBarbashin and

    Krasovskii [2] (see also Theorem 14.1

    onp.

    67 of[14]) examines

    the set

    E

    in which V =

    O

    If this set does not contain any positive

    semi-trajectory (solution

    x t)

    for all t ::: 0) other than

    x t) ==

    0,

    then x   t) --- 0 as t ---

    00.

    This result gave a practical test for

    asymptotic stability when

    V

    is only nonpositive, instead of neg

    ative definite. In his 1960 paper [10], LaSalle extracted further

    information on the asymptotic behavior of x t). Using the limit

    sets and the largest invariant set

    M

    of x = f (x) contained in the

    set E where V is zero, he showed that

    x t)

    converges to the set

    M.

    This set need not be an equil ibr ium, but can be a compact

    limit set like a limit cycle.

    This result of LaSalle, which he later termed

    I

    nvariance

    Prin

    ciple, had a significant connection with the then new concept

    of

    observability. For the system x = Ax, a positive definite

    Lyapunov function V =

    x

    P

    x

    has the derivative

    V

    = A P +

    PA =

    -x Qx.

    Suppose that

    Q

    is positive semi-definite, so that

    it can be expressed as Q = C'C for some matrix C. It then fol

    lows that

    V

    = -

    y

    y, where y

    =

    Cx can be treated as an output

    ofx =Ax. Clearly, the set E where

    V

    = 0 is y t)

    ==

    O If the pair

      A, C) is completelyobservable, then y t) == 0 implies x t) = O

    Hence, no nonzero positive semi-trajectory

    x t)

    is contained in

    E, which proves, via Barbashin-Krasovskii [2], that x =

    Ax

    is asymptotically stable. However, if the system is only stable

    with a pair of purely imaginary eigenvalues unobservable from

    y

    = Cx, then LaSalle's Principle shows that x t) converges to

    the periodic solution in the unobservable subspace.

    The Invariance Principle was subsequently extended to peri

    odic and almost periodic systems, but it does not hold for more

    309

  • 8/20/2019 An Invariance Principle in the Theory of Stability

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    general nonautonomous systems (1). Toobtain similar informa

    tion on the asymptotic behavior of x t), Yoshizawa [20] derived

    a set of conditions under which

    V

      x, t)  :s

    W   x) ,

    where

    W   x)

    is

     positive definite with respect to a set M, implies that x t) con

    verges to M. The main theorem in this paper by LaSalle mod

    ifies and improves this result of Yoshizawa, and provides the

    strongest convergence result for nonautonomous systems. Togo

    beyondthis result, further restrictions on f   x, t) are needed. One

    of them is the so-called persistency of excitation condition in

    adaptive identification and control. Typically, an adaptive algo

    rithm guarantees that V  :s -e

    2

    , where e is the scalar tracking

    error. The Yoshizawa-LaSalle theorem provides the conditions

    under which e(t) converges to zero. It has thus become an in

    dispensable tool in adaptive control design. It has also become

    instrumental in deducing stability from passivity properties as

    in feedback passivation and backstepping designs of nonlinear

    systems.

    Other settings where LaSalle's

    Invariance Principle

    has been

    studied are infinite dimensional systems, as in the work of

    Hale [5], and stochastic systems governed by continuous-time

    Markov processes, as discussed by Kushner in [9].

    REFERENCES

    [1]

    H. ANTOSIEWICZ,  A survey of Lyapunov's second method, in

    Contr.

    to Nonlinear Oscillations, S. Lefschetz, Ed., 4:141-166 (Princeton Univ.

    Press, Princeton NJ), 1958.

    [2] E.A. BARBASHIN AND N.N. KRASOVSKII,  On the stabilityof motion in the

    large,

    Dokl.Akad. Nauk USSR,

    86:453-456,1952.

    [3] N.G. CHETAYEV,

    TheStability

    of

    Motion

    , PergamonPress (Oxford), 1961.

    (Russian original, 1946.)

    [4] W.

    HAHN,

    Stability

    of

    Motion

    (Springer-Verlag, New York), 1967.

    [5] J.K. HALE,  Dynamical systemsand stability, J.

    Math.Anal. Appl., 26:39

    59,1969.

    [6] R.E. KALMAN

    AND

    J.E.

