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  • 7/28/2019 Andersen_2002_Post-Critical Behavior of Beck's Column With a Tip Mass

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    *Corresponding author.

    International Journal of Non-Linear Mechanics 37 (2002) 135}151

    Post-critical behavior of Beck's column with a tip mass

    Steen Brahe Andersen, Jon Juel Thomsen*

    Department of Solid Mechanics, Building 404, Technical University of Denmark, DK-2800 Lyngby, Denmark

    Received 1 May 2000; accepted 2 October 2000

    Abstract

    This study examines how a tip mass with rotary inertia a!ects the stability of a follower-loaded cantilevered column.

    Using nonlinear modeling and perturbation analysis, expressions are set up for determining the stability of the straight

    column and the amplitude of post-critical #utter oscillations. Bifurcation diagrams are given, showing how the vibration

    amplitude changes with follower load and other parameters. These results agree closely with numerical simulation. It is

    found that su$ciently large values of tip mass rotary inertia can change the primary bifurcation from supercritical into

    subcritical. This can imply very large motions for follower loads just beyond critical, contrasting the "nite amplitude

    motions accompanying supercritical bifurcations. Also, the straight column may be destabilized by a su$ciently strong

    disturbance at loads far below the value of critical load predicted by linear theory. A similar change in bifurcation is

    found to occur with increased external (as compared to internal) damping, and with a shortening in column length. These

    e!ects are not revealed by linear modeling and analysis, which may consequently fail to predict even qualitatively the real

    critical load for a column with tip mass. 2001 Elsevier Science Ltd. All rights reserved.

    1. Introduction

    We examine how a tip mass with rotary inertia

    a!ects the stability of a follower-loaded canti-

    levered column. If there is no tip mass this system

    corresponds to the well-known Beck's column [1],

    which is known to exhibit soft #utter as the magni-

    tude of the follower load exceeds a critical value[2]. We show how this behavior is qualitatively

    changed by the rotary inertia of a tip mass, which

    can imply that the straight equilibrium of the col-

    umn can be destabilized at a forcing lower than

    critical by a "nite-sized disturbance.

    This work was motivated by theoretical and ex-

    perimental studies by Sugiyama et al. [3] on a col-

    umn subjected to follower forcing produced by

    a solid rocket motor.

    Beck's column has a load at the tip that remains

    tangent to the deformed column axis. The signi"-

    cance of this system is its capability to model and

    illustrate, in a simple manner, the basic properties

    of systems that can display #utter vibrations due to

    follower loading. Such loads are inherentlynon-conservative, acting along lines that move

    with the deformation or displacement of a struc-

    ture. They occur with many real structures,

    e.g., rocket driven aerospace structures, aircraft

    wings, wind turbine blades, and pipes carrying

    #uid #ow. The present study sheds further light

    on possible behavior of follower loaded structures

    for cases where the follower load is delivered by

    a device whose mass and rotary inertia cannot be

    ignored.

    0020-7462/01/$- see front matter 2001 Elsevier Science Ltd. All rights reserved.

    PII: S 0 0 2 0 - 7 4 6 2 ( 0 0 ) 0 0 1 0 2 - 5

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    Beck's initial work [1] on determining the criti-

    cal force of the follower-loaded column has been

    followed by numerous studies of di!erent aspects

    and variants of the system. For example, Herrmannand Jong [4] and Bolotin [5] described the seem-

    ingly paradoxical destabilizing e!ect of internal

    damping (the #utter-critical force in the presence of

    vanishing internal damping being about half of the

    value for zero damping), as contrasted by the

    stabilizing e!ect of external damping [6]. P#uKger

    [7] seems to be the "rst to examine the stability of

    a Beck's column with a point mass, whereas more

    recently Sugiyama et al. [3] paid consideration to

    the e!ects of damping and of a tip mass with rotary

    inertia in their combined theoretical and experi-mental study of a clamped column subjected to

    follower forcing from a rocket motor; see also Lan-

    gthjem and Sugiyama [8].

    Most studies of Beck's column concerns the de-

    termination of critical loads. This can be accomp-

    lished using only linear modeling and analysis.

    However, for studying post-critical behavior one

    needs to incorporate in the model those nonlinear

    e!ects that are thought to be responsible for limit-

    ing the initially exponentially growing motions at

    post-critical loads. To the authors knowledge only

    Kolkka [2] and Chen [9] have employed nonlinearmodeling for Beck's column, showing that the bi-

    furcation describing stationary oscillation ampli-

    tudes at near-critical loads is supercritical, that is:

    for post-critical loads the column performs stable

    oscillations at a constant "nite amplitude (so-called

    `softa #utter).

    The primary motivation for the present work

    was recent laboratory experiments conducted by

    Sugiyama and Langthjem [10], indicating a critical

    load much lower than the one predicted by linear

    modeling. One possible explanation for this couldbe a change of the type of bifurcation at the (lin-

    early predicted) critical force from supercritical into

    subcritical, perhaps due to the inertial properties of

    the rocket motor. As will be explained further be-

    low the existence of such a subcritical bifurcation

    implies that the straight con"guration of the col-

    umn can lose stability at loads lower than (linearly)

    critical, if the disturbance is su$ciently large. We

    therefore investigate how the rigid body properties

    of a tip mass (mass, rotary inertia, center of gravity)

    a!ects the stability properties and types of bifurca-

    tions for Beck's column.

