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  • 7/27/2019 DEFLECTION & STIFFNESS OF MEMBERS.pdf

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    CHAPTER 5

    DEFLECTION AND STIFFNESS

    Beam deflection can be found by 3 methods: 1) Integration, 2) Superposition and 3)

    Castiglianos Theorem. These are detailed as follows:

    1) Beam deflection by Integration (Section 5-3, pg. 188 in the textbook):

    If the deflection of a beam is mainly due to the bending moment, then the following

    formula is applied to find the deflection of the beam:

    EI

    M

    dx

    yd

    2

    2

    =

    where y is the vertical deflection, x is the horizontal distance, E is the modulus

    elasticity and I is the area moment of inertia as before. We also find the slope as:

    +== 1cdxEIM

    dx

    dy

    where c1 is a constant found from the end or boundary conditions of the beam.

    Example: Find general expressions for the deflection and slope of the following

    beam.

    y ya FBD:w FF waa/2

    B x xC

    First we draw a FBD for the system to find the reactions, which are found from

    Newtons equations as RA = F+wa and MA = FL+wa2/2. We then cut the beam

    between A-B and B-C to find the bending moments ofMAB andMBCas:

    We sum the moments at the cut sections and let them to be zero to find:

    MAB = RAxwx2/2MA = wx2/2+(F+wa)x(FL+ wa2/2) and2MBC= RAxwa(xa/2)MA = (F+wa)xwa(xa/2)(FL+ wa /2) =F(xL).

    ww a

    MBC

    y

    MAMA

    MAB

    yVAB

    RA x

    VBC

    RA x

    A RAMA

    LL

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    Deflection and Slope between A-B, i.e. 0 x a:

    1

    22

    1 )2

    ()(2

    1cdx

    awFLxwaFx

    w

    EIcdx

    EI

    M

    dx

    dy AB +

    +++

    =+= Slope =AB =

    = 1

    223 )

    2(

    2

    )(1cx

    awFLx

    waFx

    w+

    ++

    +

    6EI

    Since AB = 0 atx =0 then c1 = 0. Hence:

    AB =

    +

    ++

    x

    awFLx

    waFx

    w

    EI)

    2(

    2

    )(

    6

    1 223 .

    Deflection=yAB =2

    223

    2)

    2(

    2

    )(

    6

    1cdxx

    awFLx

    waFx

    w

    EIcdx

    AB+

    +

    ++

    =+

    = 22

    234

    4

    )(2

    6

    )(

    24

    1cx

    awFLx

    waFx

    w

    EI+

    +

    ++

    SinceyAB = 0 atx =0 then c2 = 0. Hence:

    yAB =

    +

    ++

    22

    34

    4

    )(2

    6

    )(

    24

    1x

    awFLx

    waFx

    w

    EI.

    eflection and Slope between B-C, i.e. ax L:D

    lope = BC= 33 )(1

    cdxLxFEI

    cdxEI

    M

    dx

    dy BC +=+= S

    = 3

    2

    )2

    ( cLxxF

    +EI

    .

    ince AB = BCatx =a where from the above equations:S

    axAB = =

    ++ aFLaa

    EI

    )

    2

    (

    26

    +

    )

    2

    (

    6

    1 3 La

    Faaw

    EI

    + awwaFw )(1 223 =

    axBC = = 3

    2

    )2

    ( cLaa

    EI

    F+ and hence c3 =

    EI

    wa

    6

    3. Therefore:

    BC=

    6)

    2(

    1 2 3waLx

    xF

    EI.

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    Deflection =yBC= 4

    2

    46

    )2

    (1

    cdxwa

    Lxx

    FEI

    cdx3

    BC +

    =+ .

    = 4

    23

    6

    )

    26

    (1

    cxwax

    Lx

    F

    EI

    3

    +

    SinceyAB =yBCatx =a where from the above equations:

    axABy = =

    +

    ++

    22

    34

    4

    )(2

    6

    )(

    24a

    awFLa

    waFa

    w

    EI

    1=

    =

    +

    268

    234 FLaFa

    EI1 wa

    .

    axBCy = = 4

    23

    6

    )

    26

    (1

    cawaa

    La

    F

    EI

    3

    +

    and hence c4 =

    EI

    wa

    24

    4

    . Therefore:

    yBC=

    +

    246)

    26(

    1 423 wax

    waxL

    xF

    EI

    3

    .