    BERTRAM,

     Control system analysis and design

    via the 'secondmethod' of Lyapunov, I Continuous-time systems, 1.Basic

    Engineering (Trans.ASME), 82D:371-393, 1960.

    [7] N.N. KRASOVSKII,

    Stability

    of

    Motion

    ,StanfordUniv. Press (Stanford,CA),

    1963. (Russian original, 1959.)

    [8] J.

    KURZWEIL,  The

    converse second Liapunov's theorem concerning the

    stability of motion, Czechoslovak Math.

    1.,6(81):217-259

    &

    455-473,

    1956.

    [9] H,J.

    KUSHNER,

     Stochastic stability, in Stability of StochasticDynamical

    Systems,R. Curtain, Ed., Lect. Notes inMath., Springer-Verlag (New York),

    294:97-124,1972.

    [10] J.P.

    LASALLE,

     Some extensions ofLiapunov's secondmethod, IRETrans.

    Circuit Theory,

    CT·7:52G-527, 1960.

    [11] J.P.LASALLE,  Stability theory for ordinary differential equations,

    1.

    Dif

    ferential Equations,

    4:57-65,1968.

    [12] S. LEFSCHETZ,

    Differential Equations: Geometric Theory,

    Interscience,

    Wiley (New York), 1957.

    [13] S.

    LEFSCHETZ

    AND

    J.P. LASALLE,

    Stability by Liapunov s Direct Method,

    with Applications,Academic Press (New York), 1961.

    [14] A.M.

    LETOV,

    Stability inNonlinear ControlSystems (English translation),

    PrincetonUniv. Press (Princeton, NJ), 1961. (Russian original, 1955.)

    [15] A.E. LURIE,

    SomeNon-linearProblemsin theTheory

    of

    AutomaticControl

    (English translation), H.M.S.O., London, 1957. (Russian original, 1951.)

    [16] A.M. LY

    APUNOV,

     Probleme general de la stabilite du mouvement (in

    French),

    Ann.Fac.Sci. Toulouse,

    9:203-474, 1907.Reprinted

    inAnn. Math.

    Study,

    No.

    17,1949,

    Princeton Univ. Press (Princeton, NJ).

    [17] A.M. LYAPUNOV,  The general problem of the stability of motion (trans

    lated into English by A.T. Fuller),

    Int.

    J.

    Control,

    55:531-773,1992.

    [18] I.G. MALKIN,

    Theory

    of

    Stability

    of

    Motion

    ,AEC (AtomicEnergy Commis

    sion) Translation 3352, Dept. of Commerce, United States, 1958. (Russian

    original, 1952.)

    [19] J.L.MASSERA , Contributionsto stability theory, Ann.Math.,64:182-206,

    1956.

    [20] T. YOSHIZAWA,  Asymptotic behavior of solutions of a system of differ

    ential equations, in

    Contributions to Differential Equations, 1:371-387,

    1963.

    [21] T.YOSHIZAWA, StabilityTheory byLiapunov s SecondMethod, The Math

    ematical Society of Japan, Publication No.9 (Tokyo), 1966.

    [22] V.1. ZUBOV, Mathematical Methods for the Study of Automatic Control

    Systems,

    Pergamon Press (Oxford), 1962. (Russian original, 1957.)

    P.V.K.

     

    J.B.

    3

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    An

    Invariance Principle in the

    Theory

    of Stability

    JOSEPH P. LASALLEl

    Center for Dynamical Systems

    Brown University, Providence, Rhode Island

    1.

    Introduction

    The purpose of this paper is to give a unified

    presentation of Liapunov's

    theory

    of

    stability

    that

    includes

    the

    classical Liapunov

    theorems

    on

    stability

    and instability as well as

    their

    more recent extensions. The idea being ex

    ploited here had its

    beginnings

    some time ago. It was, however, the use made

    of this

    idea by Yoshizawa in [7J in his

    study of

    nonautonomous differential

    equations and by Hale in [1]in his study of autonomous functional-differen

    tial equations that caused the

    author

    to return to this subject and to adopt

    the general approach and point of view

    of

    this

    paper.

    This

    produces some

    new

    results fo r

    dynamical

    systems defined

    by

    ordinary differential equations

    which demonstrate the essential nature of a Liapunov function and which

    may be useful in applications.