    The paper is organized as follows: Section 2 de-

    scribes the physical model, and the setup of thedi!erential equation governing transverse motions

    with consideration to geometrical nonlinearities.

    Using modal expansion, this equation is discretised

    into a set of nonlinear ordinary di!erential equa-

    tions for use in subsequent analysis. Section 3 de-

    scribes how these equations are solved numerically

    and also shows numerical solutions illustrating

    typical system behavior. Section 4 presents a per-

    turbation analysis of the nonlinear equations of

    motions, leading to analytical expressions for the

    stationary solutions and their stability. In this anal-ysis, nonlinear terms up to "fth order are retained,

    in order to be able to predict possible secondary

    bifurcations associated with a primary subcritical

    bifurcation. If a secondary bifurcation exists, it

    means that stable oscillations could exist at loads

    greater than critical. In this case, the third-order

    solution would be insu$cient to describe the dy-

    namic of the system. Section 5 then employs these

    expressions to present bifurcation diagrams, show-

    ing how the solutions and their stability change

    with the magnitude of the follower load and para-

    meters describing damping and inertial propertiesof the tip mass. The perturbation results presented

    here are supported by two other types or levels of

    analysis: Numerical time integration of a "nite ele-

    ment discretisation of the underlying physical

    model, and numerical time integration of the mode

    shape discretisation. Section 6 "nally sums up the

    "ndings and the main results: the rotary inertia of

    a tip mass on Beck's column can change the type

    of bifurcation at the critical load from supercritical

    to subcritical, and increased external damping as

    compared to internal damping can have the samee!ect.

    2. Model system and equation of motion

    In this section a geometric nonlinear model is set

    up, which describes motion of the column for loads

    larger than the critical force. The model can be used

    to examine the nonlinear e!ects from the mass, its

    rotary inertia and the location of the center of

    136 S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151

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    Fig. 1. System model.

    gravity on the oscillations of the column. If the

    magnitude of the follower load exceeds the critical

    force at which #utter is initiated, linear stability

    theory predicts that the oscillation amplitude willgrow unbounded. In reality, nonlinear e!ects will

    either stabilize the #utter motion into a periodic

    oscillation with constant amplitude (a limit cycle)

    or it will result in amplitudes growing even more

    violently than predicted by the linear model (ex-

    plosive #utter).

    Fig. 1 shows the model. A rocket motor is moun-

    ted at the tip of the cantilevered column. The rocket

    motor produces a thrust P, which is the follower

    load applied to the column. The motor is assumed

    a rigid body, with mass m and rotary inertia J. The

    center of gravity is located at the distance a fromthe tip of the column. The column is assumed to be

    viscoelastic and uniform, and has mass per unit

    length A, length , moment of inertia I, andYoung's modulus E.

    A curvilinear coordinate system is used, where

    y"y(s, t) denotes the transversal deformation of

    the column, t denotes time, and s denotes the cur-

    vilinear position on the column axis. The inextensi-

    bility condition for an in"nitesimal column element

    gives the relation

    (x)#(y)"1, (1)

    where primes denote di!erentiation with respect to

    position s.

    Hamilton's extended principle is employed for

    setting up the equation of motion. Hamilton's prin-

    ciple (e.g. [11]), which holds only for conservative

    systems, states that

    H"0 where H,R

    R

    Ldt, L,T!V, (2)

    where H de"nes the Hamiltonian of the system,

    L is the Lagrangian,T andV are the kinetic and

    potential energy, t

    and t

    are arbitrary instants of

    time, and H is the variation ofH.Hamilton's extended principle states that the vir-

    tual work W done by non-conservative forcesadded to the variation of the Hamiltonian should

    vanish (e.g. [12,13])

    H#R

    R

    Wdt"0. (3)

    The kinetic and potential energy, T

    and V

    , for

    a column element is

    T"

    A(y #x ), (4)

    V"

    1

    2EI"

    1

    2EI

    y

    1!y, (5)

    where dots denote di!erentiation with respect to

    time t, and where the non-linear curvature measure

    for the curvilinear coordinate s has been used. (This

    di!ers from the curvature in rectangular coordi-

    nates, see e.g. [14, p. 46]). The Lagrangian L and

    the Lagrangian density E are introduced as

    L"

    *

    (T!V

    ) ds"

    *

    E ds. (6)

    The Hamiltonian can be divided in two:

    H"H#H

    , whereH

    is the Hamiltonian for

    the column and H

    is the Hamiltonian for the

    mass. The variation of the HamiltonianH

    for the

    column is

    H"

    R

    R

    *

    *E

    *yy#

    *E

    *yy

    #*E

    *yy#

    *E

    *xx dsdt. (7)

    By using the inextensibility condition (1) and integ-

    ration by parts, (7) can be written as

    H"!