    Note: Review example 5-1, pg. 190 in the textbook.

    2) Beam Deflection by Superposition (Section 5-5, pg. 192 in the textbook):

    Refer to 16 cases given in the Appendix A-9, from pg. 969 to 976 in the textbook. Thesuperposition for linear systems means that we can find the reactions, bending

    moments, shear forces, slope and deflection by summing up these entities for each

    loading case. So lets solve the above example by the superposition technique. We

    have,

    y yya wa w

    FFB Bx

    +C C CA AA L LL

    Deflection and Slope between A-B, i.e. 0 x a:

    Slope =AB = 1AB + 2AB , where from Table A-9-3, pg. 970 in the textbook,

    1AB =dx

    dy= )xaxax(

    EI

    w 232 336

    where lis replaced by a in the formula. Also,

    from Table A-9-1, pg. 969 in the textbook, 2AB =dx

    dy= )Lxx(

    EI

    F2

    2

    2 . Hence,

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    AB= )xaxax(EI

    w 232 336

    + )Lxx(EI

    F2

    2

    2 =

    +

    ++

    x

    awFLx

    waFx

    w

    EI)

    2(

    2

    )(

    6

    1 223 ,

    which is the same result obtained before using the integration method.

    Deflection =yAB =y1AB +y2AB , where from Table A-9-3, pg. 970 in the textbook,

    y1AB = )6(424

    222 axaxEI

    wx where again l is replaced by a in the formula. Also,

    from Table A-9-1, pg. 969 in the textbook,y2AB = )Lx(EI

    Fx3

    6

    2

    . Hence,

    yAB= )6(424

    222

    axaxEI

    wx + )3(

    6

    2

    LxEI

    Fx =

    +

    ++

    22

    34

    4

    )(2

    6

    )(

    24

    1x

    awFLx

    waFx

    w

    EI,

    which is again the same result obtained before using the integration method.

    Deflection and Slope between A-B, i.e. ax L:

    Slope =BC= 1BC+ 2BC. Since there is no bending moment between B-C for the case

    of distributed load w, we can assume that the slope remains the same as 1AB atx=a.

    Hence,1BC= axAB1 = =EI

    wa3

    6

    . Also, from Table A-9-1, pg. 969 in the textbook,

    2BC= 2AB = )2(2

    2 LxxEI

    F . Hence,

    BC=EIwa3

    6 + )2(

    22 Lxx

    EIF =

    6)

    2(1 2 3waLxxF

    EI,

    which is the same result obtained before using the integration method.

    Deflection =yBC=y1BC+y2BC.

    For the case of distributed load w, the angle 1BCremains the same between B-C, and

    hence the deflected curve between B-C is a linear one.

    ywa

    Deflected CurveB

    C1BA

    y1BCx 1BC

    From the figure,y1BC = 1BC(xa)+ y1B, wherey1B = axAB1y = =EI

    wa

    8

    4. Therefore,

    y1BC=

    EI

    axwa

    6

    )(3 +

    EI

    wa

    8

    4= )4(

    24

    3

    ax

    EI

    wa+ .

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    For the end load ofF, again referring to Table A-9-1, pg. 969 in the textbook, y2BC=

    y2AB = )3(6

    2

    LxEI

    Fx . Hence,

    yBC= =y1BC+y2BC= )4(24

    3

    axEI

    wa + + )Lx(EI

    Fx 36

    2

    =

    +

    246)

    26(1

    423waxwaxLxF

    EI

    3

    ,

    which is again the same result obtained before using the integration method.

    Note: Review examples 5-2 and 5-3, pgs. 192 and 193 in the textbook.

    3) Beam Deflection by Castiglianos Theorem (Sections 5-7 and 5-8, pgs. 198 and

    201 in the textbook):

    When a machine element is deformed, it stores a potentialorstrain energy U. This

    energy can be calculated for different loading cases, as given below:

    Loading Strain Energy (U)

    Tension or CompressionEA

    LF

    2

    2

    Direct ShearGA

    LF

    2

    2

    TorsionGJ

    LT

    2

    2

    Bending Moment EIdxM

    2

    2

    Bending Shear GAdxcV

    2

    2

    where for bending shearc is a factor that depends on the cross-section of the beam

    and is taken from Table 5-1, pg. 200, in the textbook. The Castiglianos theorem then

    states that the displacement for any point on a machine element is the partial

    derivative of the strain energy with respective to a force which is on the same point

    and in the same direction of the displacement. In short:

    ii F

    U

    =

    where i is the displacement for an ith point in the machine element andFi is the force

    acting at the same point and in the same direction of the displacement asked for. If

    there is no force at the point for which the displacement is required, then we have to

    assume an imaginary force Q and let it be zero at the end.