    Of

    greater

    importance,

    however, is the possi

    bility,

    as

    already indicated by

    Hale's results for

    functional-differential

    equa

    tions, that these ideas can be

    extended

    to more general classes

    of

    dynamical

    systems. It is hoped, for instance, that it may be possible to

    do

    this for some

    special types

    of

    dynamical

    systems defined by

    partial

    differential equations.

    In Section 2 we present some basic results for ordinary differential equa

    tions. Theorem I is a

    fundamental

    stability theorem for nonautonomous

    systems and is a modified version

    of Yoshizawa's

    Theorem 6 in [7]. A simple

    example

    shows that

    the conclusion of

    this theorem is the best possible.

    However, whenever

    the

    limit sets

    of solutions

    are

    known

    to have an invar

     

    iance

    property,

    then

    sharper

    results

    can

    be

    obtained. This invar iance

    principle explains

    the

    title

    of

    this paper.

    It

    had its origin for autonomous

    and periodic systems in [2]

    and

    [4],. although we present here improved ver

    sions

    of those results. Miller in [5] has estab li shed an invariance property

    1

    This

    research was supported in

    part

    by the National Aeronautics

    and

    Space Adrnini  

    stration under

    Grant No.

    NGR-40-002-015

    and under Contrac t No. NAS8-11264, in part

    by

    the

    United States Air Force through the Air Force Office of Scientific Research under

    Grant

    No.

    AF-AFOSR-693-65, and in part by the United Sta tes Army Research Office,

    Durham,

    under Contract

    No.

    DA-31-124-ARO-D-270.

    Reprinted

    with permission from Differential Equations and Dynamical Systems

    (New

    York: Academic Press, 1967),1. Hale and 1.P.LaSalle, eds.,

    Joseph

    LaSalle,

     An

    Invariance Principle in the

    Theory

    of Stability, pp. 277-286.

    311

  • 8/20/2019 An Invariance Principle in the Theory of Stability

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    for almost periodic systems

    and obtains

    thereby a similar stability

    theorem

    for almost periodic systems. Since little attention has been paid to theorems

    which make possible estimates of regions of attraction (regions of asymptot

    ic stability) for nonautonomous systems results of this type are included.

    Section 3 is devoted to a brief discussion of some

    of

    Hale's recent results [I]

    for

    autonomous

    functional-differential equations.

    2.

    Ordinary

    Differential

    Equations

    Consider

    the

    system

    i =f(t,

    x) (1)

    where x is an n-vector,fis a continuous function on Rn,+l to

    R

    and satisfies

    anyone

    of

    the

    conditions

    guaranteeing

    uniqueness

    of

    solutions.

    Fo r each x

    in Rn, we define I x I

    == (Xl

    +

    ... + X

    n

    2 )1 I2 ,

    and

    for E a closed set in Rn

    we define d(x, E) =

    Min

    { Ix - y I; y in E}. Since we do

    no t

    wish to

    confine ourselves to bounded solutions, we introduce the point

    at

    CX

    and

    defined(x,

    00) ==

    IX 1-1. Thus, when wewrite E* == E U

    {oo},

    we shall mean

    d(x, E*) =

    Min

    {d(x, E), d(x,

    oo)}. If x t) is a solution of (1), we say

    that

    x t)

    approaches

    E

    as t

     

    0 0 ,

    if

    d x t), E) --.0 as

    t

    - ) 0 0 0 0 .

    If

    we

    can

    find such

    a set E, we have obtained information

    about

    the asymptotic behavior of

    x t)

    as

    t

     

    CXJ.

    The

    best

    that

    we

    could hope

    to

    do

    is to find the smal lest

    closed set

     J

    that x(t) approaches as t

     

    0 0 . This set Q is called the positive

    limit set of x(t)

    and

    the points

    p

    in Q are called the

    positive

    limit points

    of

    x t). In exactly the same way, one defines

    x t)

      E as t --+- - 0 0 , negative

    limit sets,

    and

    negative l imit points. This is exact ly Birkhoff's concept of

    limit sets. A

    point

    p is a positive limit

    point of x t), if and

    only

    if there

    is a

    sequence of times t

    n

    approaching

    CX ) as n   0 0

    and

    such

    that x t

    n

    ) - p as

    n ----.