    R

    R

    *

    *

    *t

    E

    *y#

    *

    *s

    E

    *y!

    *

    *s

    E

    *y

    !y1#1

    2y

    *

    *t

    *E

    *x

    #y1#3

    2y

    *

    Q

    *

    *t

    *E

    *xdsyds dt. (8)

    S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151 137

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    The kinetic energy T

    of the mass has contribu-

    tions from plane rotation and translations, i.e.

    T"T

    G#T

    V#T

    W. By using Dirac's delta-

    function K, the energies per unit length can bewritten as

    TG"

    JK(s!s

    )

    Q"JK(s!s

    )(1#y)y , (9)

    TV"

    mK(s!s

    )

    d

    dt(x#a cos(

    ))

    "mK(s!s

    )(x#ax ), (10)

    TW"

    mK(s!s

    )

    d

    dt(y#a sin(

    ))

    "mK(s!s

    )(y#ay ), (11)

    where s

    is the location of the mass on the column-

    axis and

    denotes the rotation of the column. The

    center of gravity of the mass is located at the dis-

    tance a from s

    in tangential direction. Later s

    is

    set equal to . The variation of the Hamiltonian

    H

    for the mass can now be written as

    H"

    R

    R

    *

    T

    ds dt

    "R

    R

    *

    TG

    yy#

    TG

    y y #

    TV

    x x

    #T

    Vx

    x#T

    Wy

    y #T

    Wy

    y dsdt.(12)

    By using the inextensibility condition (1) and integ-

    ration by parts this can be transformed to

    H"!

    R

    R

    *

    *

    *t

    TW

    *y#

    *

    *s

    TG

    *y

    !*

    *s *tT

    W#T

    G*y !y1#

    1

    2y

    ;!*

    *t *s

    *TV

    *x#

    *

    *t

    *TV

    *x #y1#3

    2y

    ;*

    Q!*

    *t*s

    *TV

    *x#

    *

    *t

    *TV

    *x dsy dsdt.(13)

    The follower force P has x- and y-components

    PV

    , PW

    :

    P"(PV , PW )"(!P cos( ()),!P sin( ())), (14)

    where

    () is given by

    ()"arcsin(y()) whichgives that

    PV"!P(1!y()

    +!P(1!y()!

    y()), (15)

    PW"!P sin(arcsin(y()))"!Py(). (16)

    The virtual work of the non-conservative follower

    force can be divided in two: W"WV#W

    W,

    where WV

    and WW

    are the virtual work in the x-and y-directions, respectively. By using (15) and (16)

    these can be written as

    WV"P

    Vu"P(1!

    y()!

    y())u, (17)

    WW"P

    Wy()"!Py()y(). (18)

    Here u denotes the tip displacement in the negative

    x-direction. By considering an in"nitesimal column

    element and integrating over the column length

    , u can be found as

    du"1!dx

    ds ds"(1!(1!y) ds, (19)

    u"*

    (1!(1!y) ds"*

    f(y) ds. (20)

    The variation u become

    u"*

    f(y) ds"*

    *f(y)

    *yy ds

    K*

    y#12y#3

    8yy ds. (21)

    Inserting (21) into (17), the virtual work in the

    x-direction becomes

    WV"

    *

    P1!1

    2y()!

    1

    8y()

    ;y#1

    2y#

    3

    8yy ds. (22)

    138 S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151

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    Integrating (22) by parts and applying Dirac's

    delta-function to (18), the total virtual work from

    the force P can be written as

    W"*

    !PyK(s! )

    !Py#y3

    2y!

    1

    2y()

    #y15

    8y!

    3

    4y()y

    !1

    8y()yds. (23)

    By inserting (8), (13) and (23) in (3) and requiring

    that (3) is ful"lled for arbitrary admissible variation

    in y, one obtains in dimensionless form

    K###K(!1)

    #(!

    )(K#K )!(K(!

    )K )

    !(K(!

    )(K#K ))

    #R#'#R

    #'#R

    #R

    #R

    .

    #R.#RK#RK"0, (24)

    where the nondimensional quantities are given by

    "y

    , "

    x

    , "

    EI

    At, "

    P

    EI,

    "J

    A, "

    m

    A, "

    a

    (25)

    and the dots and primes denote di!erentiation with

    respect to dimensionless time and position . This

    equation describes the transverse displacements(, ) of the column. The "rst and second term in(24) represent linear inertia and sti!ness from the

    column, the third and fourth term represent a linear

    sti!ening e!ect from the follower force and the "fth

    to the seventh term represent linear inertia from the

    tip mass, its rotary inertia and the location of the

    center of gravity. The functions R#'

    , R#'

    , R

    ,

    R

    , R.

    , R.

    , RK

    and RK

    represent the nonlinear

    e!ects and are given in the appendix. They repres-

    ent terms of third and "fth order and describe,

    respectively, sti!ness of the columnR#'

    , R#'

    , axial

    inertia of the column R

    , R

    , e!ects from the

    follower force R.

    , R.