    Example: Lets solve the above problem for its vertical displacement at the free end,

    i.e. at point C, using the Castiglianos theorem. So the question is to find C in the

    vertical (y) direction. We have,

    FUC=

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    where the strain energy U is contributed by the bending shear force Vand bending

    momentM, but well only consider the effect ofMin U. Thus, as given above,

    U= EI

    dxM

    2

    2

    = +L

    a

    BCa

    AB

    EI

    dxM

    EI

    dxM

    22

    2

    0

    2

    and

    +

    =L

    a

    BCBCa

    ABAB

    CEI

    dxF

    MM

    EI

    dxF

    MM

    0

    where as found before: MAB = wx2/2+(F+wa)x (FL+ wa2/2) and MBC = F(xL).

    Therefore: LxF

    MAB =

    and Lx

    F

    MBC =

    . Substituting these in the formula

    above yields:[ ]dx

    EI

    LxFdx

    EI

    LxwaFLxwaFwxL

    a

    a

    C

    ++++

    =2

    0

    22 )()(/2)()(/2 .

    which upon calculation results in

    EI

    FLaL

    EI

    waC

    3)(4

    24

    33

    += .

    This result is in agreement with the result that can be found from the two methods

    above by substitutingx=L inyBC. But remember that LxBCy = = C. Why?

    Note: Review examples 5-10, 5-11 and 5-12, pgs. 202 to 206 in the textbook.

    5.10 Statically Indeterminate Problems

    When a static problem has more unknowns than the Newtons static equations, then

    this problem is known as the statically indeterminate problem. In these cases, we need

    extra displacement equations to solve the problem. There are two procedures to

    handle such problems, among which well follow the Procedure 1 in the textbook,

    whose steps are given as follows:

    1) Choose the redundant (extra) reaction(s). This redundant reaction could bea force or a moment.

    2) Write the Newtons equations of static equilibrium in terms of the appliedloads and the redundant reaction(s) of step 1.

    3) Write the deflection or slope equation(s) for the point(s) of the redundantreaction(s) of step 1. Normally this deflection or slope will be zero.

    4) Solve the equations in steps 2 and 3 for the reactions.Note: Review example 5-14, pgs. 212 and 213 in the textbook.

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    5.12 Long Columns with Central Loading

    The long columns with central compressive loading may exhibit a phenomenon

    called buckling, which needs to be checked for the safe use of these columns. Such

    columns with 4 different end conditions are shown in the textbook in Figure 5-18, pg.

    217. The formula used for the long columns is namedEuler formula, given as:

    2cr L

    EIcP

    2

    = or2

    2

    )/( kL

    Ec

    A

    Pcr =

    where Pcr is the critical or maximum central load for the column, c is the end

    condition constant that should be taken from Table 5-2, pg. 220, in the textbook, and k

    is the radius of gyration found fromI=Ak2, which is equal to d/4 for a column having

    a solid round cross-section with a diameter ofd. L/k in the formula is known as the

    slenderness ratio. There are 2 scenarios here:

    1) If the critical load Pcr is known, then one should use the above equations tofind an adequate cross-section for the column.

    2) If the cross-section of the column is known, one can use the above equationsto solve for thePcr.

    How do we know a column is long enough or it is of intermediate length? First we

    define:1/2

    2

    1

    2

    =

    yS

    cE

    k

    L

    where Sy is the yield strength of the column material. We follow the following

    criterion:

    1) If

    k

    L>

    1

    k

    Lthen use the aboveEuler formula.

    2) If

    k

    L

    1

    k

    Lthen use theJohnson formula given below in section 5-13 for

    the intermediate-length columns.

    5.13 Intermediate-Length Columns with Central Loading

    Use theJohnson formula:

    cEk

    LSS

    A

    P yy

    cr 1

    2

    2

    =

    Note: Review examples 5-16, 5-17, 5-18 and 5-19, pgs. 223 to 225 in the textbook.