    CXJ. In

    the

    above, it may be

    t ha t the

    maximal interval

    of

    definition of

    x t)

    is [0, r ),

    This

    causes no difficulty since, in

    the

    resul ts to be presented

    here, we need only, with respect to t ime

    t,

    replace

    00

    by

    T.

    We usually ignore

    this possibility

    and speak

    as

    though ou r

    solutions

    are

    defined on [0,  X or

      0 0 ,

    (0).

    Let

    V(t,

    x)

    be

    a Cl function on [0,

    oo ]

    x

    R

    to

    R,

    and

    let G be

    any

    set

    in R .

    We shall say

    that V

    is a

    Liapunov function

    on G for Eq. (1),

    if V(t, x)

      0

    and

    V(t, x)   -

    W x)

      0 for all t > 0

    and

    all x in G, where W is

    continuous

    on

    Rn

    to

    R, and

    . av

    n

    av

     r i:

    +  

    ;lfi·

    U i I ox;

    312

    (2)

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    We define (G is the closure

    of

    G)

    E = {x; W(x) ==

    0,

    x

    in

    G}.

    The following result is

    then

    a modified but closely related version of

    Yoshizawa's Theorem 6 in [7].

    Theorem 1. If V is a Liapunov function on G for Eq. (I), then each

    solution x(t)

    of (1) that remains in G for all

    t > to

      0 approaches

    E*

    =

    E u {oo} as

    t   oo,

    provided one

    of the

    following conditions is

    satisfied:

    (i) Fo r each pinG the re is a

    neighborhood N of

    p such that

    If t,

    x)

    I

    is bounded

    fo r

    all t

    >

    0 and all

    x

    in

    N.

    (ii)

    W is Cl and W is bounded from above

    or

    below

    along

    each

    solu

    t ion which remains in

    G

    for all t > to   o

    If

    E

    is bounded,

    then each

    solution

    of

    (1)

    that

    remains in

    G

    for

    t >

    to

     

    0

    either

    approaches E or

    0 0

    as

    t

      0 0 .

    Thus

    this

    theorem explains precisely the nature

    of

    the

    information

    given

    by a Liapunov funct ion. A Liapunov functi on relative to a set G defines a

    set E, which under

    the conditions

    of

    the

    theorem

    contains

    (locates) all

    the

    positive limit sets of

    solutions

    which for positive time remain in G.The prob

    lem in applying

    the

    result is to find good Liapunov functions. For in

    stance, the

    zero function

    V

    =

    0 is a Liapunov

    function

    for the whole space

    Rn

    and

    condition (ii) is satisfied bu t gives no

    information

    since

    E = R .

    It is trivial

    bu t

    useful for applications to note that if VI

    and

    V

    2

    are Liapunov

    functions on G, then

    V

    = VI

    + V

    2

    is

    also

    a

    Liapunov

    function

    and

    E = £1   £2 .

    If

    E is smaller than

    either

    £1 or £2' then V is a  better

    Liapunov function

    than either

    E.

    or £2 and is always at least as   good

    as e ither of the two.

    Condition

    (i )

    of

    Theorem 1 is essentially

    the

    one used by Yoshizawa.

    We

    now

    look at a simple example,

    where condition (ii)

    is satisfied and

    condi

    tion

    (i)

    is not.

    The

    example also shows

    that

    the conclusion

    of

    the theorem is

    the best possible. Consider

    x

    + p t) i + x = :: 0, where p(t)   (j > o Define

    2V

    = x

    2

    + y2,

    where

    Y ==

     

    i . Then

    V

    ===

    - p t)y2   -

    b

    y

    2

    and

    V

    is a Lia

    punov function

    on

    R2. Now

    W ===

    l5y2

    and W ==

    2t5YJi

    === -

    2c5 xy

    +

    p(t)y

    2

    )

      - 2f5xy. Since all solut ions are evident ly bounded for all

    t

    > 0,

    condi

    tion (ii) is satisfied. Here E is the x-axis (y:=:

    0 ) and

    for each

    solution

    x t),

    yet) =

    X(/) --+- 0 as

    t   0 0 .

    Noting that

    the equat ion

    .t (2

    +

    exp[t))

    x

    + x == 0 has a solution x t) = 1

    .t-

    exp( - t) , we see that this is the best

    possible result without further restrictions on p.