    , and e!ects from the mass

    RK , RK .A mode shape expansion is now applied to trans-

    form the partial di!erential equation (24) into an

    approximating set of ordinary di!erential equa-

    tions. The expansion

    (, )",H

    H()

    H() (26)

    is used, where H

    are the mode shapes of a canti-

    levered column with a tip mass, and H

    are the

    unknown time varying modal coe$cients. By use of

    Galerkin's method (e.g. [15]) one obtains

    M$#CQ#S#g(,Q ,$)#g(,Q ,$)"0

    (27)

    where M is the mass matrix, C is the damping

    matrix, and S is the sti!ness matrix. The vectors

    g and g contain nonlinear terms of third and "fthorder, respectively:

    g",

    HIJ

    ((HIJ#

    HIJ)

    H

    I

    J)

    #,

    HIJ

    ((HIJ#

    HIJ)

    H(

    I$

    J#Q

    IQ

    J)), (28)

    g",

    HIJKL

    ((IHIJKL#I

    HIJKL)

    H

    I

    J

    K

    L)

    #,

    HIJKL

    ((I?AAHIJKL#I?AA

    HIJKL)

    H

    I

    J

    K$

    L)

    #,

    HIJKL

    ((ITCJHIJKL#ITCJ

    HIJKL)

    H

    I

    JQ

    KQ

    L).

    (29)

    The constants HIJ

    , HIJ

    , HIJ

    , HIJ

    , IHIJKL

    , IHIJKL

    ,

    I?AAHIJKL

    , I?AAHIJKL

    , ITCJHIJKL

    and ITCJHIJKL

    are computed from

    the expansion functions and can be found in the

    appendix.

    The constants HIJ

    and HIJ

    , which correspond to

    the nonlinear e!ects of third order from the sti!ness

    and the axial inertia of the column, respectively,

    have also been found and used by e.g. Semler et al.

    [12], who set up the equation of motion for a pipe

    S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151 139

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    Fig. 2. Tip displacement and frequency spectrum for a column with no tip mass for a force "13.53 which is greater than the critical

    force "12.93. Parameters: "0, "0, "0, "0.1, "0.01. (a): Tip displacement as function of time for four di!erent initial

    conditions, where the tip amplitude is given and the velocity is zero; (b): Frequency spectrum. &*' nonlinear analytic model, &- - -' Finite

    element model.

    conveying #uid. To the author's knowledge, the set

    up of an equation of motion including "fth-order

    terms by use of Galerkins method for a column

    with a tip mass subjected to a follower force is notreported in the literature. The remaining constants

    other than HIJ

    and HIJ

    are therefore new results.

    Damping has been added to (27) in the form of

    internal and external viscous damping, where the

    elements in C are given by

    cGH"

    GH

    d#

    GH

    d. (30)

    Here is the external damping factor and is theinternal damping factor. The elements in M and

    S are given by

    mGH"

    GH

    d, (31)

    sGH"

    (GH!

    GH) d#

    G(1)

    H(1). (32)

    Eq. (27) along with (28)}(32), describes a set of

    coupled nonlinear ordinary di!erential equations

    where the time-dependent modal coe$cients H

    are

    the unknowns. The equation is now ready to be

    solved, and this is done numerically and by a per-

    turbation method in the following two sections.When the modal coe$cients are found the behavior

    of the column in time can be described by using (26)

    to calculate the transverse de#ection of the col-umn.

    3. Numerical simulation

    Numerical simulations of (27) are performed

    with the purpose to verify pertubation solutions,

    and to verify the model itself by comparing the

    numerical solutions with solutions obtained by

    a "nite element model. Furthermore, the transient

    behavior and a frequency spectrum can be ob-

    tained.

    Eq. (27) is solved numerically using the trapezmethod (e.g. [16]), which is a "nite-di!erence

    method. The solution gives the displacement of the

    column during time. Fig. 2(a) shows the tip dis-

    placement as function of time for four di!erent

    initial tip displacements, for a situation where the

    load is greater than critical for #utter. As can be

    seen the post-transient vibration amplitude is the

    same for the four simulations. A frequency spec-

    trum for the simulations in Fig. 2(a) is shown in Fig.

    2(b), along with a frequency spectrum from a "nite

    element simulation. It appears that the column

    vibrates at its "rst eigenfrequency and a higherharmonic. The "nite element simulation gives both

    140 S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151

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    Fig. 3. Finite tip vibration amplitude

    as function of number

    of shape functions. Critical force"12.93, "0, "0, "0,

    "0.1, "0.01.

    qualitative and quantitative the same results as the

    model presented here.

    Fig. 3 shows the dependency of the number N of

    expansion functions H

    on the post transient vibra-

    tion amplitude

    . It is necessary to use from four

    to nine expansion functions to ensure that the solu-

    tion is independent of the discretisation. It is neces-

    sary to use even more expansion functions near

    critical loads.The geometric nonlinear dynamic "nite element

    model, used above for comparison was set up using

    64 2D beam elements with two nodes and six de-

    grees of freedoms each. The nonlinearities have

    been applied by using a method of updating the

    coordinates [17]. Lin and Tsai [18] have used this

    method in a nonlinear dynamic analysis of a canti-

    levered column conveying #uid. The method here is

    used similarly, to simulate the dynamics of a canti-

    levered column with a tip mass and a follower force

    at the tip. The follower force and the e!ects fromthe tip mass have been applied as external forces at

    the "nite element node corresponding to the col-

    umn tip.