    313

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    In

    order

    to use

    Theorem

    1, there

    must

    be some means

    of

    determining

    which solut ions remain in G.

    The

    following corollary, which is an obvious

    consequence of

    Theorem

    1, gives one way of

    doing

    this

    and

    also provides,

    for

    nonautonomous

    systems, a

    method

    for estimating regions

    of

    attraction.

    Corollary 1.

    Assume

    that

    there exist

    continuous

    functions

    u x) and

    II(X) on Rn

    to

    R

    such

    that u x)

     

    V(t,

    x)  

    v x)

    for all

    t  

    O. Define

    Q,/+ = {x; u x) < 1J}

    and

    let

    G+

    be a

    component

    of Q 1+.

    Let G denote

    the

    component

    of

    Q 7

    =

    {x ;

    v(x) <

     YJ}

    containing

    G+.

    If V

    is a

    Liapunov

    function

    on

    G for (1)

    and

    the

    conditions

    of Theorem 1

    are satisfied,

    then

    each solution

    of

    (1) s ta rt ing in

    G+

    at any time

    to

     

    0

    remains in

    G for

    all t > to

    and

    approaches

    E*

    as

    t  

    0 0 . If G is

    bounded and

    EO =

    E

     

    G

    C

    G+, then

    EO is an

    attractor and G+

    is in its region of at

    traction.

    In general we

    know

    that

    if

    x t)

    is a solut ion

    of   I ) - i n

    fact,

    if x t)

    is any

    continuous

    function on R to Rtl-then its posit ive l imit set is closed

    and

    connected. If x t) is

    bounded,

    then its positive limit set iscompact. There are,

    however, special classes of differential

    equations

    where

    the

    limit sets of solu

    t ions have an addit ional invariance property which makes possible a refi

    nement

    of

    Theorem

    1. The first of these are the autonomous systems

    x

    =f(x).

    (3)

    The

    limit sets

    of

    solutions

    of

    (3) are invariant sets.

    If

    x t)

    is defined on [0, 00)

    and

    ifp is a positive limit

    point

    of

    x{t),

    then

    points on the

    solution

    through

    p

    on

    its

    maximal interval of definition are positive limit points

    of x t).

    If

    x t)

    is

    bounded

    for

    t >

    0, then it is defined on [0,

    00),

    its positive limit set

    Q

    is

    compact,

    nonempty

    and

    solutions

    through points p of

    Q

    are defined on

     -00, 00)

    (i.e.,

    (J

    is invariant). If the maximal

    domain

    of definition

    of

    x t) for t

    > 0 is finite, then x t) has no finite posit ive limit

    points: That

    is,

    if

    the maximal interval of definition of x t) for t

    >

    0 is [0,

    fJ),

    then

    x t)

    --+ 0 0

    as

    t

     

    fJ

    As we have said before, we will always

    speak

    as

    though our

    so

    lutions

    are

    defined on

     -0 0 , 0 0 )

    and

    it

    should

    be remembered

    that

    finite

    escape time is always a possibility unless there is, as for example in

    Corol

    lary 2

    below,

    some condition

    that

    rules it

    out.

    In Corol la ry 3 below,

    the

    solutions

    might

    welt go to infinity in finite time.

    The invariance property of the limit sets of solutions of

    autonomous

    systems (3)

    now

    enables us to refine

    Theorem I.

    Let V be a

    Cl

    function

    on

    R

    to

    R. If G

    is

    any

    arbit rary set in

    R ,

    we say

    that V

    is a

    Liapunou

    function on G

    for

    Eq. (3)

    if V

    = :

    (grad

    V) • f

    does

    not

    change sign on G.

    Define E = {x; V(x) = 0, x in G}, where G is

    the

    closure of G. Let M be

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    the largest invariant set in E. M will be a closed set.

    The

    fundamental sta

    bility theorem for

    autonomous

    systems is then the following:

    Theorem 2. If V is a Liapunov function on G for (3), then each so

    lution

    x t)

    of (3) that remains in G for all

    I

    > 0

    (I

    < 0) approaches

    M* = M

    u

    {oo} as t -- . 0 0 (I -- +

    - 0 0 ) .