    Numerical di$culties (lack of convergence) have

    been encountered with the "nite element model in

    cases where the tip mass is large or rotary inertia is

    present. Implementation of another numerical

    method, which takes into account the external for-

    ces in the tangential sti!ness matrix might solve

    this problem.

    The numerical solutions of (27) and the "nite

    element solutions described above are used for

    verifying the pertubation solutions to be described

    next.

    4. Perturbation solutions

    At loads greater than the critical, #utter occurs,

    which can evolve into periodic oscillations about

    the previously stable equilibrium. This change can

    be described as a supercritical Hopf-bifurcation. In

    this case, the nonlinear e!ects are stabilizing. An-

    other possibility is that the oscillation amplitude

    grow unbounded, which can be described as a sub-critical Hopf-bifurcation. In this case, the non-lin-

    ear e!ects are destabilizing on the oscillations.

    To obtain insight into the system behavior at

    near-critical loads, and to analyze the e!ect of

    changing system variables, a perturbation analysis

    is performed. A multiple scales method is employed

    for this (e.g. [19,20]). The procedure presented here

    is equivalent to the one used by Thomsen [21] and

    Jensen [22].

    Eq. (27) can be written as a system of"rst-order

    equations

    x"A()x#f(, x, x )#fI(, x, x ), (33)

    where x"+ Q ,2 and the parameter is introduc-ed as a bookkeeping parameter to indicate the

    smallness of non-linearities. The matrix A and the

    vectors f and fI are given by

    A"0 I

    !M\S !M\C, f"0

    !M\g,

    fI"

    0

    !M\g

    , (34)

    where I is the identity matrix. Two time scales are

    introduced: a fast scale " for describing

    motions at frequencies comparable to the natural

    frequencies, and a slow scale " describing

    slow modulation of oscillation amplitudes.

    Solutions x to (33) are approximated through

    uniformly valid expansions of the form

    x"x

    (

    ,

    )#x

    (

    ,

    )#O(), (35)

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    ;

    (d

    HIJKL!

    fHIJKL

    )

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL

    !

    eHIJKL

    uHuIuJuKuL#

    uHuIuJuKuL!

    uHuIuJuKuL!uHuIuJuKuL#

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL#

    uHuIuJuKuL

    , (51)

    q"aL

    ,

    HIJ

    (bHIJuHuIuJ!2

    cHIJuHuIuJ)

    #aaL,

    HIJKL

    (52)

    ;

    (d

    HIJKL!

    fHIJKL

    )

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL

    !

    eHIJKL

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL

    q"aL

    ,

    HIJKL

    (dHIJKL

    uHuIuJ!

    (e

    HIJKL

    #fHIJKL

    )uHuIuJuKuL

    ), (53)

    where uH

    is the jth element of u. Since i

    is an

    eigenvalue of A

    , the solution of (50) will contain

    secular terms proportional to

    exp(i

    ) unless

    q

    is orthogonal to the left eigenvector v of A

    (e.g.

    [23]), which means that v2q"0 where v is given by

    (A2!i

    )v"0. (54)

    Substituting q

    of (51) into v2q"0 yields the

    solvability condition

    da

    d

    !a!aa!aa"0, (55)

    where , , and are given by

    "v2A

    u

    v2u,

    0#i

    '(56)

    "v2L,

    HIJ(b

    HIJ(u

    HuIuJ#u

    HuIuJ#u

    HuIuJ)

    v2u

    !2

    cHIJuHuIuJ)

    v2u,

    0#i

    '(57)

    "v2L

    v2u

    ,

    HIJKL

    ;(dHIJKL!fHIJKL)uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL#

    uHuIuJuKuL

    S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151 143

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    !

    eHIJKL

    uHuIuJuKuL#

    uHuIuJuKuL!

    uHuIuJuKuL!uHuIuJuKuL#

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL!

    uHuIuJuKuL#

    uHuIuJuKuL ,0#i' . (58)

    Here (0

    , '), (

    0, ') and (

    0, ') denotes the real and

    imaginary parts of , and . The function a()can be expressed in terms of two real-valued func-

    tions A(

    ) and (

    ):

    a(

    )"A(

    ) exp(i(

    )), A, 3R. (59)

    Inserting (59) in the solvability condition (55), this

    can be written as two modulation equations, de-

    scribing evolutions of the slowly changing oscilla-

    tion amplitude A and frequency :

    dA

    d"

    0A#0A

    #0A

    , (60)

    d

    d

    A"'A#

    'A#

    'A. (61)

    Solutions corresponding to oscillations with con-

    stant amplitude can be found by letting dA/d"

    0. Below, one solution is found for the third- and

    "fth-order expansion, respectively. It is possible

    that the solution for the "fth-order expansion gives

    a secondary bifurcation that does not show up

    using only the third-order expansion [22].