    If M

    is

    bounded, then e ithe r

    x t)

     

    M or x t)   0 0

    as

    1---.

    0 0

    (I

    -- +

    - 0 0 ) .

    This one theorem contains all of

    the

    usual Liapunov like theorems on

    stability

    and

    instability

    of autonomous

    systems. Here, however, there

    are

    no conditions of definiteness for

    V

    or V,

    and

    it is often possible to obtain

    stability

    information about

    a sys tem with these

    more

    general types

    of

    Lia

    pUDOV functions.

    The

    first corol la ry below is a stabil ity resul t which for

    applications

    has

    been quite useful, and the second illustrates how

    one

    obtains

    information on instability. Cetaev's instability

    theorem

    is similarly

    an

    im

    mediate consequence of

    Theorem

    2 (see Section 3).

    Corollary

    2. Let G be a

    component

    of

    Q

    =

    {x ; V(x)

    <

    1]}.

    Assume

    that G

    is

    bounded,

    V;;£ 0

    on G, and MO = M n

    G

    c:

    G.

    Then

    MO is an

    attractor

    and

    G is in its region of attraction. If, in addition, V is constant

    on

    the boundary of

    MO ,

    then MO is a stable attractor.

    Note

    that if

    MO

    consists of a single

    point p, then p

    is asymptotically stable

    and

    G prov ides an est imate of its region of asymptotic stability.

    Corollary 3. Assume

    that

    relative to (3)

    that

    V V> 0 on G

    and

    on

    the boundary

    of G

    that V

    = O. Then each solution

    of

    (3) s tart ing in G a p

    proaches 0 0 as t   0 0

    (or

    possibly in finite time).

    There are

    also some special classes of

    nonautonomous

    systems where the

    limit sets of solut ions have an invariance property.

    The

    simplest

    of

    these

    are

    periodic systems (see [2])

    x =  ((t, x) , f(1

    + T, x =

    .f(t)

    for all

    t

    and

    .r. (4)

    Here, in

    order

    to avoid introducing the concept

    of

    a periodic

    approach

    of a

    solution of (4) to a set

    and

    the concept of a periodic limit point, let us con

    fine ourselves to solutions

    x t) of

    (4) which are bounded for t > O Let J be

    the

    positive limit set

    of

    such a

    solution x t), and

    let p be a

    point

    in

    Q.

    Then there is a solut ion

    of

    (4) starting

    at

    p which remains in

    Q

    for all

    t

    in

     -

    00, 00);

    that

    is, if

    one starts at p

    at

    the proper

    time,

    the solution

    remains

    in Q for all time. This is the sense now in which Q is an invarian t set. Let

    V(t, x) be Cl on R x R and periodic in t of period T. For an arbitrary set

    G

    of RIJ. we say

    that

    V is a

    Liapunou

    function on G for the periodic system (4)

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    if V does not change sign for all t and all

    x

    in G. Define E· = {(t, x); V(t, x)

    =

    0,

    x

    in

    G}

    and let

    M

    be

    the

    union

    of

    all solutions

    x t) of

    (4) with the

    property

    that (t,

    x(t» is in

    E

    for all

    t. M

    could be called

      the

    largest invar

    iant set relative to E. One then obtain the following version

    of

    Theorem 2

    for periodic systems:

    Theorem

    3. If

    V

    is a Liapunov function on G for the periodicsystem (4),

    then each solution

    of

    (4)

    that

    is bounded and remains in G for all t

    >

    0

    (t

    <

    0)

    approaches

    M

    as

    t

    --+ 00

    (t  

    - 00).

    In [5] Miller showed that the limit sets of solutions of almost periodic

    systems have a similar invariance property

    and

    from this he obtains a resul t

    quite like Theorem 3 for almost periodic systems. This then yields, for pe

    riodic and almost periodic systems, a whole chain

    of

    theorems on stability

    and instability quite similar to that for autonomous systems. Fo r example,

    one has

    Corollary

    4. Let Q

    FI

    +

    =

    {x ;

    V(t, x) <  Y}, all t in [0,

    T]}, and

    let G+

    be

    a component

    of

    Q,,+. Let G be the component

    of

    Q

    FI

    = {x ; V{t, x) < T

    for some r in [0, T]} containing

    G+. If G

    is bounded, V   0 for all t and

    all

    x in G, and if MO = M n G

    c

    G+, then MO is an att ractor and G+ is an

    its region of attraction. If V(t, x) = , t for all t and all

    x

    on the boundary

    of

    MO, then MO is a stable att ractor .