    4.1. Third-order solution

    For this approximation terms of"fth order in the

    modulation equations are ignored. Eq. (60) then

    has two singular points: A"0 which corresponds

    to the zero-solution, and A"(!0

    /0

    which

    corresponds to a stationary periodic solution for

    !0

    /0'0 (a limit cycle). Combining Eqs. (35),

    (48), (59) and (61) and setting "1, the limit cycle

    approximation becomes

    x"x#x

    #O()

    "2Re[A expiu exp(i)]#O()

    "2!0

    0

    "u"cos((#

    '!(

    '/0

    )0

    ))#O().

    (62)

    The post-transient tip amplitude

    for the column

    can now be found by inserting the amplitudes

    max(G)"max(x

    G), i)N of the modal coordi-

    nates into the modal expansion (26):

    " ,

    G

    G(1) max(x

    G)"2!

    00

    ,G

    G(1)"u

    G",

    (63)

    where G

    is the ith eigenmode for the cantilevered

    column with a tip mass and uG

    is the ith component

    of the eigenvector u from (49).

    4.2. Fifth-order solution

    Retaining the "fth-order terms in (60), the non-

    zero singular points become

    A"!0$(0!40020

    .(64)

    The tip amplitude

    can now be found as above by

    inserting (62) into (26)

    "2!0$(0!4002

    0

    ,G

    G(1)"u

    G".

    (65)

    4.3. Stability of stationary solutions

    The stability of the singular point A is evaluated

    by inserting it into the gradient of (60)

    (A)"0#3

    0A#5

    0A. (66)

    If this value is negative, then A is stable, otherwise

    A is unstable.

    Now, the stationary solutions and their stability

    are calculated for particular parameters of the

    column. These solutions are valid for loads in a

    vicinity of the critical force. This means that

    144 S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151

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    Fig. 4. Bifurcation diagrams. (a) No tip mass "0.0; (b) With tip mass "0.2. Damping: "0.1, "0.01. * Finite element; numerical solution to (27); &*' stable, and &- - -' unstable 3rd and 5th order pertubation solutions.

    a bifurcation diagram can be made from the solu-

    tions and their stabilities, and hereby the e!ects

    from the nonlinearities can be evaluated.

    5. Bifurcations

    The nonlinear oscillations of the column at loads

    near the critical force will now be examined. The

    nonlinear e!ects from the sti!ness of the column,

    the tip mass, its rotary inertia, and the location of

    the center of gravity will be examined separately.

    For loads greater than critical the nonlinear ef-

    fects can either stabilize the #utter into oscillations

    with constant amplitude, or they can destabilizeeven further so the #utter becomes explosive. This

    change in response as the load exceeds the critical

    value corresponds to a supercritical or a subcritical

    bifurcation, respectively.

    If the bifurcation is supercritical only the stable

    zero-solution exists at loads smaller than the criti-

    cal force. The stability limit of the zero-solution can

    therefore be found by linear theory. If the bifurca-

    tion is subcritical, however, the nonlinear e!ects

    can destabilize the zero-solution if the column ex-

    periences a disturbance of su$cient strength. In

    this case, the behavior of the system is thereforeradically changed and linear stability theory is in-

    su$cient to determine the real critical force for

    disturbances of "nite magnitude. It is therefore of

    great importance to know which kind of bifurca-

    tion there will exist at particular values of para-

    meters.

    5.1. Column with no tip mass

    Fig. 4(a) shows the bifurcation diagram for a col-

    umn with no tip mass. The bifurcation is supercriti-

    cal, which means that the nonlinear e!ects stabilize

    the #utter into a limit cycle. This is in agreement

    with Kolkka [2], who shows mathematically that

    the bifurcation is supercritical for Beck's column.

    As appears, the numerical simulations of Eq. (27)

    match very well with the "nite element simulations

    and the approximative perturbation solution. Theperturbation solutions of third and "fth order show

    no signi"cant di!erences.

    5.2. Column with a tip mass

    A tip mass with a mass of 20% of the column

    mass has been applied at the tip-end of the column.

    The bifurcation diagram in Fig. 4(b) shows that the

    bifurcation is still supercritical. The critical force is

    smaller than for the column with no tip mass. The

    shape of the bifurcation is comparable with theone for the column with no tip mass, indicating that

    the mass does not qualitatively change the dynam-

    ics of the column.

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    Fig. 5. Bifurcation diagrams for a column having rotary inertia at the tip. (a) "0.002; (b) "0.2. Damping: "0.1, "0.01. Numerical solution to (27); &*' stable, and &- - -' unstable 3rd and 5th order pertubation solutions.

    5.3. Column with rotary inertia at the tip

    To shed light on the isolated e!ect of rotary

    inertia, we consider here the (unrealizable) caseof a zero tip mass having nonzero rotary inertia.