    OUf

    last example

    of

    an invariance principle for ordinary differential equa

    tions is that due to Yoshizawa in [7] for asymptotically autonomous

    systems. It is a consequence of Theorem 1 and results by Markus

    and

    Opial

    (see [7] for references) on the limit sets

    of

    such systems. A system

    of

    the form

    x =

    F x)

    + g(t, x) +

    h(t, x)

    (5)

    is said to be asymptoticallyautonomousif (i) g(t, x)   0 as t

    --.

    00 uniformly

    for x in

    an

    arbitrary compact set

    of

    Rn, (ii)

    f:

    Ih(t,

    9 (t»

    Idt

    < 0 0

    for all

    q; bounded and continuous on [0, 00) to R ,. The combined results of Markus

    and Opial then state that the positive limit sets

    of

    solutions

    of

    (5) are invar

    iant sets

    of

    x = F(x). Using this, Yoshizawa then improved Theorem I

    for asymptotically

    autonomous systems.

    It turns out to be useful, as we shall jIlustrate in a moment on the sim

    plest possible example, in studying systems

     I

    which are

    not

    necessarily

    asymptotically autonomous to state the theorem in the following manner:

    Theorem 4. If, in addition to the conditions

    of

    Theorem 1,

    it

    is known

    that a solution x t)

    of

    (1) remains in G for t > 0 and is also a solution

    of

    an

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    asymptotically

    autonomous system (5), then

    x t)

    approaches M* == M

    u

    {oo} as

    t

      0 0 , where M is

    the largest invariant

    set of

    x

    ==

    F x) in

    E.

    It can happen that the sys tem (1) is itself asymptotically autonomous, in

    which case the above theorem

    can

    be

    applied.

    However, as the following

    example

    illustrates, the original system may

    no t

    itself be asymptotically au

    tonomous, bu t it still may be possible to

    construct

    for

    each solution of

    (I)

    an

    asymptotically autonomous system (5) which it also satisfies.

    Consider again

    the

    example

    x==y

    y

    == -

    x

    -

    p t)y,

    o

    <

    D

     

    pet)

     

    m

    for all t > o

    (6)

    Now we have the additional assumption

    that pet)

    is bounded

    from

    above.

    Let   x t), be any solution

    of

    (6). As was argued previously below

    Theorem 1, all

    solutions are

    bounded

    and yet)

      0 as t   0 0 . Now

    (X(/),

    satisfies x ==

    Y,

    rV = -

    X

    - pet) yet), and this system is asymptotically

    autonomous to

    (*)

     

    y, y := :

    - x.

    With the same

    Liapunov function as

    before, E is

    the

    x   axis and the largest

    invariant

    set of (*) in E is the origin.

    Thus fo r (6)

    the

    origin is asymptotically

    stable

    in the large.

    3.

    Autonomous

    Functional-Differential Equations

    In

    this

    section

    we

    adopt

    completely

    the

    notations

    and assumptions in

    troduced by Hale in his paper in these

    proceedings and

    present a few

    of

    the

    stability results that he has

    obtained

    for autonomous differential equations

    (7)

    A more complete account with numerous examples

    is

    given in (1).

    For

    the

    extension to per iodic and

    almost

    periodic functional-differential

    equations

    by Miller see [6].

    We continue where Hale left off in Sec tion 2

    of

    his paper, except that we

    shall assume

    that

    the

    open

    set Q is

    the whole

    state space C

    of

    continuous

    functions. We also confine ourselves to solutions

    x of

    (7) that

    are

    bounded

    and

    hence defined on [- r, 00). Except

    that

    we

    are

    in t he s ta te space

    C,

    the definition of

    the

    positive limit set

    of

    a

    trajectory x

    f

    of

    (7)

    is essentially

    the same

    as for

    ordinary

    differential

    equations,

    and

    the

    notion of an invar

    iant set is modified to take into account

    the

    fact that there is no longer

    uniqueness to

    the

    left. A set M c C is invariant in the sense that if qJ E M,

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    then

    x(tp)

    is defined on

    [ - , 0 0 ) ,

    there is an extension on

     -00, - r], and

    x, fP)

    remains in

    M

    for all

    t

    in

     -

    00, 00). With these extensions of these

    geometr ic not ions to the state space C, Hale then showed that

    the

    positive

    limit set of a

    trajectory

    of

    (7)

    bounded

    in

    the fu-ture

    is a

    nonempty,

    compact,

    connected,

    and

    invariant set in C. He was then able to

    obtain

    a

    theory

    of

    stability

    quite

    similar to

    that

    for

    autonomous ordinary

    differential equations.