    Fig. 5(a) and (b) shows the bifurcations for a col-

    umn with two di!erent values of inertia at the

    tip-end. The bifurcation is still supercritical as long

    as the rotary inertia is very small. The shape of the

    branching bifurcation becomes steeper, indicating

    that the nonlinear e!ects from the rotary inertia are

    destabilizing. This indication is supported by the

    bifurcation in Fig. 5(b), where the rotary inertia is

    even larger. First, it should be noted that the larger

    rotary inertia decreases the critical load signi"-cantly. Secondly the bifurcation has changed and

    has become subcritical, meaning that the system

    behaves in a completely di!erent way. At loads

    smaller than critical, it is possible to destabilize the

    zero solution by disturbing the column su$ciently

    so the amplitude becomes greater than the ampli-

    tude of the unstable limit circle. The "fth-order

    perturbation solution shows the same as the solu-

    tion of third order: there are no stable solutions at

    loads greater than the critical. At loads greater than

    the critical, motions are therefore not limited by the

    nonlinearities included in the present model; fora real model other nonlinearities such as plastic

    deformation or fracture will limit the response. In

    numerical simulations explosive growths in ampli-

    tudes were observed until numerical instability oc-

    curred at very large deformations.

    5.4. Column with a tip mass having rotary inertia

    Fig. 6(a) shows the bifurcation for a column with

    a tip mass having rotary inertia and Fig. 6(b) shows

    the bifurcation for a case where the center of gravity

    of the mass is located at a distance from the tip. The

    "gures show that the shape of the bifurcations are

    steeper compared to the bifurcation for the column

    with no tip mass. This is due to the rotary inertia

    and the location of the center of gravity, which

    gives a resulting moment of inertia at the tip. The

    numerical simulations match very well the solu-tions found by the third- and "fth-order perturba-

    tion solutions. If the rotary inertia is su$ciently

    large, the bifurcation will become subcritical, and

    the #utter will be explosive. This was con"rmed by

    numerical simulations.

    5.5. Change of bifurcation

    For a given tip mass having rotary inertia, Fig. 7

    shows if the bifurcation at the critical load is sub- or

    supercritical. As appears, when the rotary inertia is

    su$ciently large the type of bifurcation changesfrom super- to subcritical, we call this value the

    critical rotary inertia. When the tip mass is about

    the same as the mass of the column or larger ('1)

    146 S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151

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    Fig. 6. Bifurcation diagrams for a column with a tip mass having rotary inertia , the center of gravity beeing located a distance fromthe tip. (a) "2.0, "0.2, "0.0; (b) "2.0, "0.2, "0.1. Damping: "0.1, "0.01. Numerical solution to (27); &*' stable,and &- - -' unstable 3rd and 5th order pertubation solutions.

    Fig. 7. Type of bifurcation as function of tip mass , tip massrotary inertia , and position of center of gravity . Damping:"0.1, "0.01. Solid lines mark the boundaries between

    supercritical and subcritical bifurcations.

    there is an approximative linear relationship be-

    tween the mass and the critical rotary inertia

    (/"m/J"constant). As also appears a sub-critical bifurcation can occur only when the

    rotary inertia is non-zero. Finally, it should

    be observed, that for a given tip mass having

    rotary inertia, a shortening of column length can

    cause a change in bifurcation from super- to sub-

    critical.

    5.6. Dependency of damping

    Fig. 8 shows the signi"cants of the ratio of ex-

    ternal to internal damping / on the type of bifur-cation. As appears the bifurcation type is highly

    dependent on this ratio. The damping coe$cients

    and can be very di$cult to estimate correctlyfor real systems, and thus it may be di$cult toestimate which kind of bifurcation will actually

    occur. It should also be noted that if the energy

    dissipation is dominated by external damping

    (/

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    Fig. 8. Type of bifurcation as function of the ratio of tip mass to

    tip mass rotary inertia, /, and the ratio of external to internaldamping /.

    for near-critical loads. This lead to analytical ex-

    pressions for the post-critical solutions and their

    stability. The results were subsequently employed

    to establish bifurcation diagrams, showing how the

    stationary vibration amplitude depends on the

    magnitude of the follower load and other para-

    meters. Again, results were veri"ed by numerical

    simulation.The main result of this work is the observation

    that the rotary inertia of a tip mass on a Beck's

    column can change the type of bifurcation at the

    critical load. At su$ciently large values of rotary

    inertia, this bifurcation will change from supercriti-

    cal to subcritical. This implies two phenomena that

    are not revealed by linear analysis: First, at su$-

    ciently large values of rotary inertia there will be no

    stable small-amplitude motions for follower loads

    just beyond the critical; only motions with very

    large amplitude are then possible. Secondly, thestraight con"guration of the column may be de-

    stabilized by a su$ciently strong disturbance at

    loads below the critical load predicted by linear

    theory. Thus, the presence of large rotary inertia

    may make stability analysis based only on linear

    modeling insu$cient. The same observation holds

    true even for a tip mass with negligible rotary

    inertia, if its center of gravity is displaced rigidly

    beyond the column tip, or if a column with a given

    tip mass and rotary inertia is shortened.

    Increasing the external damping of the system (as

    compared to internal damping) also has this e!ect

    of changing the primary bifurcation from super-

    critical to subcritical. Since with real systems thecharacter and magnitude of damping e!ects are

    rarely known to any great precision, this implies

    that predictions based only on linear theory might

    fail simply due to a wrong estimate of damping

    coe$cients.