    Let

    V

    be a

    continuous

    function on C to

    R

    and

    define relative to (7)

    · - 1

    V(tp) ==

    lim - [V xr fP» - V

    0 on

    U

    when

    cp :;t:

    0

    and V O =

    0'

    and at

    the

    end

      ...

    in

    tersect the

    boundary

    of C; ... . This is clear from his

    proof and

    is necessary,

    since he wanted to generalize the usual statement of Cetaev's theorem to

    include

    the

    possibility

    that the

    equilibrium

    point

    be

    inside

    U

    as well as on

    its boundary.

    Corollary

    6.

    Let p E

    C be an equil ibrium point of (7) contained in

    the

    closure of an

    open

    set

    U and

    let

    N

    be a

    neighborhood

    of p. Assume that:

    (i)

    V

    is a

    Liapunov

    function on

    G

    =

    U

    n

    N,

    (ii)

    M

    n G is either

    the

    empty

    set or

    p,

    (iii)

    V qJ)

    < 11

    on G

    when

    cp

    = =

    p, and

    (iv)

    V(P) =  Y and V(

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    its

    boundary or approach p. Conditions

    (i)

    and

    (iv) imply

    that it cannot

    reach

    or approach tha t par t of

    the

    boundary

    of Go

    inside

    No

    nor

    can

    it

    approach

    p as

    1 -+

    0 0 .

    Now

    (iii) states

    that

    there

    are

    no points of

    M

    on

    that

    part of

    the boundary

    of

    No

    inside

    G.

    Hence each such trajectory

    must

    leave

    No in finite time. Since

    p

    is either in the inter ior or on

    the boundary

    of G,

    each neighborhood

    of

    p contains

    such trajectories,

    and p is

    therefore un

    stable.

    In .[1]

    it was shown

    that

    the

    equilibrium

    point

    q; = 0 of

    X(/) = ax

    3

    ( / )

    + bx3 1 - r)

    was unstable

    if a

    >

    0 and Ib I < Ia I.

    Using the same Liapunov function

    and

    Theorem

    6 we

    can

    show a

    bit

    more.

    With

    V(q»

    = -

    q>4 O)

    +.. - JO q;6(6)

    dO,

    4a

      r

    V(x,) =

    -- + £ r x6(8)

    dO,

    and

    which is nonposi tive

    when

    I

    b J <

    I

    a

    I (negative definite

    with

    respect to

    , (0) and tp(- r»; that is, V is a Liapunov funct ion on C

    and

    E

    = {

    0,

    the

    region

    G = {q;; V(qJ) < O}

    is nonempty,

    and

    no trajectory starting

    in G

    can

    have

    lp

    =

    0 a s a

    positive limit

    point

    nor can

    it

    leave

    G.

    Hence

    by

    Theo

    rem 5,

    each

    trajectory starting in

    G must be

    unbounded. Since

    qJ =

    0 is a

    boundary

    point of

    G,

    it is unstable.

    It

    is also easily seen [J] that

    if a < 0

    and I

    b

    1< Ia I then cp =

    0 is asymptotically stable in the large.

    In [1]

    Hale

    has a lso extended this theory for systems with infinite lag

      r =

    00), and

    in

    that

    same

    paper

    gives a

    number

    of significant examples

    of the application of this theory.

    REFERENCES

    (I)

    Hale,

    I. ,

    Sufficient conditions for stability and instability of autonomous functional

    differential eauations,

    J. Diff. Eqs.

    1, 452-482 (1965).

    [2] LaSalle,

    J., Someextensionsof

    Liapunov's second

    method, IRE

    Trans. Circuit Theory

    CT-7,

    520-527 (1960).

    319

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