    The above theoretical results will need experi-

    mental veri"cation. It would be relevant to system-

    atically examine critical loads and post-critical

    behavior for a follower-loaded clamped column as

    a function of changing rotary inertia of a tip mass.

    For example, tests similar to those described inSugiyama et al. [3] and Langthjem and Sugiyama

    [8] could be performed with two additional masses

    at the rocket motor, mounted on a rigid beam

    perpendicular to the column and with variable sep-

    aration.

    Acknowledgements

    The authors wish to thank Mikael Langthjem for

    suggesting this work, and for many useful com-

    ments and suggestions.

    Appendix A

    A.1. Dimensionless functionals

    R#'"#4# (A.1)

    R#'"6#8#, (A.2)

    R"

    K

    (

    #K )d!

    K K

    (

    #K ) d d, (A.3)

    R"

    K

    3

    2 #

    1

    2K d

    #1

    2

    K

    ( #K ) d

    !

    K K

    3

    2 #

    1

    2K d d

    148 S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151

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    !3

    2

    K K

    ( #K ) d, (A.4)

    R."

    3

    2!

    1

    2(1), (A.5)

    R."

    15

    8!

    3

    4(1)!

    1

    8(1), (A.6)

    RK"!(K(!

    )(K # ))

    !K(!)K

    ( #K ) d

    #( #K )!K(!

    )

    K

    (

    #K ) d#( #K )!

    K

    ( #K ) d#( #K ),(A.7)

    RK"!(K(!

    )(K #2 ))

    !K(!)K

    3

    2 #

    1

    2K d

    #3

    2 #

    1

    2K

    !K(!

    )

    K

    3

    2

    #1

    2

    K

    d

    #3

    2 #

    1

    2K

    !

    2K(!)

    K

    (

    #K ) d#( #K )

    !K(!

    )K

    ( #K ) d

    #( #K )

    !

    K

    3

    2 #

    1

    2K d

    #3

    2(

    ) (

    )

    #1

    2(

    )K (

    ) (A.8)

    !

    3

    2

    K

    (

    #K ) d

    #( #K ). (A.9)A.2. Non-linear coezcients

    GHIJ"

    3

    2

    GHIJ

    d

    !

    1

    2

    GHdI (1)J(1)

    , (A.10)

    GHIJ"

    GHIJ

    d#4

    GHIJ

    d

    #

    GHIJ

    d, (A.11)

    GHIJ"

    GHK

    IJ

    d d

    !

    GH

    K

    K

    IJ

    d d d, (A.12)

    BGHIJ"

    G(1)

    H(1)

    I(1)

    J(1)

    #(G(1)

    H(1)#(

    G(1)

    H(1)#

    G(1)

    H(1)))

    ;

    IJ

    d#I

    (1)J(1)

    !

    GH

    d

    IJ

    d#I

    (1)J(1),

    (A.13)

    S.B. Andersen, J.J. Thomsen /International Journal of Non-Linear Mechanics 37 (2002) 135}151 149

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    IGHIJKL"

    15

    8

    GHIJKL

    d

    !34H(1)

    I(1)

    GJKL

    d (A.14)

    !1

    8H(1)

    I(1)

    J(1)

    K(1)

    GL

    d,

    (A.15)

    IGHIJKL"6

    GHIJKL

    d

    #8

    GHIJKL

    d, (A.16)

    #

    GHIJKL

    d, (A.17)

    ITCJGHIJKL"

    3

    2

    GHK

    IJKL

    d d

    #1

    2

    GHIJK

    KL

    d d

    !3

    2

    GH

    K

    K

    IJKL

    d d d

    !3

    2

    GHIJ

    K K

    KL

    d d d,

    (A.18)

    BITCJGHIJKL"2

    G(1)

    H(1)

    I(1)

    J(1)

    K(1)

    L(1)

    #3

    2G(1)H(1)#(G(1)H (1)

    #G(1)H (1))!

    GH d

    ;

    IJKL

    d

    #I

    (1)J(1)

    K(1)

    L(1)) (A.19)

    #1

    2(

    G(1)

    H(1)

    I(1)

    J(1)

    #(G(1)

    H(1)

    I(1)

    J(1))

    !3

    GHIJ

    d;

    KL

    d#K

    (1)L

    (1), (A.20)I?AA

    GHIJKL"

    1

    2

    GHK

    IJKL

    d d

    #1

    2

    GHIJK

    KL

    d d

    !1

    2

    GH

    K K

    IJKL

    d d d

    !32

    GHIJ

    K K

    KL

    d d d

    (A.21)

    BI?AAGHIJKL"

    G(1)

    H(1)

    I(1)

    J(1)

    K(1)

    L(1)

    #1

    2G(1)H(1)#(G(1)H (1)

    #G(1)

    H(1))!

    GH

    d;

    IJKL d

    #I

    (1)J(1)

    K(1)

    L(1)) (A.22)

    #1

    2G(1)H(1)I (1)J (1)

    #(G(1)

    H(1)

    I(1)

    J(1))

    !3

    GHIJ

    d;

    KL d#K (1)L(1). (A.23)

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